{"as_of":"2026-08-19T23:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e30f3be4d937836480f083d5cab9d819b880212715980b2243c9b8f0eb679ce9","coverage":[{"denominator":76,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":76,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T14:17:11.047108Z","state":"measured"},{"denominator":77,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":77,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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":"2026-07-14T11:01:05.320963Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.14711","snapshot_observed_at":"2026-07-14T11:01:05.320963Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10533","last_updated":"2026-07-12T02:02:48Z","snapshot_observed_at":"2026-08-15T20:48:01.296220Z","submitted_at":"2026-07-12T02:02:48Z","title":"Geodesics and shadows of the spindle-deformed Kerr black hole","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-14T11:01:05.320963Z"},"links":{"cited_paper":"/paper/2605.14711","citing_paper":"/paper/2607.10533"},"observation_digest":"sha256:1f8302842f9566e7693e141dd1465faf2bde22598f3691fa9a76e14b69390348","observation_id":"9b6adb93-9808-4cb5-82d0-b8afcc852531","resolution":{"observed_at":"2026-07-14T11:01:05.320963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2605.14711/citation-record","integrity":"/paper/2605.14711/integrity","json":"/paper/2605.14711/citation-record.json","paper":"/paper/2605.14711"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T14:17:04.129757Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.129757Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:e22ff37b505eb7e0f07b26231616f9d92dd34fc0e3d6f796f3b64ac53ed3de50","observation_id":"9e101d58-087c-470c-a69e-5ccdaabc0342","resolution":{"observed_at":"2026-08-02T14:17:04.129757Z","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":"2026-08-02T14:17:04.223634Z","title":"in” and “ext","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.223634Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:ca510af61564aa3175ec79c83e233446e4e4031068d333cbaa0e7cb8339e5e22","observation_id":"5446bb64-9fb7-4ce7-b5db-f72d77801e41","resolution":{"observed_at":"2026-08-02T14:17:04.223634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.7377","last_updated":"2014-03-28T14:04:31Z","snapshot_observed_at":"2026-08-12T13:37:17.409976Z","submitted_at":"2014-03-28T14:04:31Z","title":"The Confrontation between General Relativity and Experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.7377","snapshot_observed_at":"2026-08-02T14:17:04.371825Z","title":"The Confrontation between General Relativity and Experiment,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.371825Z"},"links":{"cited_paper":"/paper/1403.7377","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:fabf2c32672126fe6509ed15e7791f004f1f09e522ab13c9719cbd53236977d0","observation_id":"4381e349-8f66-42ab-bcbb-e712fb8f6b62","resolution":{"observed_at":"2026-08-02T14:17:04.371825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.07274","last_updated":"2015-12-02T03:09:26Z","snapshot_observed_at":"2026-08-12T13:39:48.302870Z","submitted_at":"2015-01-28T21:00:11Z","title":"Testing General Relativity with Present and Future Astrophysical Observations","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.07274","snapshot_observed_at":"2026-08-02T14:17:04.488945Z","title":"Testing General Relativity with Present and Future Astrophysical Observations,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.488945Z"},"links":{"cited_paper":"/paper/1501.07274","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:00b47e91dfcb6583b8e19b2f9702960a63bf8f4fad9362580f9a4059fd21f8f4","observation_id":"87dbac3d-c27b-4a66-911c-a8d200143e9b","resolution":{"observed_at":"2026-08-02T14:17:04.488945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.07749","last_updated":"2017-06-21T13:56:34Z","snapshot_observed_at":"2026-08-18T08:12:23.258456Z","submitted_at":"2016-12-22T18:52:33Z","title":"Higher-order theories of gravity: diagnosis, extraction and reformulation via non-metric extra degrees of freedom","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.07749","snapshot_observed_at":"2026-08-02T14:17:04.634359Z","title":"Higher-order theories of gravity: diagnosis, extraction and reformulation via non-metric extra degrees of freedom—a review,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.634359Z"},"links":{"cited_paper":"/paper/1612.07749","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:89e02de69743e2d618c5d7efeed9592468e556af621ea55bf0bc4092e8af2b6e","observation_id":"1591a0fb-df2c-49ad-9a11-8700c566e349","resolution":{"observed_at":"2026-08-02T14:17:04.634359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06533","last_updated":"2022-04-13T17:24:31Z","snapshot_observed_at":"2026-08-16T17:07:07.929245Z","submitted_at":"2022-04-13T17:24:31Z","title":"Modified theories of Gravity: Why, How and What?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.06533","snapshot_observed_at":"2026-08-02T14:17:04.796817Z","title":"Modified theories of gravity: Why, how and what?,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.796817Z"},"links":{"cited_paper":"/paper/2204.06533","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:290698948927620eb536f56530fd37170f85b14781d6eca73147edac700c61b2","observation_id":"40251af2-5197-409f-83ea-0c4b3036fec2","resolution":{"observed_at":"2026-08-02T14:17:04.796817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.01725","last_updated":"2018-07-04T18:03:25Z","snapshot_observed_at":"2026-08-14T18:55:39.732370Z","submitted_at":"2018-07-04T18:03:25Z","title":"A systematic approach to generalisations of General Relativity and their cosmological implications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.01725","snapshot_observed_at":"2026-08-02T14:17:04.937132Z","title":"A systematic approach to generalisations of General Relativity and their cosmological implications,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:04.937132Z"},"links":{"cited_paper":"/paper/1807.01725","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:2031f564549eaf581632f40b1226021df887b3540f19e1b1adde222409fe3eca","observation_id":"65eacb6c-2b8b-4ebd-b7f9-8b000ca5b1fe","resolution":{"observed_at":"2026-08-02T14:17:04.937132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-08-17T06:16:36.216612Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-02T14:17:05.056207Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.056207Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:faed494925c248564eea37af85580bc9b285adaf1b345f27352e5a4bcb1a6854","observation_id":"fc3c1a4f-dfbc-4d1b-8d6d-344b2c9cc0a2","resolution":{"observed_at":"2026-08-02T14:17:05.056207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01766","last_updated":"2024-09-10T10:04:31Z","snapshot_observed_at":"2026-08-16T16:18:53.629694Z","submitted_at":"2022-11-03T12:45:58Z","title":"Spontaneous scalarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01766","snapshot_observed_at":"2026-08-02T14:17:05.157518Z","title":"Sponta- neous