{"as_of":"2026-08-15T01:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:102d8e42946300ebe9b1ed897a99bfb6c5b1c6130f83e8567821e2ce6ffda60e","coverage":[{"denominator":239,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-12T04:18:55.037825Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+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":"2026-08-02T03:35:57.515370Z","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":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.03183","snapshot_observed_at":"2026-08-02T03:35:57.515370Z","title":"Zhou, T.-N","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.13857","last_updated":"2026-07-15T14:02:52Z","snapshot_observed_at":"2026-08-12T18:06:39.936614Z","submitted_at":"2026-07-15T14:02:52Z","title":"Evaporating cosmologically coupled black holes","version":1},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-02T03:35:57.515370Z"},"links":{"cited_paper":"/paper/2607.03183","citing_paper":"/paper/2607.13857"},"observation_digest":"sha256:8adc592de6e910a1a076156413b897a7d07af032de6a09b4d74816f8f5c299d6","observation_id":"e5f1294f-e848-471e-8288-b4acaa2eeb8b","resolution":{"observed_at":"2026-08-02T03:35:57.515370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2607.03183/citation-record","integrity":"/paper/2607.03183/integrity","json":"/paper/2607.03183/citation-record.json","paper":"/paper/2607.03183"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-ex/9807003","last_updated":"1998-08-31T21:28:10Z","snapshot_observed_at":"2026-07-07T03:39:16.997821Z","submitted_at":"1998-07-03T14:23:51Z","title":"Evidence for oscillation of atmospheric neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/9807003","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Fukudaet al.(Super-Kamiokande), Phys","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/hep-ex/9807003","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:78946dc07a5da06f551c6e824d0ba171682ac98076e71aff0e984b4c02e73ed0","observation_id":"7a8b3611-edf8-477a-b563-2f008b1453eb","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Fukudaet al.(Super-Kamiokande), Phys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:f95caaed293cd6b7b1d4d41b04530f2525439192021f0c66fd5632fb728a65ee","observation_id":"1dcdf589-4683-49b5-8ae9-8493b47c4027","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-ex/0106015","last_updated":"2001-06-30T04:05:08Z","snapshot_observed_at":"2026-07-07T06:23:54.100794Z","submitted_at":"2001-06-18T16:22:42Z","title":"Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-ex/0106015","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/nucl-ex/0106015","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:7ceacfba907909ca212ed34029372fc887f5941da19fd103f21ab206ac7596d4","observation_id":"123607a0-17cf-499a-a2ad-183203f5ab0c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:02ab8be73b2256bd2157ccc3740b9f4dc5b4d75a94ee21ca44e80e8e797b289c","observation_id":"26649645-d05e-4a9a-8e5b-cc4a88b7ecca","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:cfa34f7d9d6790eefd5604d788f996239668cc973ae23d9e1ef2d0f4066c3cc4","observation_id":"8270f38f-e9ef-42a7-be67-9ceb51b7c015","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.14792","last_updated":"2020-07-27T18:00:02Z","snapshot_observed_at":"2026-08-14T09:28:30.553172Z","submitted_at":"2020-07-27T18:00:02Z","title":"The fate of hints: updated global analysis of three-flavor neutrino oscillations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.14792","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Esteban, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2007.14792","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e22555586f9233406af65b2bbd056ea2ea4abe8538df28061ea4cd75895be670","observation_id":"ba09b768-f4bc-46fe-ad04-8e4c0e335c07","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:cae3b9b7519fca5708bf0ad2aa1c553a887fd4d004b0027486bcad4e2ee25860","observation_id":"bde38e14-85c0-4f05-a806-1fae29662b7d","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.11237","last_updated":"2021-01-19T09:50:37Z","snapshot_observed_at":"2026-08-12T17:30:15.613475Z","submitted_at":"2020-06-19T17:21:48Z","title":"2020 Global reassessment of the neutrino oscillation picture","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.11237","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2006.11237","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:380282e2a204d6c54b53356bcde37ed968c79f6603e300bbaba95a0c70ad6870","observation_id":"8aeb09cb-6e5b-410e-a39d-3237104a3cc7","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05380","last_updated":"2025-10-28T13:33:51Z","snapshot_observed_at":"2026-08-13T20:34:18.192890Z","submitted_at":"2024-10-07T18:00:02Z","title":"NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05380","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Esteban, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2410.05380","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e5bceaca35cf777e11dd471709e4a7f094b72e6708dc693ed6c307549edf0872","observation_id":"050434c5-70b0-4584-8a53-762c316df016","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.07752","last_updated":"2025-03-10T18:08:31Z","snapshot_observed_at":"2026-08-13T16:15:04.373206Z","submitted_at":"2025-03-10T18:08:31Z","title":"Neutrino masses and mixing: Entering the era of subpercent