{"as_of":"2026-08-07T11:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:94163b7e45733c6b4bce14c80bbb9bd17bb03fc5a5c30b8c999b63497f1c0f9a","coverage":[{"denominator":98,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":98,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:18:40.794732Z","state":"measured"},{"denominator":99,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":99,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-27T17:53:29.423458Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-02T23:47:27.730750Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"cited_work":{"arxiv_id":"2507.06178","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.06178","snapshot_observed_at":"2026-07-02T23:47:27.730750Z","title":null,"venue":null,"work_id":"b2d43247-a0ef-4eb7-8907-9f2fbb7a3b0e","year":2025},"citing_paper":{"arxiv_id":"2606.08628","last_updated":"2026-06-07T13:45:23Z","snapshot_observed_at":"2026-08-05T17:07:38.355825Z","submitted_at":"2026-06-07T13:45:23Z","title":"Thermal emission from dark matter-heated neutron stars in the Galactic Center","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-27T17:53:29.423458Z"},"links":{"cited_paper":"/paper/2507.06178","citing_paper":"/paper/2606.08628"},"observation_digest":"sha256:7e2b60b003a8cbadc84e3a93ede655e31c8801acd6df5a027bd328d1d4303905","observation_id":"565955c3-63aa-4a80-94c7-d52c7d42aa94","resolution":{"observed_at":"2026-07-02T23:47:27.732368Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.06178/citation-record","integrity":"/paper/2507.06178/integrity","json":"/paper/2507.06178/citation-record.json","paper":"/paper/2507.06178"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0404175","last_updated":"2004-08-13T15:46:27Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2004-04-21T13:12:59Z","title":"Particle Dark Matter: Evidence, Candidates and Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0404175","snapshot_observed_at":"2026-08-06T19:18:29.340329Z","title":"Particle dark matter: Evidence, candidates and constraints,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.340329Z"},"links":{"cited_paper":"/paper/hep-ph/0404175","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:16bb77fc33d14d47e0cffdc0ac1a874bc4b6324ede4094b79808d0c38b8140e7","observation_id":"af208637-7292-425b-9f2e-c104b7e4c8e5","resolution":{"observed_at":"2026-08-06T19:18:29.340329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.03800","last_updated":"2015-07-14T10:56:14Z","snapshot_observed_at":"2026-07-06T04:23:46.562010Z","submitted_at":"2015-07-14T10:56:14Z","title":"Indirect and direct search for dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.03800","snapshot_observed_at":"2026-08-06T19:18:29.400827Z","title":"Indirect and direct search for dark matter,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.400827Z"},"links":{"cited_paper":"/paper/1507.03800","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ded3e97fbb82b7c6068686153d8e8eaffc36d059edfd86e7538a49e344441544","observation_id":"01dc1bc0-55ef-4e90-89a7-cec6e4bedcd2","resolution":{"observed_at":"2026-08-06T19:18:29.400827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.00688","last_updated":"2017-09-03T09:04:22Z","snapshot_observed_at":"2026-08-07T05:35:41.498465Z","submitted_at":"2017-09-03T09:04:22Z","title":"Current status of direct dark matter detection experiments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.00688","snapshot_observed_at":"2026-08-06T19:18:29.531301Z","title":"Current status of direct dark matter detection experiments,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.531301Z"},"links":{"cited_paper":"/paper/1709.00688","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:1ca4aa808bf9efb4a1e5cff3fbf4a46b9a67269e7a17e060ce74f202770f104e","observation_id":"2a4f8be1-4d02-4ff8-b1d3-211aab2ff134","resolution":{"observed_at":"2026-08-06T19:18:29.531301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11561","last_updated":"2020-10-07T09:46:16Z","snapshot_observed_at":"2026-08-04T16:21:30.135541Z","submitted_at":"2020-08-26T13:42:19Z","title":"Status, Challenges and Directions in Indirect Dark Matter Searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11561","snapshot_observed_at":"2026-08-06T19:18:29.630345Z","title":"Status, Challenges and Directions in Indirect Dark Matter Searches,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.630345Z"},"links":{"cited_paper":"/paper/2008.11561","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:070272a1e1fb9421ff07433653e8cf871a7b442dbe9c51fa52b59a0027d3e801","observation_id":"dd2ab8e6-ff29-4893-ad36-232c233b471e","resolution":{"observed_at":"2026-08-06T19:18:29.630345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.14435","last_updated":"2025-02-06T04:21:19Z","snapshot_observed_at":"2026-08-04T19:51:36.525243Z","submitted_at":"2023-07-26T18:11:27Z","title":"Dark matter in compact stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.14435","snapshot_observed_at":"2026-08-06T19:18:29.710740Z","title":"Dark matter in compact stars,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.710740Z"},"links":{"cited_paper":"/paper/2307.14435","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:9dfa62fcee4d6833ef25ea83502e6a46216122ae8ad4dcabcc251953cb88cd2c","observation_id":"32440c21-93b8-4be0-93c1-0ebc4052e929","resolution":{"observed_at":"2026-08-06T19:18:29.710740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606322","last_updated":"2006-06-13T18:44:59Z","snapshot_observed_at":"2026-07-07T01:01:03.854368Z","submitted_at":"2006-06-13T18:44:59Z","title":"Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0606322","snapshot_observed_at":"2026-08-06T19:18:29.860690Z","title":"Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.860690Z"},"links":{"cited_paper":"/paper/astro-ph/0606322","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:df671e1d64b410621b5bcd7560493829e9c52ce27ab57e688fa64cc788c7b76b","observation_id":"54b12d63-151c-40c4-9e19-f719c22581f9","resolution":{"observed_at":"2026-08-06T19:18:29.860690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0708.2362","last_updated":"2007-08-17T13:19:23Z","snapshot_observed_at":"2026-08-03T12:05:30.663183Z","submitted_at":"2007-08-17T13:19:23Z","title":"WIMP Annihilation and Cooling of Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0708.2362","snapshot_observed_at":"2026-08-06T19:18:29.967640Z","title":"WIMP Annihilation and Cooling of Neutron Stars,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:29.967640Z"},"links":{"cited_paper":"/paper/0708.2362","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:f642b8c8a353b84dca6602ca6b95e9affd54d8e6c712462b9f03e11b94208620","observation_id":"9b425ac7-c381-4d97-8082-5eab316f4694","resolution":{"observed_at":"2026-08-06T19:18:29.967640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.09442","last_updated":"2017-07-29T00:23:02Z","snapshot_observed_at":"2026-08-01T00:10:10.439826Z","submitted_at":"2017-07-29T00:23:02Z","title":"Neutron stars at the dark matter direct detection frontier","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.09442","snapshot_observed_at":"2026-08-06T19:18:30.158722Z","title":"Neutron stars at the dark matter direct detection frontier,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.158722Z"},"links":{"cited_paper":"/paper/1707.09442","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:e4fb42ea17dbd839c444643805ebd140be8e499fa8063ea7fd6daf1a174d5058","observation_id":"f4e1c5be-cf29-455c-ac3b-fb4e74587ab1","resolution":{"observed_at":"2026-08-06T19:18:30.158722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02840","last_updated":"2018-09-12T06:08:06Z","snapshot_observed_at":"2026-07-06T06:48:58.340685Z","submitted_at":"2018-07-08T15:42:18Z","title":"Heating up Neutron Stars with Inelastic Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.02840","snapshot_observed_at":"2026-08-06T19:18:30.347381Z","title":"Heating up Neutron Stars with Inelastic Dark Matter,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.347381Z"},"links":{"cited_paper":"/paper/1807.02840","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:416457f97b4471407b80361444af1626b482a85e6b6602e49df6dd45786a5a16","observation_id":"b034dcf5-63a5-4d80-8d9e-99ac0ef378ed","resolution":{"observed_at":"2026-08-06T19:18:30.347381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.04667","last_updated":"2020-02-19T06:32:25Z","snapshot_observed_at":"2026-08-07T03:00:58.361948Z","submitted_at":"2019-04-08T05:45:35Z","title":"Cooling Theory Faced with Old Warm Neutron Stars: Role of Non-Equilibrium Processes with Proton and Neutron Gaps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.04667","snapshot_observed_at":"2026-08-06T19:18:30.451617Z","title":"Cooling Theory Faced with Old Warm Neutron Stars: Role of Non-Equilibrium Processes with Proton and Neutron Gaps,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.451617Z"},"links":{"cited_paper":"/paper/1904.04667","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:4b990a84ea4271f673325c21236d15ca19b34699679f3b4dcbb5dde1231183bf","observation_id":"baaed140-ff6b-4098-9e34-56b76140d96d","resolution":{"observed_at":"2026-08-06T19:18:30.451617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02991","last_updated":"2019-07-04T09:46:53Z","snapshot_observed_at":"2026-07-06T07:51:09.703238Z","submitted_at":"2019-05-08T10:09:25Z","title":"Dark Matter Heating vs. Rotochemical