scalarization,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.157518Z"},"links":{"cited_paper":"/paper/2211.01766","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:0c66251ac8a73159137b5f07555123cea5e155edf840ce58a48c883dc84a8155","observation_id":"e5d8ac17-a183-49a4-b41c-c4b3b934796f","resolution":{"observed_at":"2026-08-02T14:17:05.157518Z","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":"2026-08-02T14:17:05.237449Z","title":"Vector-Metric Theory of Gravity,","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.237449Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:9d0f16816d508fe5ca38f01524ccd9ef6aa12d0d1664ef8a84edf979d942b6a2","observation_id":"dd9383fd-60f6-41d3-b4a3-ae0f99b53179","resolution":{"observed_at":"2026-08-02T14:17:05.237449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.02209","last_updated":"2022-12-24T14:43:24Z","snapshot_observed_at":"2026-08-16T16:34:35.246318Z","submitted_at":"2022-09-06T04:16:08Z","title":"Static spherical vacuum solutions in the bumblebee gravity model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.02209","snapshot_observed_at":"2026-08-02T14:17:05.395470Z","title":"Static spherical vacuum solutions in the bumblebee gravity model,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.395470Z"},"links":{"cited_paper":"/paper/2209.02209","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:88fcc6f7853c38b75125719c1410ca536d6792945c0e76419cddc2766ee078ac","observation_id":"63a82977-1ba5-4b10-93ae-600793e8de7e","resolution":{"observed_at":"2026-08-02T14:17:05.395470Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.08030","last_updated":"2023-07-01T13:28:17Z","snapshot_observed_at":"2026-08-18T17:59:28.627779Z","submitted_at":"2023-04-17T07:25:56Z","title":"Extended thermodynamics of the bumblebee black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.08030","snapshot_observed_at":"2026-08-02T14:17:05.476632Z","title":"Extended thermodynamics of the bumblebee black holes,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.476632Z"},"links":{"cited_paper":"/paper/2304.08030","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:d8dfb32c628f2c769f4d58e796668349beb8fecf4904107b92f66e5d934c6fff","observation_id":"5647808b-d984-454f-b40d-daf03d20afe2","resolution":{"observed_at":"2026-08-02T14:17:05.476632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.09346","last_updated":"2023-02-06T01:52:30Z","snapshot_observed_at":"2026-08-16T16:07:44.599970Z","submitted_at":"2022-12-19T10:23:37Z","title":"Probing vector hair of black holes with extreme mass ratio inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.09346","snapshot_observed_at":"2026-08-02T14:17:05.641686Z","title":"Probing vector hair of black holes with extreme- mass-ratio inspirals,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.641686Z"},"links":{"cited_paper":"/paper/2212.09346","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:0abccac29b27199cbf78f5d1410c15fd33055ab28b85cc080d291c585a8b7b5b","observation_id":"a480a39c-8058-46e8-a5ae-7d5e6f6a7ebb","resolution":{"observed_at":"2026-08-02T14:17:05.641686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05671","last_updated":"2023-02-11T12:07:27Z","snapshot_observed_at":"2026-08-16T15:56:04.309371Z","submitted_at":"2023-02-11T12:07:27Z","title":"Bumblebee black holes in light of Event Horizon Telescope observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05671","snapshot_observed_at":"2026-08-02T14:17:05.807172Z","title":"Bumblebee Black Holes in Light of Event Horizon Telescope Observations,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.807172Z"},"links":{"cited_paper":"/paper/2302.05671","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:c11ba8489bd8e3b976084d1135fa35a05a00f7e76cdb7d158902a452a8f0315f","observation_id":"e6bafb4a-1b2b-409d-916f-dbd800bd9f02","resolution":{"observed_at":"2026-08-02T14:17:05.807172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.07757","last_updated":"2024-04-08T16:11:17Z","snapshot_observed_at":"2026-08-19T19:56:33.719786Z","submitted_at":"2024-01-15T15:10:01Z","title":"Dynamic instability analysis for bumblebee black holes: the odd parity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.07757","snapshot_observed_at":"2026-08-02T14:17:05.932353Z","title":"Dynamic instability analysis for bumblebee black holes: The odd parity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.932353Z"},"links":{"cited_paper":"/paper/2401.07757","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:ecec7c8fddb329c2ce61cf16e219cf4fe5e5dc1846cba4d695c720a62e24b649","observation_id":"23a2f04b-19e7-4f6b-ad9c-3baa2d3b7da7","resolution":{"observed_at":"2026-08-02T14:17:05.932353Z","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":"2026-08-02T14:17:06.078184Z","title":"The stealth Kerr solution in the bumblebee gravity,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.078184Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:d08f656f983f88a90ca464c93299e450a5f0e703c8009fa830f2b5501808e2a3","observation_id":"b3991b87-021f-4bb8-809e-94a2691f0012","resolution":{"observed_at":"2026-08-02T14:17:06.078184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.02461","last_updated":"2019-02-12T16:29:26Z","snapshot_observed_at":"2026-08-15T00:18:51.124231Z","submitted_at":"2019-01-08T19:00:01Z","title":"Electromagnetism and hidden vector fields in modified gravity theories: spontaneous and induced vectorization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.02461","snapshot_observed_at":"2026-08-02T14:17:06.191674Z","title":"Electromagnetism and hidden vector fields in modi- fied gravity theories: spontaneous and induced vectorization,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.191674Z"},"links":{"cited_paper":"/paper/1901.02461","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:d4088478dcbd5ceac67115c901ad7b91b34a3dd2116d1a845106fe7b289fccc9","observation_id":"a003ac30-f17f-440b-9e58-0d3236a31b19","resolution":{"observed_at":"2026-08-02T14:17:06.191674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04805","last_updated":"2024-11-05T14:50:04Z","snapshot_observed_at":"2026-08-17T07:38:13.712783Z","submitted_at":"2024-09-07T12:08:17Z","title":"Neutron stars in the bumblebee theory of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.04805","snapshot_observed_at":"2026-08-02T14:17:06.351670Z","title":"Neutron stars in the bumblebee theory of gravity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.351670Z"},"links":{"cited_paper":"/paper/2409.04805","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:aa12cc4c5d367dbb857f3c2bf18ac91a5f3bddde1b59c00e4fd73dada4a6d9ad","observation_id":"a22f04af-3a73-4a86-adfb-dab3d1472e5c","resolution":{"observed_at":"2026-08-02T14:17:06.351670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.02486","last_updated":"2023-12-05T04:24:35Z","snapshot_observed_at":"2026-08-16T14:37:37.810395Z","submitted_at":"2023-12-05T04:24:35Z","title":"Probing the vector charge of Sagittarius A* with pulsar timing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.02486","snapshot_observed_at":"2026-08-02T14:17:06.469783Z","title":"Probing the vector charge of Sagittarius A* with pulsar