precision","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.07752","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Capozzi, W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2503.07752","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:aafd298765da60d903c312952a40213e70e1cd92f24d3e383dd3939e296c74f7","observation_id":"e14729e6-6d75-4694-8c51-5361d4a72405","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:f642bbd107df393538559ffa27a026ca26e6f1e0cbfaf6d11ddd9617e6a51d2c","observation_id":"443f40ca-3725-40a7-9004-fbcf46487750","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.09791","last_updated":"2026-04-12T17:43:39Z","snapshot_observed_at":"2026-08-13T16:49:11.972279Z","submitted_at":"2026-01-14T19:00:24Z","title":"Lessons from the first JUNO results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.09791","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Esteban, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2601.09791","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:0909afe2299465e92186ca8527f15899741fbce5f12b30784d52c8c50739bd85","observation_id":"0f9effdb-8902-44ea-b661-3811c0cacc61","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603494","last_updated":"2006-05-29T15:16:34Z","snapshot_observed_at":"2026-08-06T13:16:13.017108Z","submitted_at":"2006-03-20T10:19:09Z","title":"Massive neutrinos and cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603494","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Lesgourgues and S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0603494","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:fa0ebcb7ba92132e958688af8abc0d37944ae7219b5a9ed16aec257f7a8093a6","observation_id":"0c98c8e1-2de0-4b59-bd2f-598c009df17f","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Aghanimet al.(Planck), Astron","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:ae1f574f21234c4390cb288bc8e7e94ecf25ac6fee61c352f514bbd36a6a11b3","observation_id":"9f30ec4c-862b-4ed7-a85a-0116da303ad5","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Abdul Karimet al.(DESI), Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:ed523de9a77730429d2cffc6b4de79e28566c4309086ef4f13a75c178a8ad1ee","observation_id":"6c8d1e47-ca8b-4430-afa2-ce14dac90812","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08991","last_updated":"2024-07-09T09:56:49Z","snapshot_observed_at":"2026-08-13T11:53:26.094346Z","submitted_at":"2020-07-17T14:09:48Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08991","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Alamet al.(eBOSS), Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2007.08991","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:b7aecb1a59a6d1f552425895cc59b26aed1257967621a72d26520bc0066c0c85","observation_id":"c08b40fc-d391-46b5-b4ea-36d275a9824a","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04077","last_updated":"2022-11-14T21:28:25Z","snapshot_observed_at":"2026-08-01T22:04:41.273741Z","submitted_at":"2022-02-08T19:00:00Z","title":"The Pantheon+ Analysis: Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04077","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Broutet al., Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d362c4dac834c9f0893ed2052876c01181f2a8196c91ad51f78bad59a889adc7","observation_id":"eafe2c15-d36c-4e5e-aae3-a85ebea7395e","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9904398","last_updated":"2000-04-19T12:25:58Z","snapshot_observed_at":"2026-07-07T01:25:56.760989Z","submitted_at":"1999-04-28T18:42:28Z","title":"The Case for a Positive Cosmological Lambda-term","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9904398","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Sahni and A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/9904398","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:26dc1179b4e39060906c131229f11b26bbc4df541c24f8a3b08b73a5392373fb","observation_id":"dff833eb-0e80-4952-8c35-4032ccc23153","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510059","last_updated":"2005-10-03T19:45:26Z","snapshot_observed_at":"2026-07-07T00:54:39.935968Z","submitted_at":"2005-10-03T19:45:26Z","title":"Insights into Dark Energy: Interplay Between Theory and Observation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510059","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0510059","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:91da8860112cc5e5ccfa77194af87d9bbdc838ca06792e576f7c4924f7787416","observation_id":"306ae90c-3141-4394-9eaa-e32296c25e37","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5302","last_updated":"2013-10-01T02:58:48Z","snapshot_observed_at":"2026-08-15T00:16:55.280565Z","submitted_at":"2013-05-23T02:27:04Z","title":"Planck Constraints on Holographic Dark Energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5302","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, X.-D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1305.5302","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:038dbcb9da61d6395a6abb8d8ff06fed4dfe2e789c575454bb604a49ca6c0dc3","observation_id":"7594ab08-68da-41a2-a2e6-4b03cbdcfbad","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.7028","last_updated":"2014-12-17T15:02:17Z","snapshot_observed_at":"2026-08-14T23:39:43.855397Z","submitted_at":"2014-03-27T13:48:03Z","title":"Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.7028","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, Y.-H","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1403.7028","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:caeca6538ac36b437ad47d52da62a3c67ef2da9b64da19e6e5629fea48fa2a0f","observation_id":"5c84f48b-623a-4683-8d14-5e6fe13f7078","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.08456","last_updated":"2017-09-02T10:33:40Z","snapshot_observed_at":"2026-08-14T21:10:10.962113Z","submitted_at":"2017-03-24T15:17:49Z","title":"Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.08456","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhao, D.