Heating in Old Neutron Stars","version":2},"cited_work":{"arxiv_id":"1905.02991","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.02991","snapshot_observed_at":"2026-08-06T19:18:44.836742Z","title":"Dark Matter Heating vs. Rotochemical Heating in Old Neutron Stars","venue":"hep-ph","work_id":"745aedf8-efad-4dbb-beba-91245c1c9d75","year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.579376Z"},"links":{"cited_paper":"/paper/1905.02991","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:49a37f7a2a18f9259d80cb4705d18db821d3448e9b19fa45afaba3bb321e8a62","observation_id":"be290141-312c-49d0-aabe-0dc8a744212a","resolution":{"observed_at":"2026-08-06T19:18:44.928704Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.13257","last_updated":"2021-03-29T02:31:46Z","snapshot_observed_at":"2026-07-06T10:08:24.026870Z","submitted_at":"2020-10-26T00:23:26Z","title":"Improved Treatment of Dark Matter Capture in Neutron Stars II: Leptonic Targets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.13257","snapshot_observed_at":"2026-08-06T19:18:30.675674Z","title":"Improved Treatment of Dark Matter Capture in Neutron Stars II: Leptonic Targets,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.675674Z"},"links":{"cited_paper":"/paper/2010.13257","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:743735c11263ca88de775ed7a07ad20af13c977f0096caa306fae1dee92745a3","observation_id":"d9327b3e-bbe7-4538-a565-8cb197ee7118","resolution":{"observed_at":"2026-08-06T19:18:30.675674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10728","last_updated":"2020-10-04T02:13:52Z","snapshot_observed_at":"2026-07-06T09:57:54.236173Z","submitted_at":"2020-09-22T18:00:01Z","title":"Observing the thermalization of dark matter in neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10728","snapshot_observed_at":"2026-08-06T19:18:30.822167Z","title":"Observing the thermalization of dark matter in neutron stars,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.822167Z"},"links":{"cited_paper":"/paper/2009.10728","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:c1e51d1db6f5300234b8177c3e14fc11c50cfabc980acf05fbf8fe2124fa63cf","observation_id":"739c9d9e-6fee-4d09-bc88-01a05abde0c4","resolution":{"observed_at":"2026-08-06T19:18:30.822167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09539","last_updated":"2020-10-28T06:30:52Z","snapshot_observed_at":"2026-07-06T09:13:49.452689Z","submitted_at":"2020-04-20T18:00:43Z","title":"Dark Kinetic Heating of Neutron Stars from Contact Interactions with Relativistic Targets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09539","snapshot_observed_at":"2026-08-06T19:18:30.956532Z","title":"Dark kinetic heating of neutron stars from contact interactions with relativistic targets,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:30.956532Z"},"links":{"cited_paper":"/paper/2004.09539","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ddc2f9d6285455af0a0b885d8087420d6bd47e72793ffe3d43732af378714fd9","observation_id":"8f6e2443-915d-4bed-8e75-0f0529748c8d","resolution":{"observed_at":"2026-08-06T19:18:30.956532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02238","last_updated":"2022-10-09T15:29:35Z","snapshot_observed_at":"2026-08-04T01:50:17.868420Z","submitted_at":"2022-04-05T14:22:37Z","title":"Capture of Electroweak Multiplet Dark Matter in Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.02238","snapshot_observed_at":"2026-08-06T19:18:31.128723Z","title":"Capture of electroweak multiplet dark matter in neutron stars,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.128723Z"},"links":{"cited_paper":"/paper/2204.02238","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:7a83622c9062a70d07ff6d4a7da9195aaa02669d4300c8d2a0f9fb74a84b4779","observation_id":"b39d3c77-4e45-44b9-aae8-cdf054a4ac38","resolution":{"observed_at":"2026-08-06T19:18:31.128723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.01577","last_updated":"2017-04-05T18:00:00Z","snapshot_observed_at":"2026-07-06T05:36:41.783704Z","submitted_at":"2017-04-05T18:00:00Z","title":"Dark Kinetic Heating of Neutron Stars and An Infrared Window On WIMPs, SIMPs, and Pure Higgsinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.01577","snapshot_observed_at":"2026-08-06T19:18:31.279372Z","title":"Dark Kinetic Heating of Neutron Stars and An Infrared Window On WIMPs, SIMPs, and Pure Higgsinos,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.279372Z"},"links":{"cited_paper":"/paper/1704.01577","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:4682cb4b75a656e6ffeb0daa7de8c5aaf6dbf337da728b713b5949f3ac2ea48d","observation_id":"557a4a94-0994-4edc-bccf-f8128c232f7d","resolution":{"observed_at":"2026-08-06T19:18:31.279372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18472","last_updated":"2025-01-03T15:39:05Z","snapshot_observed_at":"2026-07-06T18:21:30.595036Z","submitted_at":"2024-05-28T18:00:01Z","title":"Dark Matter Catalyzed Baryon Destruction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18472","snapshot_observed_at":"2026-08-06T19:18:31.506412Z","title":"Dark Matter Catalyzed Baryon Destruction,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.506412Z"},"links":{"cited_paper":"/paper/2405.18472","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:34775634160bf945bbf14abc63a486bb5615fa66ddb178e07dfa492d10cf0aab","observation_id":"8897dcc7-e205-4215-9e1a-3bc9f30d113c","resolution":{"observed_at":"2026-08-06T19:18:31.506412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.01839","last_updated":"2024-02-02T19:00:11Z","snapshot_observed_at":"2026-07-06T17:24:37.090243Z","submitted_at":"2024-02-02T19:00:11Z","title":"Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.01839","snapshot_observed_at":"2026-08-06T19:18:31.658615Z","title":"Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.658615Z"},"links":{"cited_paper":"/paper/2402.01839","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:eb07ca83aba576dc6b361d7065d639f345928c52a61fa6db16e668e219cae24a","observation_id":"4a8ac604-0d10-40cc-a86d-874f6900981e","resolution":{"observed_at":"2026-08-06T19:18:31.658615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:31.763521Z","title":"Weakly Interacting Massive Particles and Neutron Stars,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.763521Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:29b022c21e784aefa1118579ba7e10da8ec1d7cbbbe96d1548dd914e5d047fd2","observation_id":"6e13db8a-c15f-42e4-99db-730aceb3724b","resolution":{"observed_at":"2026-08-06T19:18:31.763521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:31.872694Z","title":"Neutron stars: Graveyard of charged dark matter,","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:31.872694Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:1c0220e8f639503dc761183fb0b2a01c8a26dfa4d6d9ecf306e5e91af1030985","observation_id":"2e75735f-6a81-472d-bac0-4a912c4bb55a","resolution":{"observed_at":"2026-08-06T19:18:31.872694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.0586","last_updated":"2010-04-05T08:16:35Z","snapshot_observed_at":"2026-07-06T02:05:57.253144Z","submitted_at":"2010-04-05T08:16:35Z","title":"Can Neutron stars constrain Dark Matter?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.0586","snapshot_observed_at":"2026-08-06T19:18:32.027563Z","title":"Can Neutron stars constrain Dark Matter?,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.027563Z"},"links":{"cited_paper":"/paper/1004.0586","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:6d6e200548fc8500f8ed6d2df80de9ab4ee380e1f53167470674b54d8048a338","observation_id":"ac2875c6-72fc-41a0-b6ce-1983fb89357d","resolution":{"observed_at":"2026-08-06T19:18:32.027563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.0629","last_updated":"2010-04-05T13:32:57Z","snapshot_observed_at":"2026-07-06T02:09:03.870412Z","submitted_at":"2010-04-05T13:32:57Z","title":"Neutron Stars as Dark Matter Probes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.0629","snapshot_observed_at":"2026-08-06T19:18:32.159590Z","title":"Neutron Stars as Dark Matter Probes,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.159590Z"},"links":{"cited_paper":"/paper/1004.0629","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:fc4781da021d6741190ac1ae6fcd0990f733b7937eb1f728cfa4fdbd70ff0cc8","observation_id":"6aee4257-69a1-4227-9530-4dc4e3b91b09","resolution":{"observed_at":"2026-08-06T19:18:32.159590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.5472","last_updated":"2012-01-26T15:50:47Z","snapshot_observed_at":"2026-08-04T20:11:11.369375Z","submitted_at":"2011-03-28T20:11:07Z","title":"Constraints on Scalar Asymmetric Dark Matter from Black Hole Formation in Neutron Stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.5472","snapshot_observed_at":"2026-08-06T19:18:32.282921Z","title":"Constraints on Scalar Asymmetric Dark Matter from Black Hole Formation in Neutron Stars,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.282921Z"},"links":{"cited_paper":"/paper/1103.5472","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:5ef11b124cfda409c589725a7113caeaa653fc61e68ec6fa6941d9d6897f41aa","observation_id":"d48c8ed2-096d-4636-b972-32b662cf0fe6","resolution":{"observed_at":"2026-08-06T19:18:32.282921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1031","last_updated":"2014-10-27T21:34:06Z","snapshot_observed_at":"2026-07-06T03:42:51.880836Z","submitted_at":"2014-05-05T20:00:00Z","title":"Detecting Dark Matter