timing,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.469783Z"},"links":{"cited_paper":"/paper/2312.02486","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:836cbcee2e66f5135e195fed6a15b4177f6697e1d6aaa98b79ead03f9079237b","observation_id":"f440c7e5-ba49-4f29-aa6e-d79909ca1f65","resolution":{"observed_at":"2026-08-02T14:17:06.469783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.04594","last_updated":"2022-01-20T18:35:06Z","snapshot_observed_at":"2026-08-16T17:50:38.473461Z","submitted_at":"2021-10-09T15:16:48Z","title":"The ghost of vector fields in compact stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.04594","snapshot_observed_at":"2026-08-02T14:17:06.639432Z","title":"Ghost of vector fields in compact stars,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.639432Z"},"links":{"cited_paper":"/paper/2110.04594","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:04403a96e5b5ad3aaa649039f9362d3ac5d43182d3c3e83a4671735940a77699","observation_id":"eacde23f-fa10-43e6-aa57-86074fa910a6","resolution":{"observed_at":"2026-08-02T14:17:06.639432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04269","last_updated":"2021-12-09T14:21:01Z","snapshot_observed_at":"2026-08-18T08:52:53.479616Z","submitted_at":"2021-12-08T13:04:21Z","title":"Instability of vectorized stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04269","snapshot_observed_at":"2026-08-02T14:17:06.793574Z","title":"Instability of vectorized stars,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.793574Z"},"links":{"cited_paper":"/paper/2112.04269","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:abe1a04a8cfadc71c35a643a37c2c7823342bf0e50474868c059f9802ceb2666","observation_id":"fe0f3ae9-3804-4178-ac85-1de32b91eb28","resolution":{"observed_at":"2026-08-02T14:17:06.793574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.7026","last_updated":"2019-08-01T13:48:04Z","snapshot_observed_at":"2026-08-16T00:33:34.858404Z","submitted_at":"2014-02-27T19:14:27Z","title":"Generalization of the Proca Action","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.7026","snapshot_observed_at":"2026-08-02T14:17:06.920125Z","title":"Generalization of the Proca Action,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:06.920125Z"},"links":{"cited_paper":"/paper/1402.7026","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:c148294d0c85b440e70c21cf2e61fcf973ee183898770d80a086f3f57b38c8ed","observation_id":"a4280c9d-31c9-49fc-bf48-91996d35cc8d","resolution":{"observed_at":"2026-08-02T14:17:06.920125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6450","last_updated":"2014-02-26T08:34:51Z","snapshot_observed_at":"2026-08-14T23:43:18.695614Z","submitted_at":"2014-02-26T08:34:51Z","title":"Cosmic Acceleration from Abelian Symmetry Breaking","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6450","snapshot_observed_at":"2026-08-02T14:17:07.055566Z","title":"Cosmic Acceleration from Abelian Symmetry Breaking,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.055566Z"},"links":{"cited_paper":"/paper/1402.6450","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:e8109d4eff1c0b0257f7616ae46f1d4e3103042eb1fcb7a0d47b5b090fdee15a","observation_id":"2a6100f3-902e-4c53-bf62-11cdfe2569ef","resolution":{"observed_at":"2026-08-02T14:17:07.055566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.03681","last_updated":"2015-11-19T11:25:16Z","snapshot_observed_at":"2026-08-15T15:22:48.351919Z","submitted_at":"2015-11-11T21:11:27Z","title":"Einstein-Vector Gravity, Emerging Gauge Symmetry and de Sitter Bounce","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.03681","snapshot_observed_at":"2026-08-02T14:17:07.139026Z","title":"Einstein-Vector Gravity, Emerging Gauge Symmetry and de Sitter Bounce,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.139026Z"},"links":{"cited_paper":"/paper/1511.03681","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:b1ac636dffe21e4e755be1ab98ba2858132735e0eb10e2e4d0b47c09a269f507","observation_id":"89b6291d-45f3-467a-bc1c-56e54d242a0c","resolution":{"observed_at":"2026-08-02T14:17:07.139026Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.05806","last_updated":"2016-07-03T03:58:14Z","snapshot_observed_at":"2026-08-16T07:21:36.858390Z","submitted_at":"2016-03-18T09:38:24Z","title":"Cosmology in generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.05806","snapshot_observed_at":"2026-08-02T14:17:07.237488Z","title":"Cos- mology in generalized Proca theories,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.237488Z"},"links":{"cited_paper":"/paper/1603.05806","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:12aaba4137d61f53ba5878fe5ffebd05a0875f08ea03fceb4b3c17b3866010ea","observation_id":"065af847-38dd-47e0-8995-c04a86aa865c","resolution":{"observed_at":"2026-08-02T14:17:07.237488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.08355","last_updated":"2016-09-09T09:36:21Z","snapshot_observed_at":"2026-08-14T21:55:34.030216Z","submitted_at":"2016-05-26T16:36:10Z","title":"On the 4D generalized Proca action for an Abelian vector field","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.08355","snapshot_observed_at":"2026-08-02T14:17:07.343068Z","title":"On the 4D generalized Proca action for an Abelian vector field,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.343068Z"},"links":{"cited_paper":"/paper/1605.08355","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:7ce2ab3901fcf0441de6e1e7e74b44162a94b08224c1c2d0d0dbf83e7769d073","observation_id":"5e1019f1-ed10-4d7e-a8ea-925619a4ca60","resolution":{"observed_at":"2026-08-02T14:17:07.343068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.07066","last_updated":"2017-04-20T01:24:07Z","snapshot_observed_at":"2026-08-15T00:18:34.406262Z","submitted_at":"2016-08-25T09:48:42Z","title":"Extended vector-tensor theories","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.07066","snapshot_observed_at":"2026-08-02T14:17:07.435027Z","title":"Extended vector-tensor theories,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.435027Z"},"links":{"cited_paper":"/paper/1608.07066","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:0f34175438e61d60d28f2e39e9d9898d45f320b8558326edef3b2235d614825b","observation_id":"6223d97f-ac42-49e2-bf73-6ceeaf978222","resolution":{"observed_at":"2026-08-02T14:17:07.435027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.4903","last_updated":"2012-03-20T16:19:49Z","snapshot_observed_at":"2026-08-15T04:24:54.046426Z","submitted_at":"2011-12-21T01:42:12Z","title":"Gravitational radiation from compact binary systems in the massive Brans-Dicke theory of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.4903","snapshot_observed_at":"2026-08-02T14:17:07.501334Z","title":"Gravitational radiation from compact binary systems in the massive Brans-Dicke theory of gravity,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.501334Z"},"links":{"cited_paper":"/paper/1112.4903","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:a6b14713ee1d7eba9dce77c63ab0e42cdd8527629606f37bee852d9db687690b","observation_id":"c3d59c98-89d3-4890-b81e-6584f20a6398","resolution":{"observed_at":"2026-08-02T14:17:07.501334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0312310","last_updated":"2004-03-23T19:59:08Z","snapshot_observed_at":"2026-07-07T04:49:20.259241Z","submitted_at":"2003-12-30T16:55:34Z","title":"Gravity, Lorentz