-Z","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1703.08456","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:8e452d08ec4c64954163b4dbb56a3273a5fe5e9ad6da95fae6520fbe30bc6f21","observation_id":"21790666-02c0-4bc8-8985-0466db6b1953","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.02340","last_updated":"2019-01-28T12:57:25Z","snapshot_observed_at":"2026-08-14T18:31:47.224014Z","submitted_at":"2018-09-07T08:05:46Z","title":"Can the $H_0$ tension be resolved in extensions to $\\Lambda$CDM cosmology?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.02340","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Guo, J.-F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1809.02340","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:6ac7a917b25e7222b5610b4e4a577dbd13dd3b6dbc7ef74b342839ec11cd3e59","observation_id":"2265e7f0-7190-468c-854d-0291567761f2","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-07-06T08:09:59.842324Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Verde, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e4811a8385681d18762d7b01924eb3f225c2d3273a00ab52a153e039647bff1f","observation_id":"ca053896-38e6-4a2a-8f82-67806c7a6c57","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11284","last_updated":"2020-10-13T11:06:51Z","snapshot_observed_at":"2026-08-13T21:46:00.875155Z","submitted_at":"2020-08-25T21:37:24Z","title":"Cosmology Intertwined II: The Hubble Constant Tension","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11284","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Di Valentinoet al., Astropart","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2008.11284","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:a8b9101ebb56461a7303c86566f76dfef6be8ee62a046b27a672909f4840d8b9","observation_id":"8cd28ded-e835-46b1-8ace-0ec4e332e724","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11285","last_updated":"2020-10-13T11:11:55Z","snapshot_observed_at":"2026-08-10T13:14:09.209280Z","submitted_at":"2020-08-25T21:41:42Z","title":"Cosmology Intertwined III: $f \\sigma_8$ and $S_8$","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11285","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Di Valentinoet al., Astropart","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2008.11285","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:8a45ae4f1c51eaa64fdbf352837721e98582fbd8265a3b191850fdb4f7fc9d72","observation_id":"00df48de-c5f7-4bab-a9e5-e4f3db2e59c5","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.04281","last_updated":"2020-07-01T09:13:30Z","snapshot_observed_at":"2026-08-14T21:44:35.303861Z","submitted_at":"2019-08-12T17:48:35Z","title":"Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.04281","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1908.04281","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d78196a0815fd94eee9fea53d47acdf61c9a2461da6833a18dec39305f1b04fb","observation_id":"681ee92d-f6cd-4c72-b1d7-50a8d5f29c47","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.07569","last_updated":"2020-06-26T09:34:46Z","snapshot_observed_at":"2026-08-14T16:05:04.266879Z","submitted_at":"2019-07-17T15:10:07Z","title":"New physics in light of the $H_0$ tension: an alternative view","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.07569","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Vagnozzi, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1907.07569","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:9c53d75c45426b358aa94326020840de3ad4a83575db2f5d9b3263da64af81bb","observation_id":"0ba91c8a-7ef1-49b3-a863-455a24923310","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.10425","last_updated":"2021-07-23T08:40:59Z","snapshot_observed_at":"2026-08-10T16:06:26.046456Z","submitted_at":"2021-05-21T15:51:25Z","title":"Consistency tests of $\\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.10425","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Vagnozzi, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2105.10425","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:3b1f3d08ffe2953b8f601550226359a1bb4a1cb8139392e52f4e6c336e1fa653","observation_id":"87ab3f89-ba0f-49a5-a594-1c4e17381ecf","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.10421","last_updated":"2022-08-03T06:24:03Z","snapshot_observed_at":"2026-08-10T16:03:47.102299Z","submitted_at":"2021-05-21T15:41:25Z","title":"Implications for the Hubble tension from the ages of the oldest astrophysical objects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.10421","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Vagnozzi, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2105.10421","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:991b0d7f274c5adc4bc366f35911db270d8446dd10df719b1fe84d82684335dc","observation_id":"28363d0e-088b-425f-bd3c-3f9822ab2bee","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16628","last_updated":"2023-08-31T10:49:29Z","snapshot_observed_at":"2026-08-13T10:23:33.893455Z","submitted_at":"2023-08-31T10:49:29Z","title":"Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.16628","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Vagnozzi, Universe9, 393 (2023), arXiv:2308.16628 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2308.16628","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:ce825940f8cb384afdf337a93af038f99865cca18006f756b30bfdad484a9fa7","observation_id":"f32ae36d-3b38-4806-b53a-51273e0856f9","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.10714","last_updated":"2021-05-26T07:56:37Z","snapshot_observed_at":"2026-08-13T20:24:49.754801Z","submitted_at":"2021-01-26T11:20:45Z","title":"Relieving the $H_0$ tension with a new interacting dark energy model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.10714","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Gao, Z.