with Imploding Pulsars in the Galactic Center","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1031","snapshot_observed_at":"2026-08-06T19:18:32.396391Z","title":"Detecting Dark Matter with Imploding Pulsars in the Galactic Center,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.396391Z"},"links":{"cited_paper":"/paper/1405.1031","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:717360989669b2a800ca775c20d83c686879e3c5559a31fcf43152bbbb9a606a","observation_id":"9abc4c63-cca4-42d7-861d-985ffc415a5c","resolution":{"observed_at":"2026-08-06T19:18:32.396391Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.08773","last_updated":"2018-12-20T18:54:18Z","snapshot_observed_at":"2026-07-06T07:22:41.644418Z","submitted_at":"2018-12-20T18:54:18Z","title":"New Analysis of Neutron Star Constraints on Asymmetric Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.08773","snapshot_observed_at":"2026-08-06T19:18:32.526449Z","title":"New Analysis of Neutron Star Constraints on Asymmetric Dark Matter,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.526449Z"},"links":{"cited_paper":"/paper/1812.08773","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:e9a192a261b1acb651d8f556107c21b003d04872fff15fbc8abdd0250e366992","observation_id":"8387c5ed-ddb6-47b5-9916-4ff95a569778","resolution":{"observed_at":"2026-08-06T19:18:32.526449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.3509","last_updated":"2014-05-28T20:03:09Z","snapshot_observed_at":"2026-08-01T22:21:28.483871Z","submitted_at":"2013-10-13T20:00:11Z","title":"Bounds on self-interacting fermion dark matter from observations of old neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.3509","snapshot_observed_at":"2026-08-06T19:18:32.637256Z","title":"Bounds on self-interacting fermion dark matter from observations of old neutron stars,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.637256Z"},"links":{"cited_paper":"/paper/1310.3509","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:691480e4941d1a8d5e68bb4f2cd8206507c43c0663656b5d9fed07c653b4abb3","observation_id":"fafca788-01fb-42e2-9fa8-873538b06abf","resolution":{"observed_at":"2026-08-06T19:18:32.637256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0036","last_updated":"2013-03-20T20:00:01Z","snapshot_observed_at":"2026-07-06T03:03:05.619333Z","submitted_at":"2013-01-01T01:38:40Z","title":"Constraints on Bosonic Dark Matter From Observations of Old Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0036","snapshot_observed_at":"2026-08-06T19:18:32.730337Z","title":"Constraints on bosonic dark matter from observation of old neutron stars,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.730337Z"},"links":{"cited_paper":"/paper/1301.0036","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:47b393135ac359dfad39b83d70d5ffbcbf08a35fcfdda8f3d49d8ca6f55b3258","observation_id":"88cf0fd3-14e9-490f-9b69-62c469b97fba","resolution":{"observed_at":"2026-08-06T19:18:32.730337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.6811","last_updated":"2013-06-11T09:29:29Z","snapshot_observed_at":"2026-07-06T03:05:06.660056Z","submitted_at":"2013-01-29T00:26:32Z","title":"Realistic neutron star constraints on bosonic asymmetric dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.6811","snapshot_observed_at":"2026-08-06T19:18:32.869545Z","title":"Realistic neutron star constraints on bosonic asymmetric dark matter,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:32.869545Z"},"links":{"cited_paper":"/paper/1301.6811","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:daede62eb6f4eb54401442bfd24d6c9c167cd89fbf6f0af1b9e10f4f4877e817","observation_id":"3536b056-ba71-4b0f-82f1-846975fe3a6c","resolution":{"observed_at":"2026-08-06T19:18:32.869545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2400","last_updated":"2014-04-09T05:11:29Z","snapshot_observed_at":"2026-08-03T01:16:04.239885Z","submitted_at":"2012-01-11T20:38:51Z","title":"On the capture of dark matter by neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2400","snapshot_observed_at":"2026-08-06T19:18:33.025895Z","title":"On the capture of dark matter by neutron stars,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.025895Z"},"links":{"cited_paper":"/paper/1201.2400","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:91a3805471be3dc8d947f1f8849ccc7045ca391f55a8b13d15389454b6be1aad","observation_id":"49a4142c-87ce-412b-9e15-6c13ce3514f0","resolution":{"observed_at":"2026-08-06T19:18:33.025895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06740","last_updated":"2018-04-17T11:51:37Z","snapshot_observed_at":"2026-07-06T06:34:07.685856Z","submitted_at":"2018-04-17T11:51:37Z","title":"Non-Primordial Solar Mass Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.06740","snapshot_observed_at":"2026-08-06T19:18:33.176511Z","title":"NonPrimordial Solar Mass Black Holes,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.176511Z"},"links":{"cited_paper":"/paper/1804.06740","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ee3e32bccf0c767e41a03b9aec1663af79fe132544ae0928182963b1d08e4774","observation_id":"14969c7d-82c2-449a-8011-efe08e332aae","resolution":{"observed_at":"2026-08-06T19:18:33.176511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.05312","last_updated":"2020-07-14T02:42:25Z","snapshot_observed_at":"2026-07-06T09:11:36.787270Z","submitted_at":"2020-04-11T05:35:01Z","title":"Analysis on the black hole formations inside old neutron stars by isospin-violating dark matter with self-interaction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.05312","snapshot_observed_at":"2026-08-06T19:18:33.312723Z","title":"Analysis on the black hole formations inside old neutron stars by isospin-violating dark matter with self-interaction,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.312723Z"},"links":{"cited_paper":"/paper/2004.05312","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:d7b86a4c6100f1073f94d46634015b64656d37b5b12db1d10daf5e6255b64d13","observation_id":"118b14dc-5c12-4236-94fc-286dd06da0ac","resolution":{"observed_at":"2026-08-06T19:18:33.312723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09716","last_updated":"2022-03-17T10:42:08Z","snapshot_observed_at":"2026-07-06T12:20:05.607892Z","submitted_at":"2021-12-17T19:00:07Z","title":"Solar mass black holes from neutron stars and bosonic dark matter","version":2},"cited_work":{"arxiv_id":"2112.09716","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.09716","snapshot_observed_at":"2026-08-06T19:18:44.431595Z","title":"Solar mass black holes from neutron stars and bosonic dark matter","venue":"hep-ph","work_id":"e266f8fe-9560-42c5-808a-a78ce48d1c47","year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.432858Z"},"links":{"cited_paper":"/paper/2112.09716","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:25f1949bbb9d78e7499b36459eff795a7d5a4566e05893eb31b0c879f89a17b7","observation_id":"f065123b-d7fd-4f16-9a32-53746d666b30","resolution":{"observed_at":"2026-08-06T19:18:44.556448Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.15739","last_updated":"2022-10-27T19:40:26Z","snapshot_observed_at":"2026-08-02T13:23:22.132133Z","submitted_at":"2022-10-27T19:40:26Z","title":"Constraining properties of asymmetric dark matter candidates from gravitational-wave observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.15739","snapshot_observed_at":"2026-08-06T19:18:33.541661Z","title":"Constraining properties of asymmetric dark matter candidates from gravitational-wave observations,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.541661Z"},"links":{"cited_paper":"/paper/2210.15739","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:dc2ede6df6de16baaad9cce882c3cfb0924778879d57e93f8d68cf25452372f0","observation_id":"a4074b35-0f55-472a-bbea-e417842e156e","resolution":{"observed_at":"2026-08-06T19:18:33.541661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-02T20:25:05.492372Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-06T19:18:33.624680Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.624680Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:23094963d6dc17199ee4928e4e997821d74b4f8217f26d3f0e81fc28a3345466","observation_id":"6345e454-b680-4718-98f5-13b2359bafab","resolution":{"observed_at":"2026-08-06T19:18:33.624680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.15144","last_updated":"2025-02-11T15:48:11Z","snapshot_observed_at":"2026-08-01T14:25:03.048442Z","submitted_at":"2024-02-23T07:00:40Z","title":"Polarization Signals from Axion-Photon Resonant Conversion in Neutron Star Magnetosphere","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.15144","snapshot_observed_at":"2026-08-06T19:18:33.762512Z","title":"Polarization signals from axion-photon resonant conversion in a neutron star magnetosphere,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.762512Z"},"links":{"cited_paper":"/paper/2402.15144","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:61aecd97674069fc99a27d8ef8425ce58902dc19f505ac562f78f6a24c4afabd","observation_id":"e59e1bfe-998c-404c-a1ab-435981283216","resolution":{"observed_at":"2026-08-06T19:18:33.762512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.02492","last_updated":"2025-02-26T20:20:46Z","snapshot_observed_at":"2026-08-04T16:22:06.374881Z","submitted_at":"2024-11-04T19:00:01Z","title":"Axion Astrophysics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.02492","snapshot_observed_at":"2026-08-06T19:18:33.848553Z","title":"Axion