Violation, and the Standard Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0312310","snapshot_observed_at":"2026-08-02T14:17:07.561008Z","title":"Gravity, Lorentz violation, and the standard model,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.561008Z"},"links":{"cited_paper":"/paper/hep-th/0312310","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:287c35d675302725cd40ee7a6a0f4557596a00600625c8f88eea118d39686474","observation_id":"98279b58-0f71-4fb0-862d-054af30d08a3","resolution":{"observed_at":"2026-08-02T14:17:07.561008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02273","last_updated":"2017-11-07T03:46:30Z","snapshot_observed_at":"2026-08-14T20:16:17.820004Z","submitted_at":"2017-11-07T03:46:30Z","title":"An exact Schwarzschild-like solution in a bumblebee gravity model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02273","snapshot_observed_at":"2026-08-02T14:17:07.622412Z","title":"Exact Schwarzschild-like solution in a bumblebee gravity model,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.622412Z"},"links":{"cited_paper":"/paper/1711.02273","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:b62ba143babe0ee37f87b3555403ff9f36f3867096ebe2a1d912d069e5a3dda9","observation_id":"73d73fc7-85c6-4a3d-9a1d-c43723f82309","resolution":{"observed_at":"2026-08-02T14:17:07.622412Z","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":"2026-08-02T14:17:07.703180Z","title":"Self-consistent neutron stars in a class of massive vector-tensor gravity,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.703180Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:bdaaf17952fdb9dcaec2656f93603188a489a4dddaa77a5e9533801889a31404","observation_id":"cf9ea5a1-8d26-4692-8d0d-17013fee0bec","resolution":{"observed_at":"2026-08-02T14:17:07.703180Z","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":"2026-08-02T14:17:07.764355Z","title":"Gravitational Field of a Global Monopole,","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.764355Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:c920c3e3e155a5a62f935572b5a926a419f5281541853babbfce70a96c11488a","observation_id":"822fa6fe-02de-4906-a39a-861e467a06d5","resolution":{"observed_at":"2026-08-02T14:17:07.764355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.08697","last_updated":"2016-03-08T16:38:51Z","snapshot_observed_at":"2026-08-14T22:08:26.746098Z","submitted_at":"2016-02-28T10:35:39Z","title":"Black Holes and Abelian Symmetry Breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.08697","snapshot_observed_at":"2026-08-02T14:17:07.855246Z","title":"Black Holes and Abelian Symmetry Breaking,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.855246Z"},"links":{"cited_paper":"/paper/1602.08697","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:9a00db39db3c0a5b5fc55f769e2ffc71834d09dba998116bb4c69163349fd3aa","observation_id":"302af13c-1050-437c-ba91-b57081424554","resolution":{"observed_at":"2026-08-02T14:17:07.855246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.06278","last_updated":"2016-10-30T12:55:36Z","snapshot_observed_at":"2026-08-14T21:47:25.612960Z","submitted_at":"2016-07-21T11:46:53Z","title":"Solutions in the generalized Proca theory with the nonminimal coupling to the Einstein tensor","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.06278","snapshot_observed_at":"2026-08-02T14:17:07.929586Z","title":"Solutions in the generalized Proca theory with the nonminimal coupling to the Einstein tensor,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.929586Z"},"links":{"cited_paper":"/paper/1607.06278","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:a8806898340e18dd9aeb34ab5dbdb1919be40d71c3d2b72f2048d5991e6bb9c7","observation_id":"ba608609-785a-4f55-b042-cfbbcbb217ba","resolution":{"observed_at":"2026-08-02T14:17:07.929586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07951","last_updated":"2017-07-25T12:31:47Z","snapshot_observed_at":"2026-08-14T20:45:27.790690Z","submitted_at":"2017-07-25T12:31:47Z","title":"Stealth configurations in vector-tensor theories of gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.07951","snapshot_observed_at":"2026-08-02T14:17:07.995246Z","title":"Stealth configurations in vector-tensor theories of gravity,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:07.995246Z"},"links":{"cited_paper":"/paper/1707.07951","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:e2af528a317acd62874e525c08f41e262cc300a4806fd40809a1aa4a724dffe4","observation_id":"0a2f34c4-1829-4ab4-8f3e-e9be20f993d7","resolution":{"observed_at":"2026-08-02T14:17:07.995246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.14451","last_updated":"2025-01-07T16:54:54Z","snapshot_observed_at":"2026-08-16T13:08:02.383819Z","submitted_at":"2024-10-18T13:23:59Z","title":"To stealth or not to stealth: Thermodynamics of stealth black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.14451","snapshot_observed_at":"2026-08-02T14:17:08.041601Z","title":"Thermodynamics of stealth black holes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.041601Z"},"links":{"cited_paper":"/paper/2410.14451","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:62c66af9886f570c2752d526734792afce88d47d39bb11c81515a2ce8b30569c","observation_id":"56372b24-564d-4054-a85f-76ba656ef2f9","resolution":{"observed_at":"2026-08-02T14:17:08.041601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.3204","last_updated":"2014-09-10T18:57:42Z","snapshot_observed_at":"2026-08-14T23:52:02.184737Z","submitted_at":"2013-12-11T15:12:58Z","title":"Dressing a black hole with a time-dependent Galileon","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.3204","snapshot_observed_at":"2026-08-02T14:17:08.106449Z","title":"Dressing a black hole with a time-dependent Galileon,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.106449Z"},"links":{"cited_paper":"/paper/1312.3204","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:2794cffe068fd76bcecfcd50344d0999360388c33f69d02bb79c3e11b690fa25","observation_id":"ae984c40-3a31-4e73-b363-b32127d8035f","resolution":{"observed_at":"2026-08-02T14:17:08.106449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01082","last_updated":"2023-09-22T06:32:41Z","snapshot_observed_at":"2026-08-16T15:11:22.290664Z","submitted_at":"2023-08-02T11:12:34Z","title":"Black hole thermodynamics in Horndeski theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01082","snapshot_observed_at":"2026-08-02T14:17:08.180305Z","title":"Black hole thermodynamics in Horndeski theories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.180305Z"},"links":{"cited_paper":"/paper/2308.01082","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:0cc06b1f097862d076b4e1217ba8c59e28201bb2011b0d16a31dbe91958d5752","observation_id":"b168d2b6-0602-46ba-9fd4-75c8565d96f1","resolution":{"observed_at":"2026-08-02T14:17:08.180305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2511.19926","last_updated":"2026-05-19T10:56:21Z","snapshot_observed_at":"2026-08-15T17:05:51.419048Z","submitted_at":"2025-11-25T05:08:30Z","title":"Revisiting black holes and their thermodynamics in Einstein-Kalb-Ramond gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.19926","snapshot_observed_at":"2026-08-02T14:17:08.274786Z","title":"Revisiting