-W","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2101.10714","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c79b9c6fdcdf79a837f819eede0c8b101e1c1817bef49b0bdfe0d8b20f25a59b","observation_id":"034d45da-9a2f-4c27-81fa-7e039b467514","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.01859","last_updated":"2021-11-12T09:53:32Z","snapshot_observed_at":"2026-08-15T00:40:31.861224Z","submitted_at":"2021-06-03T14:01:57Z","title":"How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.01859","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Jin, L.-F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2106.01859","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:2b5607ac0df2922f31bec8130e570166cd3e251d53ef29d21568c1a2f018cb79","observation_id":"fe72bb03-f768-4470-9d5e-9d75bfa05286","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e8e2acb1c5b58b25aa6e15a4bd5e20e87fdceb6a4fa566952e6219858dfab8af","observation_id":"56f3c109-4bb1-4498-9def-5d0bf2abf3ad","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.10291","last_updated":"2021-10-15T15:48:33Z","snapshot_observed_at":"2026-08-14T02:04:58.036108Z","submitted_at":"2021-07-21T18:15:15Z","title":"The $H_0$ Olympics: A fair ranking of proposed models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.10291","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Sch¨ oneberg, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2107.10291","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:36c49929aa31e8f59fdc7c1fa442d2db0f3fb5aa2c5fa29ee5a8bb3e39bd010d","observation_id":"a7da408b-5666-4702-841a-a0df5110357c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Abdallaet al., JHEAp34, 49 (2022), arXiv:2203.06142 [astro-ph.CO]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:656a4be3a5c207191826144ceca6ff0aff39d1bf990584baabf25801cf3fb4e6","observation_id":"371c928c-83e9-43ed-a225-906a04d9bed0","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Di Valentino, Universe8, 399 (2022)","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:aa63faa16a1a3555ae1f0ea905e62daa55b8f647b21ef3905ee33e78e83f16ca","observation_id":"f3b892ac-0c7c-443e-9910-35386293a036","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04492","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Kamionkowski and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2211.04492","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:3a49973135bb9d89867b8987c297244fd6cf89a49c2d7e16646dff3db318b0e2","observation_id":"39902162-d880-4ae6-9a61-a51a3b362032","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.13146","last_updated":"2024-03-29T03:18:11Z","snapshot_observed_at":"2026-08-15T00:40:32.555985Z","submitted_at":"2022-12-26T13:04:11Z","title":"Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.13146","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Gao, S.-S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2212.13146","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:af1c347d46d7f22345099365b1559ad843f7c42aa9fd543fc67415e77b713b9c","observation_id":"24fd9841-4dbb-4524-9771-892855a1a52c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16919","last_updated":"2023-06-02T10:32:38Z","snapshot_observed_at":"2026-08-15T00:40:49.753554Z","submitted_at":"2023-05-26T13:33:18Z","title":"CMB Anomalies and the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16919","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Giar` e, (2023), 10.1007/978-981-99-0177-7 36, arXiv:2305.16919 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2305.16919","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d981084c2f162048884045d59591b21e00bfec2dbbd532836087d72a2a42a176","observation_id":"d16d0aed-91ef-4e15-99a8-aa5f5f4bd414","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05709","last_updated":"2023-02-11T14:51:33Z","snapshot_observed_at":"2026-08-13T12:46:54.224821Z","submitted_at":"2023-02-11T14:51:33Z","title":"Hubble Tension: The Evidence of New Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05709","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Hu and F.-Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2302.05709","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:7ed169271f451a021e417bdea6d761025d56ffbfe0134d8eaddbbd5bd45de261","observation_id":"0d1f6261-17e0-4a4b-a133-f53a0bbea6bc","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19441","last_updated":"2025-10-21T16:24:56Z","snapshot_observed_at":"2026-07-06T20:58:14.950470Z","submitted_at":"2025-03-25T08:30:40Z","title":"KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19441","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2503.19441","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:88857fa4304dd5ccab015e4d231b36fe2180afcdc60c33369e5e615f30f8b5c5","observation_id":"f0997761-8c33-47eb-a8ce-13936e2170d4","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-14T03:18:00.674049Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.20434","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Cai and S.