astrophysics,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.848553Z"},"links":{"cited_paper":"/paper/2411.02492","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:4bc7353b8eca4c11154cd4bcb16140189732dd4cddd94d062a78cb28fe23f955","observation_id":"b1a37302-fd1c-4c5e-9b3e-d0ea679df467","resolution":{"observed_at":"2026-08-06T19:18:33.848553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.13728","last_updated":"2024-03-12T17:38:28Z","snapshot_observed_at":"2026-08-03T18:36:38.003151Z","submitted_at":"2024-01-24T19:00:00Z","title":"Astrophysical Axion Bounds: The 2024 Edition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.13728","snapshot_observed_at":"2026-08-06T19:18:33.975257Z","title":"Astrophysical Axion Bounds: The 2024 Edition,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.975257Z"},"links":{"cited_paper":"/paper/2401.13728","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:22c390ed3f5f128ef5c46871e36a36ef8936db1d6b309ff69e5c03254d3bdc20","observation_id":"20b0ba40-c496-4da4-a270-bb87bbcd9ab9","resolution":{"observed_at":"2026-08-06T19:18:33.975257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20450","last_updated":"2025-05-26T18:43:50Z","snapshot_observed_at":"2026-07-06T21:30:57.177648Z","submitted_at":"2025-05-26T18:43:50Z","title":"Searching for Axion Dark Matter Near Relaxing Magnetars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20450","snapshot_observed_at":"2026-08-06T19:18:34.123893Z","title":"Searching for Axion Dark Matter Near Relaxing Magnetars,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.123893Z"},"links":{"cited_paper":"/paper/2505.20450","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:85027f471eb2c57f67d7307d24b52625a3a08c6dd089abc756b9132236a73e04","observation_id":"812fb56a-7844-4281-b16b-afb70be28b82","resolution":{"observed_at":"2026-08-06T19:18:34.123893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02875","last_updated":"2021-10-06T16:02:06Z","snapshot_observed_at":"2026-07-06T11:55:04.054344Z","submitted_at":"2021-10-06T16:02:06Z","title":"Dark photon limits from magnetic fields and astrophysical plasmas","version":1},"cited_work":{"arxiv_id":"2110.02875","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.02875","snapshot_observed_at":"2026-08-06T19:18:44.034639Z","title":"Dark photon limits from magnetic fields and astrophysical plasmas","venue":"hep-ph","work_id":"cb913acd-ed60-488f-b09d-05f5eb8864c8","year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.245832Z"},"links":{"cited_paper":"/paper/2110.02875","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:9038bfdb2cb299ad5b5aaefe3318af7083f6e2ab5d976e226cd8ee6ee4ab3d09","observation_id":"84730950-a645-405e-accf-10ba13cd6076","resolution":{"observed_at":"2026-08-06T19:18:44.227788Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06746","last_updated":"2024-07-30T06:57:36Z","snapshot_observed_at":"2026-07-06T17:00:04.276081Z","submitted_at":"2023-12-11T19:00:00Z","title":"Constraints on photon mass and dark photon from the Jovian magnetic field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06746","snapshot_observed_at":"2026-08-06T19:18:34.373755Z","title":"Constraints on photon mass and dark photon from the Jovian magnetic field,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.373755Z"},"links":{"cited_paper":"/paper/2312.06746","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:5c860fd980d97f2d796b18e32a78eee4d7c1b09e69bb81472c7ac10a2708c113","observation_id":"df8c03ce-a726-4426-884a-ab8ffbe65cbe","resolution":{"observed_at":"2026-08-06T19:18:34.373755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.11575","last_updated":"2023-10-03T17:21:38Z","snapshot_observed_at":"2026-07-06T15:44:38.851931Z","submitted_at":"2023-06-20T14:43:43Z","title":"A Hunt for Magnetic Signatures of Hidden-Photon and Axion Dark Matter in the Wilderness","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.11575","snapshot_observed_at":"2026-08-06T19:18:34.502517Z","title":"Hunt for magnetic signatures of hidden-photon and axion dark matter in the wilderness,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.502517Z"},"links":{"cited_paper":"/paper/2306.11575","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:9522648d32b4b48bd02fd75f9090055e2aa8f0d4e56553275c3a2d2651276a53","observation_id":"e1b9d09b-12d1-42fc-a56c-688c0a1787b9","resolution":{"observed_at":"2026-08-06T19:18:34.502517Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.09630","last_updated":"2025-04-13T15:57:38Z","snapshot_observed_at":"2026-07-06T21:08:37.884789Z","submitted_at":"2025-04-13T15:57:38Z","title":"Probing Millicharged Dark Matter with Magnetometer Coupled to Circuit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.09630","snapshot_observed_at":"2026-08-06T19:18:34.625942Z","title":"Probing Millicharged Dark Matter with Magnetometer Coupled to Circuit,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.625942Z"},"links":{"cited_paper":"/paper/2504.09630","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:90d0813d1b0ac1a0e1490fa8d6b0557d191bf30498a0949019d716d0f9c6ef13","observation_id":"781654b8-fd3d-4e0b-87ef-42b0a5947ac7","resolution":{"observed_at":"2026-08-06T19:18:34.625942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:34.715559Z","title":"Geomagnetic Signal of Millicharged Dark Matter,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.715559Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:31769c25e2bfa2f017cb9eed702ebb420220f39d15f875350bec84fcb1e55c7d","observation_id":"887fdce2-2306-483f-adb8-4e5890d8906a","resolution":{"observed_at":"2026-08-06T19:18:34.715559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1485","last_updated":"2007-11-15T16:57:21Z","snapshot_observed_at":"2026-07-06T01:29:48.927183Z","submitted_at":"2007-09-10T21:10:33Z","title":"Compact Stars as Dark Matter Probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.1485","snapshot_observed_at":"2026-08-06T19:18:34.817738Z","title":"Compact Stars as Dark Matter Probes,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.817738Z"},"links":{"cited_paper":"/paper/0709.1485","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:2938545f7674f7dfc1d00c6a901308d98875306d5cec66093ae19bcee1352568","observation_id":"cd851867-5ae4-440d-88ac-e757cefa8323","resolution":{"observed_at":"2026-08-06T19:18:34.817738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.2039","last_updated":"2010-12-09T15:55:16Z","snapshot_observed_at":"2026-07-06T02:20:27.142343Z","submitted_at":"2010-12-09T15:55:16Z","title":"Constraining Asymmetric Dark Matter through observations of compact stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.2039","snapshot_observed_at":"2026-08-06T19:18:34.923797Z","title":"Constraining Asymmetric Dark Matter through observations of compact stars,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:34.923797Z"},"links":{"cited_paper":"/paper/1012.2039","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:14b16c45d01e03493fc12dd2c98e7dece5df073241d3dcb0db09b41b5ef7ba2f","observation_id":"add1ff88-45a1-4f91-8f6e-5b2fde5a7ef9","resolution":{"observed_at":"2026-08-06T19:18:34.923797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:35.064774Z","title":"Dark-matter admixed neutron stars,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.064774Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:bcd7d8cf8acf64d2e946997752a5ec79f97e475151773814fc0d2d2c6a093f0e","observation_id":"9ad12896-ee10-4312-9612-de718ff098a3","resolution":{"observed_at":"2026-08-06T19:18:35.064774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.08254","last_updated":"2018-09-21T18:00:56Z","snapshot_observed_at":"2026-08-01T08:25:32.090914Z","submitted_at":"2018-09-21T18:00:56Z","title":"Asymmetric Dark Stars and Neutron Star Stability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.08254","snapshot_observed_at":"2026-08-06T19:18:35.255248Z","title":"Asymmetric Dark Stars and Neutron Star Stability,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.255248Z"},"links":{"cited_paper":"/paper/1809.08254","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:f1e1eb0b2c94c513871e5210332835ea66a275eee5d2a3abfa46bc33f7d0155a","observation_id":"8001db8d-af49-4741-8726-a02e34cbf5a6","resolution":{"observed_at":"2026-08-06T19:18:35.255248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.01183","last_updated":"2019-03-04T11:36:14Z","snapshot_observed_at":"2026-07-06T07:36:50.580026Z","submitted_at":"2019-03-04T11:36:14Z","title":"Dark compact objects: an extensive overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.01183","snapshot_observed_at":"2026-08-06T19:18:35.362877Z","title":"Dark compact objects: an extensive overview,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.362877Z"},"links":{"cited_paper":"/paper/1903.01183","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:967e946bbdd8281d457814f3112624fc53ffa04120845cecc173ee4edce5e892","observation_id":"3ea4914b-5dab-433d-b8c7-992087cc97f0","resolution":{"observed_at":"2026-08-06T19:18:35.362877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.11993","last_updated":"2019-11-26T18:42:56Z","snapshot_observed_at":"2026-08-05T13:38:29.250444Z","submitted_at":"2019-04-26T18:00:04Z","title":"Supernovae Sparked By Dark Matter in White Dwarfs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.11993","snapshot_observed_at":"2026-08-06T19:18:35.466720Z","title":"Supernovae Sparked By Dark