black holes and their thermodynamics in Einstein-Kalb-Ramond gravity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.274786Z"},"links":{"cited_paper":"/paper/2511.19926","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:dd6e89b462c5dd7b538fe92082942c4bc4377184ccb46b5143cc02fad13c3107","observation_id":"a60270ad-dd57-4dc5-9675-93406d04ba4c","resolution":{"observed_at":"2026-08-02T14:17:08.274786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01028","last_updated":"2015-04-14T09:28:07Z","snapshot_observed_at":"2026-08-14T23:01:30.374009Z","submitted_at":"2015-02-03T21:02:28Z","title":"Black Holes in Higher-Derivative Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01028","snapshot_observed_at":"2026-08-02T14:17:08.362122Z","title":"Black Holes in Higher-Derivative Gravity,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.362122Z"},"links":{"cited_paper":"/paper/1502.01028","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:3d39d802bedd153d6b0f8b3ad357b725b3bb842adbd5018c69acbe9ed42fffc9","observation_id":"8f8dceff-38ef-48e6-95e0-e773f98ef8bf","resolution":{"observed_at":"2026-08-02T14:17:08.362122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.14395","last_updated":"2020-05-10T12:59:44Z","snapshot_observed_at":"2026-08-18T11:00:54.545763Z","submitted_at":"2020-04-29T18:00:02Z","title":"Black Hole Scalarization in Gauss-Bonnet Extended Starobinsky Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.14395","snapshot_observed_at":"2026-08-02T14:17:08.447141Z","title":"Black hole scalarization in Gauss-Bonnet extended Starobinsky gravity,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.447141Z"},"links":{"cited_paper":"/paper/2004.14395","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:46899bace4db2a7bbbeb1f507d949cf68010798f96e669d2cfd3ea56d76bcf21","observation_id":"44e6f26b-1f2b-4234-a24a-a0a0295b442a","resolution":{"observed_at":"2026-08-02T14:17:08.447141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07198","last_updated":"2017-12-07T06:32:05Z","snapshot_observed_at":"2026-08-14T20:39:31.332590Z","submitted_at":"2017-08-23T21:46:38Z","title":"Quasi-Topological Ricci Polynomial Gravities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.07198","snapshot_observed_at":"2026-08-02T14:17:08.512646Z","title":"Quasi-Topological Ricci Polynomial Gravities,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.512646Z"},"links":{"cited_paper":"/paper/1708.07198","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:68ad870f13e6d8b6a232c0da89e4ddba7498c246ae8e0a47c29635a1b15879ba","observation_id":"c508a13a-16f0-4965-942b-6b8e4160ad16","resolution":{"observed_at":"2026-08-02T14:17:08.512646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.01406","last_updated":"2026-05-19T11:50:08Z","snapshot_observed_at":"2026-08-16T23:15:30.854631Z","submitted_at":"2023-12-03T14:09:12Z","title":"Neutron stars more compact than black holes as a probe of strong-field gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.01406","snapshot_observed_at":"2026-08-02T14:17:08.566757Z","title":"Can a star be smaller than a black hole of the same mass?,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.566757Z"},"links":{"cited_paper":"/paper/2312.01406","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:b8e27bfe5089e99b9205cd0c1674a5523579722d1c360965c458af79a808b147","observation_id":"72e217f3-b4a1-4993-a635-64b2e7f1f29f","resolution":{"observed_at":"2026-08-02T14:17:08.566757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9307038","last_updated":"1993-07-29T16:37:13Z","snapshot_observed_at":"2026-07-07T03:24:21.295752Z","submitted_at":"1993-07-29T16:37:13Z","title":"Black Hole Entropy is Noether Charge","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9307038","snapshot_observed_at":"2026-08-02T14:17:08.640077Z","title":"Black hole entropy is the Noether charge,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.640077Z"},"links":{"cited_paper":"/paper/gr-qc/9307038","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:6ae439a66177094bb18b2f548e03938036d4a0c7291c5dcf800443f6cfb21ff0","observation_id":"836728d7-945f-4db5-8a44-ccb45244f8ab","resolution":{"observed_at":"2026-08-02T14:17:08.640077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9403028","last_updated":"1994-03-15T18:18:00Z","snapshot_observed_at":"2026-08-08T08:03:16.411862Z","submitted_at":"1994-03-15T18:18:00Z","title":"Some Properties of Noether Charge and a Proposal for Dynamical Black Hole Entropy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9403028","snapshot_observed_at":"2026-08-02T14:17:08.705595Z","title":"Some properties of Noether charge and a proposal for dynamical black hole entropy,","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.705595Z"},"links":{"cited_paper":"/paper/gr-qc/9403028","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:3e5a2d439c9a7f5f7dc02a05e735aec188aeee6efb29595e7a93780d439c5945","observation_id":"7324ac4a-ffcd-4108-b718-ad143f95f1a8","resolution":{"observed_at":"2026-08-02T14:17:08.705595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.04392","last_updated":"2018-01-12T10:48:44Z","snapshot_observed_at":"2026-08-14T20:33:31.393984Z","submitted_at":"2017-09-13T15:56:40Z","title":"Black holes in vector-tensor theories and their thermodynamics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.04392","snapshot_observed_at":"2026-08-02T14:17:08.769843Z","title":"Black holes in vector-tensor theories and their thermodynamics,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.769843Z"},"links":{"cited_paper":"/paper/1709.04392","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:4b58b6c2394bf62005b48cedb849a373cacda6bd17d62c3f1473dad15005b2f5","observation_id":"089f2044-be99-4146-af35-54386aef55b5","resolution":{"observed_at":"2026-08-02T14:17:08.769843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0304094","last_updated":"2003-08-25T09:10:36Z","snapshot_observed_at":"2026-08-14T15:57:13.939127Z","submitted_at":"2003-04-24T09:53:46Z","title":"First law of black hole mechanics in Einstein-Maxwell and Einstein-Yang-Mills theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0304094","snapshot_observed_at":"2026-08-02T14:17:08.857570Z","title":"The First law of black hole mechanics in Einstein-Maxwell and Einstein-Yang-Mills theories,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.857570Z"},"links":{"cited_paper":"/paper/gr-qc/0304094","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:0c60d2d302b93ca1d2da8e1d3934a1f1b73934e991e40ed4d0f60e01e7115065","observation_id":"8bec37d0-858f-448e-8e85-02ee8e8bc836","resolution":{"observed_at":"2026-08-02T14:17:08.857570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.02733","last_updated":"2016-07-05T03:18:47Z","snapshot_observed_at":"2026-08-19T00:06:12.046430Z","submitted_at":"2016-06-08T20:02:52Z","title":"Dyonic (A)dS Black Holes in Einstein-Born-Infeld Theory in Diverse Dimensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.02733","snapshot_observed_at":"2026-08-02T14:17:08.926023Z","title":"Dyonic (A)dS Black Holes in Einstein-Born-Infeld Theory in Diverse