-J","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2606.20434","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:5c9f065e7c472d31042b89165fc3b1ce85600f7cd95d7d054ee95df5d0f74c4d","observation_id":"aae5a271-dff2-491c-92fd-43c0f5f134b5","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Pantos and L","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:463702deaa71b9a755922f0ee72bedfdff79377dee3126434becc398136431c4","observation_id":"33d3ed14-c3d9-494d-9304-f76e737bc2ca","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04773","last_updated":"2024-01-09T19:03:36Z","snapshot_observed_at":"2026-08-15T00:40:49.995520Z","submitted_at":"2024-01-09T19:03:36Z","title":"JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8 sigma Confidence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04773","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2401.04773","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c97b306a49c465de163cfe47362dde22f0213f7744136b6cf2cba4de51986925","observation_id":"2453a13b-a486-4a6f-909f-a2bd1222b4b1","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0009008","last_updated":"2000-09-25T18:37:17Z","snapshot_observed_at":"2026-07-07T03:13:00.877347Z","submitted_at":"2000-09-04T15:09:00Z","title":"Accelerating Universes with Scaling Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0009008","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Chevallier and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/gr-qc/0009008","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:9724ef141e807f60080996f1d2c9ff2246487ee707cfb743639acdfc64454042","observation_id":"4cc46226-254a-4957-85a1-bb2d6c8c19b6","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0103004","last_updated":"2001-03-21T16:30:06Z","snapshot_observed_at":"2026-08-14T11:10:05.023063Z","submitted_at":"2001-03-01T16:36:41Z","title":"An alternative to quintessence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0103004","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/gr-qc/0103004","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:8c066c3a401075db6f6b1435cfe1f541f9e0bc71921dfbc39f148fc20fc17cdf","observation_id":"f9c0a2f8-59db-47ca-8eb0-906cefc634a4","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0208512","last_updated":"2002-08-28T23:21:10Z","snapshot_observed_at":"2026-07-07T00:28:09.066072Z","submitted_at":"2002-08-28T23:21:10Z","title":"Exploring the Expansion History of the Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0208512","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0208512","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:6875ab64fa0d594f41f567f40e5a46aa208a30793a65e35a7e2a1b43f163fab9","observation_id":"655ff5fb-c362-459a-afb3-9341816089d3","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Li, Phys","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:5bfa6b0f715424205994dfd1c0e9d47aae27d0483b720c1ad3cfab7e6e9cb039","observation_id":"cd1667c0-de39-4a00-a80a-2f4bf69c776a","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404229","last_updated":"2004-04-23T05:35:13Z","snapshot_observed_at":"2026-07-07T00:41:56.225026Z","submitted_at":"2004-04-12T15:11:39Z","title":"The Holographic Dark Energy in a Non-flat Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0404229","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Huang and M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0404229","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:b9c4a0a45b0b5f8451f91c021805b6f9f7fc3cc3e3ad2b73ed81a7d6687dbb5e","observation_id":"aa28c4e0-6134-459e-86f6-9f4b4e791332","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0404057","last_updated":"2005-02-16T11:37:56Z","snapshot_observed_at":"2026-07-07T04:50:13.827377Z","submitted_at":"2004-04-07T01:09:41Z","title":"Constraints on the dark energy from holography","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0404057","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/hep-th/0404057","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:23d28f7924fab3c74e34b2804f441760151130300f27470871c764f5439e84f7","observation_id":"de0e39d4-9fdb-44ac-b259-1a2736bc9d6c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506310","last_updated":"2005-08-19T08:07:46Z","snapshot_observed_at":"2026-07-07T00:51:18.608238Z","submitted_at":"2005-06-14T15:12:02Z","title":"Constraints on holographic dark energy from type Ia supernova observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506310","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang and F.-Q","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0506310","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:b75db7fc7688053fcc35692087884271ff3b70d3ef8f2933676b479286cd0143","observation_id":"cfd81231-e0ca-4981-a45b-8a8b49691f04","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504586","last_updated":"2005-09-29T15:03:24Z","snapshot_observed_at":"2026-07-07T00:50:12.061165Z","submitted_at":"2005-04-27T08:36:31Z","title":"Statefinder diagnostic for holographic dark energy model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504586","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, Int","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0504586","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c76a0df5d608fb6d746bb59a0ee46368a702493f770a269a71900051af01c2b8","observation_id":"177084ee-5641-47c7-aa61-69378e66d502","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.2262","last_updated":"2009-05-09T06:49:40Z","snapshot_observed_at":"2026-08-05T16:40:27.224469Z","submitted_at":"2009-01-15T13:43:48Z","title":"Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.2262","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, Phys","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/0901.2262","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:a4ff7f7cd552c4bc5a03ee1133628d791df8b23baa0312ab104136292cb2705f","observation_id":"a61152fe-69fd-47db-9d48-6cd19f662559","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Zhang, Phys","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:66edb816d2d04914fc978c708d7b693072ede83728405d0e01f99e304f5a02b5","observation_id":"d0d2ed9c-881f-4bd1-ad60-eca27b11615d","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.2350","last_updated":"2012-03-23T05:47:44Z","snapshot_observed_at":"2026-08-04T19:50:11.082924Z","submitted_at":"2011-12-11T13:06:29Z","title":"Holographic Ricci dark energy: Interacting model and cosmological constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.2350","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Fu, J.