Matter in White Dwarfs,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.466720Z"},"links":{"cited_paper":"/paper/1904.11993","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:1a36b9d4957e89b488a79b47441509e0bfae2b92eebd6bb4ab3d2b404c87efda","observation_id":"a7ee222d-8a08-4671-add3-c9e8285e2ae4","resolution":{"observed_at":"2026-08-06T19:18:35.466720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.01825","last_updated":"2021-04-08T16:33:30Z","snapshot_observed_at":"2026-08-06T08:22:51.391593Z","submitted_at":"2020-09-03T17:44:19Z","title":"Low Mass Black Holes from Dark Core Collapse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.01825","snapshot_observed_at":"2026-08-06T19:18:35.630244Z","title":"Low Mass Black Holes from Dark Core Collapse,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.630244Z"},"links":{"cited_paper":"/paper/2009.01825","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:430db79aa2de62ffb545ee685ca1e6f37d72c396b0bfe44a33c79254ff8c099e","observation_id":"69cc5d87-0ede-41e5-aec1-72c3a598a236","resolution":{"observed_at":"2026-08-06T19:18:35.630244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:35.755922Z","title":"Dark matter capture in celestial objects: light mediators, self-interactions, and complementarity with direct detection,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.755922Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:97a5e835aa1e15ee31f1b716ac92e26d4ac514f05f4103b43d033cff0ab8bdac","observation_id":"f6a47796-fe4e-4464-a312-ecf988dd7f51","resolution":{"observed_at":"2026-08-06T19:18:35.755922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.08257","last_updated":"2021-11-08T17:37:40Z","snapshot_observed_at":"2026-08-06T05:53:10.628675Z","submitted_at":"2021-02-16T16:28:14Z","title":"Dark matter admixed neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.08257","snapshot_observed_at":"2026-08-06T19:18:35.880718Z","title":"Dark matter admixed neutron stars,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.880718Z"},"links":{"cited_paper":"/paper/2102.08257","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:9ad5e06760a45caacdfa666d7bdee8f65b5ebd144a4b2d9d82ec210ecdb72dbb","observation_id":"bb46ad53-c6a0-43b9-a1b2-b6eb3b6fa49e","resolution":{"observed_at":"2026-08-06T19:18:35.880718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01812","last_updated":"2023-09-13T15:13:42Z","snapshot_observed_at":"2026-07-30T20:46:51.706607Z","submitted_at":"2022-10-04T18:00:01Z","title":"Light Dark Matter Accumulating in Planets: Nuclear Scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01812","snapshot_observed_at":"2026-08-06T19:18:35.983619Z","title":"Light dark matter accumulating in planets: Nuclear scattering,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.983619Z"},"links":{"cited_paper":"/paper/2210.01812","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:3cef8f5e9ef44615166691c23c6c1fe1630c92250fb4e642782e274da6705eb5","observation_id":"55b03a63-fe32-4c1b-89b0-3c7b6cbb970f","resolution":{"observed_at":"2026-08-06T19:18:35.983619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.12547","last_updated":"2023-06-15T11:10:13Z","snapshot_observed_at":"2026-07-06T14:34:34.451413Z","submitted_at":"2022-12-23T19:00:03Z","title":"Bounds on Long-lived Dark Matter Mediators from Neutron Stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.12547","snapshot_observed_at":"2026-08-06T19:18:36.080018Z","title":"Bounds on long-lived dark matter mediators from neutron stars,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.080018Z"},"links":{"cited_paper":"/paper/2212.12547","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:046d267668be5e6924af165b2412b680121ea725d39f0ec954411d462aff1468","observation_id":"ff2a67a5-d34e-4c42-a30f-bf9e01f8db49","resolution":{"observed_at":"2026-08-06T19:18:36.080018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.02221","last_updated":"2022-07-05T18:00:00Z","snapshot_observed_at":"2026-07-06T13:28:05.405493Z","submitted_at":"2022-07-05T18:00:00Z","title":"Neutron star observations of pseudoscalar-mediated dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.02221","snapshot_observed_at":"2026-08-06T19:18:36.196082Z","title":"Neutron star observations of pseudoscalar-mediated dark matter,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.196082Z"},"links":{"cited_paper":"/paper/2207.02221","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:d5f693bb7282f8630dae7be92fb6769d088a4fa2a8a424266f8d266d7dae025a","observation_id":"4b2988e6-eeed-44d4-9f86-710c518dd8b1","resolution":{"observed_at":"2026-08-06T19:18:36.196082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03625","last_updated":"2023-04-07T14:26:16Z","snapshot_observed_at":"2026-08-05T06:25:05.310427Z","submitted_at":"2023-01-09T19:00:14Z","title":"Celestial Objects as Strongly-Interacting Non-Annihilating Dark Matter Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03625","snapshot_observed_at":"2026-08-06T19:18:36.269461Z","title":"Celestial objects as strongly-interacting nonannihilating dark matter detectors,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.269461Z"},"links":{"cited_paper":"/paper/2301.03625","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:d8125821fdd319c3bb2329c1079c4cfff996a97c2df0dbfb2b168b4ea175891a","observation_id":"955a4740-43b4-446f-adc0-f14dc372435c","resolution":{"observed_at":"2026-08-06T19:18:36.269461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.07898","last_updated":"2023-08-30T19:47:18Z","snapshot_observed_at":"2026-08-05T16:38:43.851096Z","submitted_at":"2023-02-15T19:00:02Z","title":"Can LIGO Detect Non-Annihilating Dark Matter?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.07898","snapshot_observed_at":"2026-08-06T19:18:36.360990Z","title":"Can LIGO Detect Nonannihilating Dark Matter?,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.360990Z"},"links":{"cited_paper":"/paper/2302.07898","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:cf23d336e161ec25aead41919135fa61e2b805b2fe12762dedebc4c7f5635597","observation_id":"9ada18f4-5934-4ef6-8aee-dd1241340000","resolution":{"observed_at":"2026-08-06T19:18:36.360990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04931","last_updated":"2024-01-17T04:49:10Z","snapshot_observed_at":"2026-07-06T17:13:33.874642Z","submitted_at":"2024-01-10T05:01:03Z","title":"Possible Dark Matter Signals from White Dwarfs","version":2},"cited_work":{"arxiv_id":"2401.04931","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.04931","snapshot_observed_at":"2026-08-06T19:18:43.572360Z","title":"Possible Dark Matter Signals from White Dwarfs","venue":"hep-ph","work_id":"6c852a8b-9c53-45a3-b7e5-815a6e886851","year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.464078Z"},"links":{"cited_paper":"/paper/2401.04931","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:6cc8b704d2260dbb13bcfcd7e116bb69f9dc7b3bf25a2158659cda2ace042827","observation_id":"028520f7-b94f-4def-b70c-289b2e90afcc","resolution":{"observed_at":"2026-08-06T19:18:43.701502Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.09772","last_updated":"2023-04-21T13:39:25Z","snapshot_observed_at":"2026-08-04T06:11:19.950217Z","submitted_at":"2022-12-19T19:00:02Z","title":"Dark photon superradiance: Electrodynamics and multimessenger signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.09772","snapshot_observed_at":"2026-08-06T19:18:36.558310Z","title":"Dark photon superradiance: Electrodynamics and multimessenger signals,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.558310Z"},"links":{"cited_paper":"/paper/2212.09772","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:0e33d4b9533671bce9537c5d362792eb0e4a0df5a0ba00ba6c8a0bb60fcf9ee3","observation_id":"5e1d51b1-cad3-4d70-ae83-ac44e5a6a2df","resolution":{"observed_at":"2026-08-06T19:18:36.558310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.09219","last_updated":"2025-09-02T11:42:34Z","snapshot_observed_at":"2026-07-06T21:23:42.895337Z","submitted_at":"2025-05-14T08:40:19Z","title":"Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers","version":2},"cited_work":{"arxiv_id":"2505.09219","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.09219","snapshot_observed_at":"2026-08-06T19:18:43.275159Z","title":"Probing Self-Interacting Dark Matter via Gravitational-Wave Background from Eccentric Supermassive Black Hole Mergers","venue":"astro-ph.GA","work_id":"503c329c-a586-46e5-b442-ba6cf592ea06","year":2025},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.678033Z"},"links":{"cited_paper":"/paper/2505.09219","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:7946d3f2268e6bb224ba224272a50673bbd0c60afd8963229cb7cad10dda9c37","observation_id":"417b7035-abda-4c1d-9986-8487d2ab87a2","resolution":{"observed_at":"2026-08-06T19:18:43.374261Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.14450","last_updated":"2024-06-03T17:26:27Z","snapshot_observed_at":"2026-07-06T17:20:37.280501Z","submitted_at":"2024-01-25T19:00:00Z","title":"Self-interacting dark matter solves the final parsec problem of supermassive black hole mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.14450","snapshot_observed_at":"2026-08-06T19:18:36.830457Z","title":"Self-Interacting Dark Matter Solves the Final Parsec Problem of Supermassive Black Hole