Dimensions,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.926023Z"},"links":{"cited_paper":"/paper/1606.02733","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:6c8c96a864be4284a0c68e7718c971e421c5bedef8f2f0cb26ad6d5ca1e463c6","observation_id":"eda2423b-f77c-4596-ad8e-1c175018a34e","resolution":{"observed_at":"2026-08-02T14:17:08.926023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.00117","last_updated":"2015-05-28T06:05:18Z","snapshot_observed_at":"2026-08-14T22:50:13.693065Z","submitted_at":"2015-05-01T08:19:50Z","title":"Thermodynamics of static dyonic AdS black holes in the $\\omega$-deformed Kaluza-Klein gauged supergravity theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.00117","snapshot_observed_at":"2026-08-02T14:17:08.980139Z","title":"Thermodynamics of Static Dyonic AdS Black Holes in theω- Deformed Kaluza-Klein Gauged Supergravity Theory,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:08.980139Z"},"links":{"cited_paper":"/paper/1505.00117","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:375173fbc1084401efa0859a6abf51229b94611d140b6d9467a2d5865b3b9cce","observation_id":"02c0a1cc-07c2-498a-afd6-7020e9c0550c","resolution":{"observed_at":"2026-08-02T14:17:08.980139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15430","last_updated":"2024-06-26T07:24:01Z","snapshot_observed_at":"2026-08-19T22:14:53.563519Z","submitted_at":"2024-01-27T14:52:07Z","title":"Notes on thermodynamics of Schwarzschild-like bumblebee black hole","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.15430","snapshot_observed_at":"2026-08-02T14:17:09.068510Z","title":"Notes on thermodynamics of Schwarzschild-like bumblebee black hole,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.068510Z"},"links":{"cited_paper":"/paper/2401.15430","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:8b7f5a2532458640b40a2e77bb760494a758f3e04600d691c8b389a9232d2451","observation_id":"6dde938a-4005-449b-be31-c1ef85c0db95","resolution":{"observed_at":"2026-08-02T14:17:09.068510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.23104","last_updated":"2025-05-29T05:14:13Z","snapshot_observed_at":"2026-08-15T21:27:20.698468Z","submitted_at":"2025-05-29T05:14:13Z","title":"Taub-NUT-like Black Holes in Einstein-Bumblebee Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.23104","snapshot_observed_at":"2026-08-02T14:17:09.155434Z","title":"Taub-NUT-like black holes in Einstein-bumblebee gravity,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.155434Z"},"links":{"cited_paper":"/paper/2505.23104","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:f74a0bdb68c160299bb11fd3ab8daf23bbe5bf76c8bc03270e35a869436999c7","observation_id":"bf114eaa-895e-4513-a66e-e5315a2b7cb6","resolution":{"observed_at":"2026-08-02T14:17:09.155434Z","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":"2026-08-02T14:17:09.218953Z","title":"Dyonic RN-like and Taub-NUT-like black holes in Einstein- bumblebee gravity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.218953Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:f22aa2e8fd8002883502e1e6435b39e9f8e45254eb41f55d0382ca68438ce489","observation_id":"5f71d964-d705-4666-8909-670e2b25c13d","resolution":{"observed_at":"2026-08-02T14:17:09.218953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06613","last_updated":"2023-12-06T02:54:06Z","snapshot_observed_at":"2026-08-17T09:56:12.226783Z","submitted_at":"2023-08-12T17:08:28Z","title":"Static and spherically symmetric black holes in gravity with a background Kalb-Ramond field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06613","snapshot_observed_at":"2026-08-02T14:17:09.287097Z","title":"Static and spherically symmetric black holes in gravity with a background Kalb-Ramond field,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.287097Z"},"links":{"cited_paper":"/paper/2308.06613","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:2088e4c274de90b7b95e710d08599ad0ea31a61a78c51e342830bf132936f6e9","observation_id":"cb91c98f-112c-4a20-a26b-71fb5c53b03e","resolution":{"observed_at":"2026-08-02T14:17:09.287097Z","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":"2026-08-02T14:17:09.338528Z","title":"Improved determination ofγby VLBI,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.338528Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:39ed5bbda185294c012e4580720735b439e14dccec2332fa642096c43228f296","observation_id":"0f50df80-204c-43e0-a236-81d41314c902","resolution":{"observed_at":"2026-08-02T14:17:09.338528Z","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":"2026-08-02T14:17:09.437819Z","title":"A test of general relativity using radio links with the Cassini spacecraft,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.437819Z"},"links":{"citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:a8d6eb34c4fece6ff636cc47191506fcc8ff5cc5a8a3b83654a13be21d45699b","observation_id":"1c19c7b0-f3cc-481a-a1ac-1b7641d41693","resolution":{"observed_at":"2026-08-02T14:17:09.437819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.01374","last_updated":"2025-09-09T14:08:08Z","snapshot_observed_at":"2026-08-19T20:52:31.053256Z","submitted_at":"2025-05-02T16:25:16Z","title":"On the self-consistency of compact objects in Lorentz-violating gravity theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.01374","snapshot_observed_at":"2026-08-02T14:17:09.487220Z","title":"Self-consistency of compact objects in Lorentz-violating gravity theories,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.487220Z"},"links":{"cited_paper":"/paper/2505.01374","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:1f6942eca102a743fade0e395b8207c7a55c23f6f9941cc9d835f245d7340299","observation_id":"640ea260-c165-476b-9ec9-2b7494ce7286","resolution":{"observed_at":"2026-08-02T14:17:09.487220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111092","last_updated":"2001-11-12T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2001-11-05T17:05:33Z","title":"A unified equation of state of dense matter and neutron star structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111092","snapshot_observed_at":"2026-08-02T14:17:09.551019Z","title":"A unified equation of state of dense matter and neutron star structure,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.551019Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:aa59b9b29550e5fc41ea4a379caad29286f3a7d3322a182ab447f8960e7b276f","observation_id":"e2a9413b-0cbb-43b7-adf8-4205ec065a3f","resolution":{"observed_at":"2026-08-02T14:17:09.551019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408324","last_updated":"2004-09-07T15:46:04Z","snapshot_observed_at":"2026-07-07T00:44:10.542942Z","submitted_at":"2004-08-18T10:49:48Z","title":"Analytical representations of unified equations of state of neutron-star matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408324","snapshot_observed_at":"2026-08-02T14:17:09.646300Z","title":"Analytical representations of unified equations of state of neutron-star matter,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.646300Z"},"links":{"cited_paper":"/paper/astro-ph/0408324","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:a99c297851a8886c7a91060b1d939e22cf6fe14b542a82b7507913f1ab4d0931","observation_id":"0e693c91-dd8d-4379-a5f3-078d84b9dc09","resolution":{"observed_at":"2026-08-02T14:17:09.646300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.14108","last_updated":"2024-12-15T07:04:39Z","snapshot_observed_at":"2026-08-16T13:08:12.096955Z","submitted_at":"2024-10-18T01:26:31Z","title":"Neutron