-F","venue":null,"work_id":null,"year":1932},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1112.2350","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:dfa10a5865558ebae9331893b89c85cc419e390cdff00be7a9de1332bee49c50","observation_id":"aef47aad-5871-4639-ae70-2d633e6b16e6","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.0716","last_updated":"2009-02-04T12:34:26Z","snapshot_observed_at":"2026-07-06T01:50:50.188825Z","submitted_at":"2009-02-04T12:34:26Z","title":"New agegraphic dark energy as a rolling tachyon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.0716","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/0902.0716","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:5d83d8e37d264a63c8ab5c7430c4202aad291d3b8dedccbbdc63e6125406e25b","observation_id":"549ad9da-4e8c-4725-a8e5-953cdc7d67bc","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1517","last_updated":"2008-02-11T07:55:39Z","snapshot_observed_at":"2026-07-06T01:29:48.927183Z","submitted_at":"2007-09-11T02:14:28Z","title":"Possible theoretical limits on holographic quintessence from weak gravity conjecture","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.1517","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Ma and X","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/0709.1517","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:ca712e75eb21c4ef46c0a3c3fab1026e0124a8c6da28acdb2eed9e0a879ef27e","observation_id":"074ff1b9-6c91-40b4-b1f5-f23026678158","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701405","last_updated":"2007-06-05T03:14:07Z","snapshot_observed_at":"2026-07-07T01:06:07.111737Z","submitted_at":"2007-01-14T08:32:38Z","title":"Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701405","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang and F.-Q","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0701405","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:2abdc4a249389264c56a412f618686fc4ef4b8266d7b84ac87a54a0a5938294e","observation_id":"fd48bc5a-7fc8-48b2-8d07-60e6cc13c746","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.00345","last_updated":"2017-06-21T13:26:47Z","snapshot_observed_at":"2026-08-14T21:27:34.995099Z","submitted_at":"2016-12-01T16:46:23Z","title":"Holographic Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.00345","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1612.00345","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:9a6b3dd19385e8b89a59fda792ae2339918bdf267deb3931493ff98d9e283509","observation_id":"7919e879-a790-442f-b5b9-5e2d7613677c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0307316","last_updated":"2003-09-23T20:15:35Z","snapshot_observed_at":"2026-07-07T00:34:55.455186Z","submitted_at":"2003-07-16T14:17:14Z","title":"Interacting Dark Matter and Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0307316","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0307316","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:3a00c3e92a20c25060b157b190e922069b2066762f713dc4e616fd1125a08f6b","observation_id":"24c933fc-787e-447d-b971-0337e9b849e6","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0411221","last_updated":"2005-12-10T08:48:23Z","snapshot_observed_at":"2026-07-07T00:45:54.523355Z","submitted_at":"2004-11-09T11:46:25Z","title":"New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0411221","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, F.-Q","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0411221","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:b8ff0bb63f3f80f4896f85d861be22926b560cc87b4f8c83ce3770c275378c3f","observation_id":"213f5726-a546-46dc-953c-e75730cbe364","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0411025","last_updated":"2005-01-08T00:55:32Z","snapshot_observed_at":"2026-07-07T04:52:20.024398Z","submitted_at":"2004-11-02T01:46:29Z","title":"Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0411025","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Cai and A","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/hep-th/0411025","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d9ab1e23f25c768aaaf4976ca4ae6519fb699885d7f9dddc8a3bf6f80b3b4a06","observation_id":"3321b2f4-1e73-4e99-a10c-e15de2089042","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0503072","last_updated":"2005-09-27T03:57:28Z","snapshot_observed_at":"2026-07-07T00:48:26.943523Z","submitted_at":"2005-03-03T13:48:47Z","title":"Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0503072","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, Mod","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/astro-ph/0503072","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:8dbd7fea27b0f58683dc6994dbca6109fba08bb23620d29258b05184b1f336fa","observation_id":"315923db-11e7-4d27-89fd-2514e5ff72e3","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Zhang, Commun","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:f55538c5bb940e20d12e6d1f65bf94d4ff7da47ca1d997db0a80f3bb1286ad2b","observation_id":"3cfdb1ee-c419-4d2f-8858-a170855add67","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Zhang, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:44767c20576b974d67f1fc098dd4d0a4831d3f9fd060c43f3ba1ede6cfbc6830","observation_id":"93f4b129-9931-4871-89fe-20f93fd47285","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e62224b95b663f595ef8ca6cf303ed71edaac86ff196797a09326020e06746fe","observation_id":"d5171afe-37ca-4251-b3a8-69ee326cbfb3","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.6135","last_updated":"2012-06-12T10:15:38Z","snapshot_observed_at":"2026-07-06T02:47:08.913365Z","submitted_at":"2012-04-27T08:14:46Z","title":"Revisit