Mergers,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.830457Z"},"links":{"cited_paper":"/paper/2401.14450","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:b058d3d76345e757ad32e42fb42e1919c7940c3bb701b223f3c4c2e29ae21e9c","observation_id":"01637c2e-6bfa-44e9-a7ca-b89e2b3b3e46","resolution":{"observed_at":"2026-08-06T19:18:36.830457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.09696","last_updated":"2025-08-13T05:26:12Z","snapshot_observed_at":"2026-07-06T21:24:01.607451Z","submitted_at":"2025-05-14T18:00:34Z","title":"Dark Matter-Independent Orbital Decay Bounds on Ultralight Bosons from OJ287","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.09696","snapshot_observed_at":"2026-08-06T19:18:36.958303Z","title":"Superradiant Bosons Driving Supermassive Black Hole Mergers,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:36.958303Z"},"links":{"cited_paper":"/paper/2505.09696","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:c4bfd04ab7084b29de9967bec99f8d1509b1c1e9848d35d9a5810521068365b1","observation_id":"79eadb47-5d8d-486b-8805-ac48b5542f46","resolution":{"observed_at":"2026-08-06T19:18:36.958303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.080969Z","title":"Probing Boson Clouds with Supermassive Black Hole Binaries,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.080969Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:56318d5bf457fb907278e2998b2039e7afe582a85af64fcdceb03d38048a7027","observation_id":"8d8584dd-028b-41e1-90a0-ba17435d25b9","resolution":{"observed_at":"2026-08-06T19:18:37.080969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.08824","last_updated":"2023-09-10T12:06:45Z","snapshot_observed_at":"2026-08-04T23:00:52.348394Z","submitted_at":"2023-04-18T08:43:22Z","title":"A Dark Matter Probe in Accreting Pulsar-Black Hole Binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.08824","snapshot_observed_at":"2026-08-06T19:18:37.175656Z","title":"A dark matter probe in accreting pulsar-black hole binaries,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.175656Z"},"links":{"cited_paper":"/paper/2304.08824","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:0b3e9ae338939ef3197e7e10d17eca80c1629b8372bee4cd92a1db15f955e8e9","observation_id":"32cff2d5-0465-4b8d-8df7-0d0209e2e94a","resolution":{"observed_at":"2026-08-06T19:18:37.175656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10316","last_updated":"2019-07-10T19:52:09Z","snapshot_observed_at":"2026-08-03T01:18:09.709575Z","submitted_at":"2019-06-25T04:15:55Z","title":"Constraining light fermionic dark matter with binary pulsars","version":2},"cited_work":{"arxiv_id":"1906.10316","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.10316","snapshot_observed_at":"2026-08-06T19:18:43.031690Z","title":"Constraining light fermionic dark matter with binary pulsars","venue":"astro-ph.GA","work_id":"19ba57d9-09bc-413a-b12c-a4a9c4d8988a","year":2019},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.284031Z"},"links":{"cited_paper":"/paper/1906.10316","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:bde990e5dda52c3ed97b2e7e109566b3397ebe7d4cd6ed317f9594f52c4f44b7","observation_id":"d4293c2b-0028-431d-84e6-8d5d0b6fe7b6","resolution":{"observed_at":"2026-08-06T19:18:43.104342Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.392638Z","title":"Gravitational radiation from point masses in a Keplerian orbit,","venue":null,"work_id":null,"year":1963},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.392638Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:8aa92346fb7e3ae238b2f35929d5ce998d4be411f9e5de9e4b47a7093af15b29","observation_id":"c0875b26-42cb-474e-bd58-776d2c01ff82","resolution":{"observed_at":"2026-08-06T19:18:37.392638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.535435Z","title":"Gravitational Radiation and the Motion of Two Point Masses,","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.535435Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:1224f26a41a802b003d8ad84cf464998914531773a1fccbb2b53ef6244b81454","observation_id":"44485f71-f8f9-4223-ab14-0acf45d7a84b","resolution":{"observed_at":"2026-08-06T19:18:37.535435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.697481Z","title":"Higher order gravitational radiation losses in binary systems,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.697481Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:83a7e928e7a6255ea06633849aa048ed484eca19c9acdb9653ba1a12f4662cdd","observation_id":"1a27cb67-3350-4d18-af0c-17be0a008e1b","resolution":{"observed_at":"2026-08-06T19:18:37.697481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.793666Z","title":"Maggiore, Gravitational Waves","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.793666Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:0d34cac39c1d8bf91194b80b4400f3d708de1a0aa981939b640e5c9b17b2d9b6","observation_id":"cd692a29-3940-4158-86dd-1966f1b4d395","resolution":{"observed_at":"2026-08-06T19:18:37.793666Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:37.905471Z","title":"Discovery of a pulsar in a binary system,","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:37.905471Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:80363b1338c08856fdf744134b9f2ba8a7710a8b341b6a3eddc02f06f1ff602e","observation_id":"3de7eb83-066e-4816-b1e1-7a8821bfbea7","resolution":{"observed_at":"2026-08-06T19:18:37.905471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9804325","last_updated":"1998-04-29T17:45:31Z","snapshot_observed_at":"2026-07-07T01:20:40.325068Z","submitted_at":"1998-04-29T17:45:31Z","title":"Gravitational Radiation and Rotation of Accreting Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9804325","snapshot_observed_at":"2026-08-06T19:18:38.006253Z","title":"Gravitational radiation and rotation of accreting neutron stars,","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.006253Z"},"links":{"cited_paper":"/paper/astro-ph/9804325","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ede61dd6e5c80155e3a003967dfde9fe8f8bf3b9bd4221a1aaf08f1c989e4a68","observation_id":"5e5bab52-50e8-4c0b-a978-63df2c318c78","resolution":{"observed_at":"2026-08-06T19:18:38.006253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:38.134082Z","title":"Capture by the sun of a galactic population of weakly interacting, massive particles,","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.134082Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:bc5cad0cbc579d841b7f174a309275ed8e74133c17835a9e4154fe341b947db6","observation_id":"070234d7-14af-48fa-915d-843afeb492e8","resolution":{"observed_at":"2026-08-06T19:18:38.134082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:18:38.211724Z","title":"Resonant Enhancements in Weakly Interacting Massive Particle Capture by the Earth,","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.211724Z"},"links":{"citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:c84bda4767b59b06b9e5717a26eefa032885428ae3a875a2b3721225a85a6f5a","observation_id":"2bdfa67b-d85a-4df8-980b-95e34f786997","resolution":{"observed_at":"2026-08-06T19:18:38.211724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08918","last_updated":"2022-11-30T19:13:36Z","snapshot_observed_at":"2026-08-07T04:22:53.725938Z","submitted_at":"2020-12-16T13:07:00Z","title":"Nucleon Structure and Strong Interactions in Dark Matter Capture in Neutron Stars","version":3},"cited_work":{"arxiv_id":"2012.08918","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.08918","snapshot_observed_at":"2026-08-06T19:18:42.849808Z","title":"Nucleon Structure and Strong Interactions in Dark Matter Capture in Neutron Stars","venue":"hep-ph","work_id":"b5c020aa-d2c0-4247-ac06-d3d5ad272d03","year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.279407Z"},"links":{"cited_paper":"/paper/2012.08918","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:002cd40ffa3c6b2f071e552c30fe422364b55275c186d7ee52affdb1dbd53594","observation_id":"4a32f7c8-6222-4f32-9598-81f1b4d06061","resolution":{"observed_at":"2026-08-06T19:18:42.940245Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.08478","last_updated":"2022-12-16T13:45:38Z","snapshot_observed_at":"2026-07-06T14:31:42.631932Z","submitted_at":"2022-12-16T13:45:38Z","title":"Improved Treatment of Dark Matter Capture in Compact Stars","version":1},"cited_work":{"arxiv_id":"2212.08478","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.08478","snapshot_observed_at":"2026-08-06T19:18:42.662248Z","title":"Improved Treatment of Dark Matter Capture in Compact Stars","venue":"hep-ph","work_id":"ee6df213-2a54-4f63-8ad3-c08a1b93acac","year":2022},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.348159Z"},"links":{"cited_paper":"/paper/2212.08478","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:02d2136416ed531192f9d5eaa4678930092276af02c6c09da58fb6c83b3adf94","observation_id":"fcfc0f47-e1a0-4c50-a651-317a316ab1ba","resolution":{"observed_at":"2026-08-06T19:18:42.744271Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.11892","last_updated":"2024-04-03T18:59:02Z","snapshot_observed_at":"2026-07-06T17:05:06.923713Z","submitted_at":"2023-12-19T06:35:19Z","title":"Thermalization and Annihilation of Dark Matter in Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.11892","snapshot_observed_at":"2026-08-06T19:18:38.448418Z","title":"Thermalization and Annihilation of Dark Matter in Neutron