stars in Gauss-Bonnet extended Starobinsky gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.14108","snapshot_observed_at":"2026-08-02T14:17:09.722697Z","title":"Neutron stars in Gauss-Bonnet extended Starobinsky gravity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.722697Z"},"links":{"cited_paper":"/paper/2410.14108","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:551ad73999cf54187adfa0fc907ce495f4893d2823db9c3011e384574326e87e","observation_id":"798d2da6-8c5f-4eea-ad12-595de98666ba","resolution":{"observed_at":"2026-08-02T14:17:09.722697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.18916","last_updated":"2025-07-25T03:16:36Z","snapshot_observed_at":"2026-08-16T16:57:51.238884Z","submitted_at":"2025-07-25T03:16:36Z","title":"Radial oscillations of neutron stars in Starobinsky gravity and its Gauss-Bonnet extension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.18916","snapshot_observed_at":"2026-08-02T14:17:09.804954Z","title":"Radial oscillations of neutron stars in Starobin- sky gravity and its Gauss-Bonnet extension,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.804954Z"},"links":{"cited_paper":"/paper/2507.18916","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:2e33fa9eaa41e224684ba5f45c24d5fa2d20316717217cd5515c91c5154d73af","observation_id":"55d03959-9c54-44d2-bed4-c71d183bf7ae","resolution":{"observed_at":"2026-08-02T14:17:09.804954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6875","last_updated":"2013-04-25T11:01:50Z","snapshot_observed_at":"2026-08-15T02:01:27.880780Z","submitted_at":"2013-04-25T11:01:50Z","title":"A Massive Pulsar in a Compact Relativistic Binary","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6875","snapshot_observed_at":"2026-08-02T14:17:09.893091Z","title":"A Massive Pulsar in a Compact Relativistic Binary,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.893091Z"},"links":{"cited_paper":"/paper/1304.6875","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:29c1a0213ebce3183556dea582f5c8953917aca0a924d1a750ad571219b8e80c","observation_id":"480f5b83-815f-47fb-983d-94e775915c4a","resolution":{"observed_at":"2026-08-02T14:17:09.893091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10352","last_updated":"2020-03-24T17:32:24Z","snapshot_observed_at":"2026-08-15T00:30:21.572621Z","submitted_at":"2019-08-27T17:48:59Z","title":"Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10352","snapshot_observed_at":"2026-08-02T14:17:09.981366Z","title":"Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:09.981366Z"},"links":{"cited_paper":"/paper/1908.10352","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:075e9eaa18564427be80f084bb4ead4d23eab1b1e5c1011e97e03d1121552399","observation_id":"30aed80c-6bf8-4a16-833a-b9299089ceb3","resolution":{"observed_at":"2026-08-02T14:17:09.981366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.04766","last_updated":"2016-02-15T18:54:07Z","snapshot_observed_at":"2026-08-14T22:10:15.753357Z","submitted_at":"2016-02-15T18:54:07Z","title":"Slowly rotating neutron stars in scalar-tensor theories with a massive scalar field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.04766","snapshot_observed_at":"2026-08-02T14:17:10.049186Z","title":"Slowly rotating neutron stars in scalar-tensor theories with a massive scalar field,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.049186Z"},"links":{"cited_paper":"/paper/1602.04766","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:dd27443dd01070d70d00ec33fd201310c10eb8dce9f228002b18431f589587f8","observation_id":"fa97e666-87af-4887-b1a6-2cd50c5c4f34","resolution":{"observed_at":"2026-08-02T14:17:10.049186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.07818","last_updated":"2018-05-20T19:59:57Z","snapshot_observed_at":"2026-08-14T19:13:13.110471Z","submitted_at":"2018-05-20T19:59:57Z","title":"Static and slowly rotating neutron stars in scalar-tensor theory with self-interacting massive scalar field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.07818","snapshot_observed_at":"2026-08-02T14:17:10.143954Z","title":"Static and slowly rotating neutron stars in scalar–tensor theory with self-interacting massive scalar field,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.143954Z"},"links":{"cited_paper":"/paper/1805.07818","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:12fb985bb19a11e79be836dc73f22cb2525b21e1537e541bac208c1cae3ef499","observation_id":"755b39de-3e14-4857-b66c-45578139c1a3","resolution":{"observed_at":"2026-08-02T14:17:10.143954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2180","last_updated":"2014-07-08T17:19:41Z","snapshot_observed_at":"2026-08-14T23:27:29.261325Z","submitted_at":"2014-07-08T17:19:41Z","title":"Slowly rotating neutron and strange stars in $R^2$ gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2180","snapshot_observed_at":"2026-08-02T14:17:10.213709Z","title":"Slowly rotating neutron and strange stars inR 2 gravity,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.213709Z"},"links":{"cited_paper":"/paper/1407.2180","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:7e3aa20a0d892b570106ebb6dbaa1155ea507f7e6393bfbdd5e9bb6bc88b23bc","observation_id":"e3237b95-f453-4f4a-9f2e-918c57a34ebd","resolution":{"observed_at":"2026-08-02T14:17:10.213709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4469","last_updated":"2014-06-02T18:32:12Z","snapshot_observed_at":"2026-08-15T02:40:51.282494Z","submitted_at":"2014-02-18T20:55:59Z","title":"Non-perturbative and self-consistent models of neutron stars in R-squared gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4469","snapshot_observed_at":"2026-08-02T14:17:10.298611Z","title":"Non-perturbative and self-consistent models of neutron stars in R-squared gravity,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.298611Z"},"links":{"cited_paper":"/paper/1402.4469","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:5e6f692fa826dce929e0aecb4874d5e63e46495ddfce25752807fa706d9213f3","observation_id":"772d6514-6fc2-4662-be3c-379fd41f1fd9","resolution":{"observed_at":"2026-08-02T14:17:10.298611Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.4499","last_updated":"2013-11-18T18:29:02Z","snapshot_observed_at":"2026-08-16T14:47:28.573166Z","submitted_at":"2013-02-19T01:19:43Z","title":"I-Love-Q","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.4499","snapshot_observed_at":"2026-08-02T14:17:10.370066Z","title":"I-Love-Q,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.370066Z"},"links":{"cited_paper":"/paper/1302.4499","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:b29cde682e16e82171af3d580fd01aa0ec30d96ae275592b8687f1213469b667","observation_id":"66b984e8-742d-443a-9dee-aa0ec1af320f","resolution":{"observed_at":"2026-08-02T14:17:10.370066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1528","last_updated":"2017-11-30T16:53:50Z","snapshot_observed_at":"2026-08-15T00:26:19.755098Z","submitted_at":"2013-03-06T21:00:03Z","title":"I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1528","snapshot_observed_at":"2026-08-02T14:17:10.460983Z","title":"I-Love-Q