of the Interaction between Holographic Dark Energy and Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.6135","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhang, S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1204.6135","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:ccddb1a5e59aceeb5cdde8477d41e8911356bad3bb90e9f5f6e57fafb6405157","observation_id":"67140fb5-e805-4ca1-a807-7fa96c5dd491","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.7205","last_updated":"2014-12-16T23:40:24Z","snapshot_observed_at":"2026-08-14T23:18:08.711598Z","submitted_at":"2014-09-25T10:31:52Z","title":"Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.7205","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, J.-F","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1409.7205","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:77d7d2ccf72e75c1cfb25ddcc91e7741438cd1ded77c1ab81c415ea1a5c19606","observation_id":"649222d0-157e-4c8e-a38b-3056fa0e05ce","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.06349","last_updated":"2016-01-14T07:00:52Z","snapshot_observed_at":"2026-08-14T22:43:35.545124Z","submitted_at":"2015-06-21T11:18:37Z","title":"Testing models of vacuum energy interacting with cold dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.06349","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, J.-F","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1506.06349","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:27268b3b915cd9013c622db417588f2cc2c9ea51e86876e9206e4de92df801e5","observation_id":"6f6a9cba-84a8-4ca2-8f3b-c7df347f6a43","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03120","last_updated":"2020-05-06T07:25:43Z","snapshot_observed_at":"2026-08-10T23:59:57.243784Z","submitted_at":"2020-01-09T17:29:56Z","title":"Field theoretic interpretations of interacting dark energy scenarios and recent observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03120","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2001.03120","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:21520e8700f689627eae29a72bc1de30676d53bf2142035fd0a4bccabfd9c21b","observation_id":"bddf8b5d-9830-47ce-95ba-8d23c93dbab8","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05955","last_updated":"2024-05-30T07:58:59Z","snapshot_observed_at":"2026-08-13T21:07:15.374582Z","submitted_at":"2022-07-13T04:15:51Z","title":"Can interacting dark energy with dynamical coupling resolve the Hubble tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05955","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Yao and X.-H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2207.05955","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:4909947d90385b632e6ac127bbf89a9ddf0af8758bdee8e3d7e24551938e6e9e","observation_id":"2a229e3b-70c3-4664-b78a-6bd38701fc10","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.00819","last_updated":"2024-02-01T18:00:00Z","snapshot_observed_at":"2026-08-15T00:40:53.257123Z","submitted_at":"2024-02-01T18:00:00Z","title":"Further understanding the interaction between dark energy and dark matter: current status and future directions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.00819","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2402.00819","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c09a72b8aa02bdccbd22af6e6aa5477800e2ab4f4eb2d32c0e710812c6b5e4c5","observation_id":"9344820b-8578-47e2-af7f-532ba4a7e033","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.09331","last_updated":"2022-06-22T13:50:48Z","snapshot_observed_at":"2026-08-13T18:48:08.129526Z","submitted_at":"2021-02-18T13:41:35Z","title":"Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.09331","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Wang, J.-H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2102.09331","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:12f378f4c03e6bed70ed81ed360258904249f4cc20a95c0e447d925ad9c21be9","observation_id":"2f5c1119-bc38-45f8-8e77-3390ff7bf32c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04083","last_updated":"2019-06-11T10:04:20Z","snapshot_observed_at":"2026-08-14T18:01:28.256190Z","submitted_at":"2018-11-09T19:00:00Z","title":"Early Dark Energy Can Resolve The Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04083","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Poulin, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1811.04083","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d4d9027dbd0268ebf35b527c70fb079678e3465bc60d0d31ecf80674f75bf2b7","observation_id":"a4c7f945-74f7-470c-be12-338377c66fd5","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10740","last_updated":"2020-09-22T18:00:04Z","snapshot_observed_at":"2026-08-13T21:32:29.404896Z","submitted_at":"2020-09-22T18:00:04Z","title":"Early dark energy is not excluded by current large-scale structure data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10740","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2009.10740","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c41bcce7d475133c5d0d1c39c9f76fc7771823c7d5d1bc3672cea09ea5cb075f","observation_id":"f952d0db-1f9b-4cb5-a14e-763df9e69ae3","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07937","last_updated":"2023-05-13T15:01:52Z","snapshot_observed_at":"2026-08-13T11:43:17.972639Z","submitted_at":"2023-05-13T15:01:52Z","title":"Is Cosmic Birefringence model-dependent?