Stars,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.448418Z"},"links":{"cited_paper":"/paper/2312.11892","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:684351bb8961cc3a1df7679403760852dbaf728becb53fdcebd104befa71927b","observation_id":"8f398735-077e-4a66-b840-936f4e52819f","resolution":{"observed_at":"2026-08-06T19:18:38.448418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.04043","last_updated":"2020-06-18T19:40:59Z","snapshot_observed_at":"2026-08-06T01:14:02.176942Z","submitted_at":"2017-03-11T23:32:22Z","title":"Multiscatter stellar capture of dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.04043","snapshot_observed_at":"2026-08-06T19:18:38.565892Z","title":"Multiscatter stellar capture of dark matter,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.565892Z"},"links":{"cited_paper":"/paper/1703.04043","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:14f01d9ed0122cb0e22c9b07650f7bc8ab10f516c8f4921fad5fd3d0d3116d64","observation_id":"cae39962-92af-4f29-b2e9-a5360d4d9212","resolution":{"observed_at":"2026-08-06T19:18:38.565892Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.09054","last_updated":"2022-04-23T13:16:03Z","snapshot_observed_at":"2026-08-03T17:58:01.664142Z","submitted_at":"2022-03-17T03:19:44Z","title":"Revisiting constraints on asymmetric dark matter from collapse in white dwarf stars","version":3},"cited_work":{"arxiv_id":"2203.09054","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.09054","snapshot_observed_at":"2026-08-06T19:18:42.433195Z","title":"Revisiting constraints on asymmetric dark matter from collapse in white dwarf stars","venue":"astro-ph.CO","work_id":"f506b2e2-e74b-44d7-9e95-9a6e03ed7604","year":2022},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.689151Z"},"links":{"cited_paper":"/paper/2203.09054","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:046e3fe848aa0421d6aae02a6ec5b3e5eed00270a870e8188003b88c714fb0c8","observation_id":"e2edd688-d4bc-4a5f-99c9-b364a8b5afb1","resolution":{"observed_at":"2026-08-06T19:18:42.522726Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.00669","last_updated":"2023-09-01T18:00:00Z","snapshot_observed_at":"2026-07-06T16:13:23.343694Z","submitted_at":"2023-09-01T18:00:00Z","title":"Dark Matter Capture in Celestial Objects: Treatment Across Kinematic and Interaction Regimes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.00669","snapshot_observed_at":"2026-08-06T19:18:38.784800Z","title":"Dark matter capture in celestial objects: treatment across kinematic and interaction regimes,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.784800Z"},"links":{"cited_paper":"/paper/2309.00669","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:542019ceff80c42d2e499bcce6d05a839fa7114abd99d00add1060ac97f94d74","observation_id":"bacafa65-4662-40a2-9f9d-fe1d54ea82b9","resolution":{"observed_at":"2026-08-06T19:18:38.784800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04378","last_updated":"2016-05-24T19:20:43Z","snapshot_observed_at":"2026-07-06T04:15:12.703402Z","submitted_at":"2015-04-16T20:00:54Z","title":"Generalised form factor dark matter in the Sun","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04378","snapshot_observed_at":"2026-08-06T19:18:38.822994Z","title":"Generalised form factor dark matter in the Sun,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.822994Z"},"links":{"cited_paper":"/paper/1504.04378","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:45fba6f1d0994b6fbb5a9d310449fae9c5926140ed523f43fde4308af8bba269","observation_id":"4c7fba7a-fb00-495b-b248-dc72f15277f0","resolution":{"observed_at":"2026-08-06T19:18:38.822994Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07187","last_updated":"2024-04-10T17:41:33Z","snapshot_observed_at":"2026-07-06T17:58:25.894552Z","submitted_at":"2024-04-10T17:41:33Z","title":"Constraining Bosonic Dark Matter-Baryon Interactions from Neutron Star Collapse","version":1},"cited_work":{"arxiv_id":"2404.07187","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.07187","snapshot_observed_at":"2026-08-06T19:18:42.227514Z","title":"Constraining Bosonic Dark Matter-Baryon Interactions from Neutron Star Collapse","venue":"hep-ph","work_id":"a0968379-543e-49a7-8c61-ab9a227a5472","year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:38.946164Z"},"links":{"cited_paper":"/paper/2404.07187","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:7fa2fd4c2025dee6c3edb840024443957dc6dbcb3596139f2ac6dd6bc5a91ab8","observation_id":"3e7188d0-67e1-4c92-9d3c-a18ed13d8e16","resolution":{"observed_at":"2026-08-06T19:18:42.258157Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.00594","last_updated":"2024-08-01T14:22:15Z","snapshot_observed_at":"2026-08-05T12:14:03.337904Z","submitted_at":"2024-08-01T14:22:15Z","title":"Neutron Star Collapse From Accretion: a Probe of Massive Dark Matter Particles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.00594","snapshot_observed_at":"2026-08-06T19:18:39.075755Z","title":"Neutron star collapse from accretion: A probe of massive dark matter particles,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.075755Z"},"links":{"cited_paper":"/paper/2408.00594","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ccfad00c95ffbb2adab4ca6e9180e35996ac66cf0a791a720e98c4436f8bf9d9","observation_id":"e57e35df-9f73-4aa8-953e-6670d4eaae7a","resolution":{"observed_at":"2026-08-06T19:18:39.075755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.1611","last_updated":"2015-08-28T18:15:04Z","snapshot_observed_at":"2026-07-06T03:12:54.302471Z","submitted_at":"2013-05-07T19:15:08Z","title":"Matrix element analyses of dark matter scattering and annihilation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.1611","snapshot_observed_at":"2026-08-06T19:18:39.175588Z","title":"Matrix element analyses of dark matter scattering and annihilation,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.175588Z"},"links":{"cited_paper":"/paper/1305.1611","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:5d54f325d4dc68906e75db2a5512fd3d14bcba2aca7c218d9328c9bdbe365578","observation_id":"1eb2b6a2-dc52-48a2-b5d7-989382541cee","resolution":{"observed_at":"2026-08-06T19:18:39.175588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05946","last_updated":"2020-08-05T19:28:17Z","snapshot_observed_at":"2026-07-06T09:19:44.971207Z","submitted_at":"2020-05-12T17:47:01Z","title":"Comment on \"Multiscatter stellar capture of dark matter\"","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.05946","snapshot_observed_at":"2026-08-06T19:18:39.270377Z","title":"Comment on “Multiscatter stellar capture of dark matter","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.270377Z"},"links":{"cited_paper":"/paper/2005.05946","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:d861fa57a4cf7a10a698e950e9f7d9e39bb7cb16d4e3ac31428008593909ed32","observation_id":"ee8d1f78-3e18-4aa2-9531-1c6159fa56cd","resolution":{"observed_at":"2026-08-06T19:18:39.270377Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4836","last_updated":"2014-04-08T06:25:25Z","snapshot_observed_at":"2026-08-02T10:55:07.960781Z","submitted_at":"2014-02-19T22:13:33Z","title":"A Comprehensive Study of Relativistic Gravity using PSR B1534+12","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4836","snapshot_observed_at":"2026-08-06T19:18:39.342105Z","title":"A Comprehensive Study of Relativistic Gravity using PSR B1534+12,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.342105Z"},"links":{"cited_paper":"/paper/1402.4836","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:aa56873906b61c7cdc46615f3d9dcfc36443044b780bbcfc87506041a660d514","observation_id":"d176fcfc-e2ff-4063-b3f1-122c47ca8f8d","resolution":{"observed_at":"2026-08-06T19:18:39.342105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02744","last_updated":"2016-06-03T23:54:45Z","snapshot_observed_at":"2026-07-06T04:59:19.498394Z","submitted_at":"2016-06-03T23:54:45Z","title":"Relativistic Measurements from Timing the Binary Pulsar PSR B1913+16","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02744","snapshot_observed_at":"2026-08-06T19:18:39.397203Z","title":"Relativistic Measurements from Timing the Binary Pulsar PSR B1913+16,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.397203Z"},"links":{"cited_paper":"/paper/1606.02744","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:8e9e52a8d05049fafa29d16baf786aa89947e5a3c06de3c8d7c147f0c143306c","observation_id":"26bbcbe3-165a-4344-b9a1-f0b23d1c7d3a","resolution":{"observed_at":"2026-08-06T19:18:39.397203Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0609417","last_updated":"2006-09-14T19:59:48Z","snapshot_observed_at":"2026-08-03T20:33:55.047537Z","submitted_at":"2006-09-14T19:59:48Z","title":"Tests of general relativity from timing the double pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0609417","snapshot_observed_at":"2026-08-06T19:18:39.535804Z","title":"Tests of general relativity from timing the double pulsar,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.535804Z"},"links":{"cited_paper":"/paper/astro-ph/0609417","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:d5e0e8e644186f4240276b17a571739e6f06fb35563327be1a5bb9414e3521e5","observation_id":"d8278b2a-01ee-495b-b5df-f41d5729374f","resolution":{"observed_at":"2026-08-06T19:18:39.535804Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.07697","last_updated":"2018-01-14T22:24:30Z","snapshot_observed_at":"2026-07-06T06:10:30.224957Z","submitted_at":"2017-11-21T10:17:20Z","title":"The High Time Resolution Universe Pulsar Survey - XIII. PSR J1757-1854, the most accelerated binary