Relations in Neutron Stars and their Applications to As- trophysics, Gravitational Waves and Fundamental Physics,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.460983Z"},"links":{"cited_paper":"/paper/1303.1528","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:fe639b36364d91d74aa1e64cb552ca1ddf1c7c259ba80a97bc43de3ddd0a02f1","observation_id":"5caf43de-96a4-45f7-951e-db4400ab15ed","resolution":{"observed_at":"2026-08-02T14:17:10.460983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08774","last_updated":"2024-08-29T10:11:48Z","snapshot_observed_at":"2026-08-18T18:58:34.700063Z","submitted_at":"2024-07-11T18:00:01Z","title":"Fixing the dynamical evolution of self-interacting vector fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08774","snapshot_observed_at":"2026-08-02T14:17:10.528398Z","title":"Fixing the dynam- ical evolution of self-interacting vector fields,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.528398Z"},"links":{"cited_paper":"/paper/2407.08774","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:cb6eef383c5450e83da5e8ce999c77802adbb565e4ceb848deb5e4063896c062","observation_id":"3b6d62c8-c13d-404e-8480-7086feb0ad5e","resolution":{"observed_at":"2026-08-02T14:17:10.528398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07784","last_updated":"2022-10-04T16:47:20Z","snapshot_observed_at":"2026-08-16T16:59:58.692163Z","submitted_at":"2022-05-16T16:15:24Z","title":"The intrinsic pathology of self-interacting vector fields","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.07784","snapshot_observed_at":"2026-08-02T14:17:10.590497Z","title":"Intrinsic Pathology of Self-Interacting Vector Fields,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.590497Z"},"links":{"cited_paper":"/paper/2205.07784","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:bab75b3507bc6ff2851e5426e5e465e00b33165696da8d8eb0a96b5d71fe2ff5","observation_id":"02cf9d55-4472-4268-ae4c-fa75f0e72bb9","resolution":{"observed_at":"2026-08-02T14:17:10.590497Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.00443","last_updated":"2022-11-25T09:48:37Z","snapshot_observed_at":"2026-08-16T16:48:57.600989Z","submitted_at":"2022-07-01T14:09:19Z","title":"The well-posedness of the Cauchy problem for self-interacting vector fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.00443","snapshot_observed_at":"2026-08-02T14:17:10.687536Z","title":"The well-posedness of the Cauchy problem for self-interacting vector fields,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.687536Z"},"links":{"cited_paper":"/paper/2207.00443","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:a953c93d5ca2c57db120a052540900538740442ea0dff963417388feca3a42f7","observation_id":"6eac577a-d87b-42f7-b875-44f857d4e170","resolution":{"observed_at":"2026-08-02T14:17:10.687536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.08027","last_updated":"2023-01-17T19:19:35Z","snapshot_observed_at":"2026-08-19T16:40:48.260772Z","submitted_at":"2022-11-15T10:19:08Z","title":"Coordinate singularities of self-interacting vector field theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.08027","snapshot_observed_at":"2026-08-02T14:17:10.750551Z","title":"Coordinate Singularities of Self-Interacting Vector Field Theories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.750551Z"},"links":{"cited_paper":"/paper/2211.08027","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:9aa9431809666734a2190da025b56b8dc1ffd7f5a4e46d8a9519767e1e0f00aa","observation_id":"e55655e2-f51a-4cce-b786-a254e126407a","resolution":{"observed_at":"2026-08-02T14:17:10.750551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.02263","last_updated":"2023-05-16T05:09:21Z","snapshot_observed_at":"2026-08-19T21:13:50.460638Z","submitted_at":"2023-01-05T19:00:13Z","title":"Pervasiveness of the breakdown of self-interacting vector field theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.02263","snapshot_observed_at":"2026-08-02T14:17:10.830205Z","title":"Pervasiveness of the breakdown of self-interacting vector 28 field theories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.830205Z"},"links":{"cited_paper":"/paper/2301.02263","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:d4085e7d266ffb1ee2315ff2da716bbfb053c46665430e856efdd6038549fb38","observation_id":"55d02a85-e7ea-4539-9075-8846f8950c97","resolution":{"observed_at":"2026-08-02T14:17:10.830205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.03554","last_updated":"2023-08-13T11:07:31Z","snapshot_observed_at":"2026-08-19T15:53:30.020438Z","submitted_at":"2023-06-06T10:09:47Z","title":"Loss of hyperbolicity and tachyons in generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.03554","snapshot_observed_at":"2026-08-02T14:17:10.880876Z","title":"Loss of hyperbolicity and tachyons in generalized Proca theories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.880876Z"},"links":{"cited_paper":"/paper/2306.03554","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:fba3231f23cc958d558fe4188377cf330a818457fb004dc69c724b97cd69f6cd","observation_id":"b65a1579-b98f-4dff-98a2-5d0ad6d6d330","resolution":{"observed_at":"2026-08-02T14:17:10.880876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.07743","last_updated":"2023-11-13T16:14:22Z","snapshot_observed_at":"2026-08-16T15:16:03.558427Z","submitted_at":"2023-07-15T08:33:44Z","title":"Treatments and placebos for the pathologies of effective field theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.07743","snapshot_observed_at":"2026-08-02T14:17:10.966421Z","title":"Treatments and placebos for the pathologies of effective field theories,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:10.966421Z"},"links":{"cited_paper":"/paper/2307.07743","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:cb9cab7dd9fbffc8263b1ba30a73a02fe6a2b40bda62732122d5f174d12ca205","observation_id":"a84e3a03-16bb-4909-97b7-8137c8ed2392","resolution":{"observed_at":"2026-08-02T14:17:10.966421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.15321","last_updated":"2024-06-21T17:28:24Z","snapshot_observed_at":"2026-08-16T13:40:40.244850Z","submitted_at":"2024-06-21T17:28:24Z","title":"Aspects of time evolution in $p$-form field theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.15321","snapshot_observed_at":"2026-08-02T14:17:11.047108Z","title":"Aspects of time evolution in p-form field theories,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:11.047108Z"},"links":{"cited_paper":"/paper/2406.15321","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:f0e3dcc6c6964a94b29ab2d95c1c09419341dab4a083fef892b1790be1c502bd","observation_id":"6e8c3aca-b995-4611-954e-fa5536c39e41","resolution":{"observed_at":"2026-08-02T14:17:11.047108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-12T14:27:37.984606Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory"},"reference_resolution":{"displayed":76,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":76,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":76},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 76 of 76 outbound references and 1 inbound Pith citation observation for arXiv:2605.14711."}