pulsar","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.07697","snapshot_observed_at":"2026-08-06T19:18:39.620121Z","title":"The High Time Resolution Universe Pulsar Survey – XIII. PSR J1757 −1854, the most accelerated binary pulsar,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.620121Z"},"links":{"cited_paper":"/paper/1711.07697","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:b8f6b974b2dd9eee41272db67bbd477c88ac546e0d2d611007cb1e41f3b4a848","observation_id":"c27a7a11-c290-4723-b263-c4c07c2b229a","resolution":{"observed_at":"2026-08-06T19:18:39.620121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.09460","last_updated":"2024-07-24T10:50:18Z","snapshot_observed_at":"2026-08-03T21:22:49.075713Z","submitted_at":"2023-07-18T17:43:09Z","title":"Probing Light Dark Matter through Cosmic-Ray Cooling in Active Galactic Nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.09460","snapshot_observed_at":"2026-08-06T19:18:39.782665Z","title":"Probing light dark matter through cosmic-ray cooling in active galactic nuclei,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.782665Z"},"links":{"cited_paper":"/paper/2307.09460","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:10961b2d380eeba90178652b898e73e65986fdc3e4af4b989b1acfcb6453e6d5","observation_id":"5fddc43b-6242-458b-8ebe-e1a813c5b3dc","resolution":{"observed_at":"2026-08-06T19:18:39.782665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.03409","last_updated":"2025-04-04T12:39:30Z","snapshot_observed_at":"2026-07-06T21:04:20.337334Z","submitted_at":"2025-04-04T12:39:30Z","title":"Probing Gauged $U(1)$ Sub-GeV Dark Matter via Cosmic Ray Cooling in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.03409","snapshot_observed_at":"2026-08-06T19:18:39.839965Z","title":"Probing Gauged U (1) Sub-GeV Dark Matter via Cosmic Ray Cooling in Active Galactic Nuclei,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.839965Z"},"links":{"cited_paper":"/paper/2504.03409","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:ad533d21835b984b0b022b5e06fd7df1b22ecb0359c3b3ee094b28c76ca67e4f","observation_id":"441482d3-9ced-480c-b56c-271baaba24b3","resolution":{"observed_at":"2026-08-06T19:18:39.839965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6119","last_updated":"2015-04-29T19:34:06Z","snapshot_observed_at":"2026-07-06T04:04:07.039401Z","submitted_at":"2014-12-18T21:17:54Z","title":"Dark Matter-induced Collapse of Neutron Stars: A Possible Link Between Fast Radio Bursts and the Missing Pulsar Problem","version":2},"cited_work":{"arxiv_id":"1412.6119","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.6119","snapshot_observed_at":"2026-08-06T19:18:41.929494Z","title":"Dark Matter-induced Collapse of Neutron Stars: A Possible Link Between Fast Radio Bursts and the Missing Pulsar Problem","venue":"astro-ph.HE","work_id":"14e30ffe-ea9a-45b5-b626-b491c98c061f","year":2014},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:39.961508Z"},"links":{"cited_paper":"/paper/1412.6119","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:9b330d84cfcaa768cf22297c09623b1a4677c13851bf094b4fcd666d19a8a901","observation_id":"b63d186c-3223-41c8-b4e0-dea5d19d5615","resolution":{"observed_at":"2026-08-06T19:18:42.036510Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08057","last_updated":"2024-08-03T10:11:38Z","snapshot_observed_at":"2026-07-06T17:59:04.250437Z","submitted_at":"2024-04-11T18:01:27Z","title":"Revisiting Primordial Black Hole Capture by Neutron Stars","version":4},"cited_work":{"arxiv_id":"2404.08057","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.08057","snapshot_observed_at":"2026-08-06T19:18:41.624798Z","title":"Revisiting Primordial Black Hole Capture by Neutron Stars","venue":"astro-ph.HE","work_id":"31de27ae-2622-4bac-8a31-959343c73fbf","year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.078113Z"},"links":{"cited_paper":"/paper/2404.08057","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:eeef3b9d5000f40c4ce7f1712d642394ea93667d25d64ed44894375f715f2154","observation_id":"434259bc-ca7f-4f52-80d7-b5df42d58968","resolution":{"observed_at":"2026-08-06T19:18:41.742089Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.17035","last_updated":"2024-03-24T18:50:40Z","snapshot_observed_at":"2026-07-06T17:50:26.908430Z","submitted_at":"2024-03-24T18:50:40Z","title":"Axion-Polaritons in quark stars: a possible solution to the missing pulsar problem","version":1},"cited_work":{"arxiv_id":"2403.17035","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.17035","snapshot_observed_at":"2026-08-06T19:18:41.308403Z","title":"Axion-Polaritons in quark stars: a possible solution to the missing pulsar problem","venue":"nucl-th","work_id":"ec5962ca-90da-48ae-977f-bf87e9e219a2","year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.193324Z"},"links":{"cited_paper":"/paper/2403.17035","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:c496518b08410ba8fa4f49f456bc85798cd53a68977630363427742bad0dc971","observation_id":"b13ee2a7-0e9d-4700-9d12-cdc244fcd363","resolution":{"observed_at":"2026-08-06T19:18:41.441652Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9407005","last_updated":"1994-07-01T21:08:33Z","snapshot_observed_at":"2026-08-05T03:07:48.015057Z","submitted_at":"1994-07-01T21:08:33Z","title":"Models of Galaxies with Central Black Holes: Adiabatic Growth in Spherical Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9407005","snapshot_observed_at":"2026-08-06T19:18:40.363552Z","title":"Models of Galaxies with Central Black Holes: Adiabatic Growth in Spherical Galaxies,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.363552Z"},"links":{"cited_paper":"/paper/astro-ph/9407005","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:24d213385695b7e65e1d2157c326ca33484802288fca311fecda4a1fa293819d","observation_id":"5428ac32-a054-4ab6-b48e-f2125b3b0321","resolution":{"observed_at":"2026-08-06T19:18:40.363552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9906391","last_updated":"1999-06-24T17:21:14Z","snapshot_observed_at":"2026-08-06T04:32:21.476097Z","submitted_at":"1999-06-24T17:21:14Z","title":"Dark matter annihilation at the galactic center","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9906391","snapshot_observed_at":"2026-08-06T19:18:40.501365Z","title":"Dark matter annihilation at the galactic center,","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.501365Z"},"links":{"cited_paper":"/paper/astro-ph/9906391","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:b3db76982458f13153f51c75a5d144f8886a04c14ac54a8c2b4d03d8fc8b0f14","observation_id":"ded45678-a035-4b9f-891b-bac26538bce3","resolution":{"observed_at":"2026-08-06T19:18:40.501365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0101481","last_updated":"2001-01-26T16:03:23Z","snapshot_observed_at":"2026-07-07T00:15:40.122044Z","submitted_at":"2001-01-26T16:03:23Z","title":"A Dark-Matter Spike at the Galactic Center?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0101481","snapshot_observed_at":"2026-08-06T19:18:40.607142Z","title":"A Dark matter spike at the galactic center?,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.607142Z"},"links":{"cited_paper":"/paper/astro-ph/0101481","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:5f7690f4a335b1eb12cc30214b2bfa6c96c365d6dee354a24d886fc58bffc6c4","observation_id":"ecb11edc-0bfc-4cde-b591-ef6ac3cf2a20","resolution":{"observed_at":"2026-08-06T19:18:40.607142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.14559","last_updated":"2024-10-18T16:04:18Z","snapshot_observed_at":"2026-07-06T19:36:01.448627Z","submitted_at":"2024-10-18T16:04:18Z","title":"Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars","version":1},"cited_work":{"arxiv_id":"2410.14559","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.14559","snapshot_observed_at":"2026-08-06T19:18:40.988864Z","title":"Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars","venue":"astro-ph.HE","work_id":"5723119f-7e2b-4dc2-a9ba-6dab3ca8bf37","year":2024},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:40.794732Z"},"links":{"cited_paper":"/paper/2410.14559","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:8abb7fe9e32d0e9ff540ffc827d09c512913c99382a3ba872319d64218fc6abe","observation_id":"4dbbdd89-3683-4a7a-ba3d-6b402f0e89ae","resolution":{"observed_at":"2026-08-06T19:18:41.141939Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.1787","last_updated":"2011-11-08T03:13:33Z","snapshot_observed_at":"2026-07-06T02:37:10.370619Z","submitted_at":"2011-11-08T03:13:33Z","title":"Dark-Matter Admixed Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.1787","snapshot_observed_at":"2026-08-06T19:18:35.167572Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":2011,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:35.167572Z"},"links":{"cited_paper":"/paper/1111.1787","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:59e90bc59f38409a0844c14fdf389c9337c7000b1b2f5a864c7465ef4597a9f8","observation_id":"aad192de-8d64-46c9-a73b-b7c28ebc379f","resolution":{"observed_at":"2026-08-06T19:18:35.167572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-06T19:06:38.742831Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?"},"reference_resolution":{"displayed":98,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":84,"verified_exact":14,"verified_fuzzy":0},"total_outbound_references":98},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 98 of 98 outbound references and 1 inbound Pith citation observation for arXiv:2507.06178."}