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.07937","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2305.07937","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:abe372dfbb372c71ac88af4f8ca06641fedd543f307d02d2e85b6c059046500b","observation_id":"fbc160a2-3b74-48e0-84b0-d6ac60c9540c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.13535","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Bella, V","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2604.13535","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:a98ae02a154738f06eff72a33e2a24cdde9d64e2366e4cf8e565f52eb5411d73","observation_id":"45fb4876-1c1a-4e8b-96f0-1f5ca69d7b2f","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.02451","last_updated":"2020-04-05T02:34:54Z","snapshot_observed_at":"2026-08-14T04:45:25.021785Z","submitted_at":"2020-01-08T11:26:05Z","title":"Is the Hubble tension a hint of AdS phase around recombination?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.02451","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Ye and Y.-S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2001.02451","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:1f0cf42f17196392935b8c04882fc32e5538c914415c213b7a029530336b3538","observation_id":"81433b12-4bc3-45e0-b4de-67c8354dc6f6","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-08-09T03:11:42.668077Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.31362","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2606.31362","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:567acfffb03391a40ab4aab9ba59d2117828962a06db6e9a980d315bf8df97c7","observation_id":"ab245c72-308f-47de-aee7-2c5fd78dcbd0","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.19090","last_updated":"2026-06-17T13:58:39Z","snapshot_observed_at":"2026-07-06T23:54:27.624372Z","submitted_at":"2026-06-17T13:58:39Z","title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.19090","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Du, T.-N","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2606.19090","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:92ff594c23427717245831f9c681f5e9e4685e7c51ceb1a098cb2c99691bdc75","observation_id":"8b11427a-5849-4ca7-a083-342bc0a47735","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":"Boisseau, G","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:630c199070b985f2fc72f3cba877243fa13a0d0fbc1de5f7d8bd0527f7e0a58f","observation_id":"01acf867-1735-4bea-bc9a-38c6ebec3290","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.2476","last_updated":"2012-03-12T12:39:47Z","snapshot_observed_at":"2026-07-06T02:29:12.672489Z","submitted_at":"2011-06-13T16:06:49Z","title":"Modified Gravity and Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.2476","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Clifton, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1106.2476","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:5872a6b0c28159e60e1a4028bcbd1b9fc4f8ed1070ce8f7edae3968a488ad995","observation_id":"6ffdd5e7-8ee1-4a6f-aba1-5477bf7381ec","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.07586","last_updated":"2016-09-08T17:34:46Z","snapshot_observed_at":"2026-08-14T22:21:35.565379Z","submitted_at":"2015-11-24T06:36:47Z","title":"f(T) teleparallel gravity and cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.07586","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1511.07586","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:d17c20edc9b5a3b495ad562c8edab1c1c3c014fe8278eb0f5bda4abe2d604484","observation_id":"dce61a65-5f31-44d7-be93-b696453c34d6","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04623","last_updated":"2016-03-23T18:19:38Z","snapshot_observed_at":"2026-08-14T22:52:01.184620Z","submitted_at":"2015-04-17T20:00:48Z","title":"Cosmological Tests of Modified Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04623","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Koyama, Rept","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/1504.04623","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:7c267ad3e58b2e8d93c2a8218d5c629695829745e8d1e66a14ecfcc981e63e0c","observation_id":"7d599d4b-d4a2-4eef-a7c3-86035af898ef","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.13574","last_updated":"2024-09-11T16:01:08Z","snapshot_observed_at":"2026-08-13T10:48:12.579915Z","submitted_at":"2023-07-25T15:27:52Z","title":"Unraveling the early universe's equation of state and primordial black hole production with PTA, BBN, and CMB observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.13574","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Zhu, Z.-C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2307.13574","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:3ca8cd0faa07fb7672c1c95ae7a58bdbc2e805ddd646e64b7e6a995f175a84d6","observation_id":"9205e3e3-707b-4f17-be48-060c2ca02dce","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:3db6bce8e271ca07f7b14b83b4eb9996700c6c4fb1560b05458b5da4451ff8f0","observation_id":"2972c6df-05d9-459a-b29a-a14e6c44f810","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.21521","last_updated":"2026-03-24T13:25:09Z","snapshot_observed_at":"2026-08-15T00:32:39.868648Z","submitted_at":"2025-10-24T14:43:09Z","title":"Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.21521","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Du, J.-Y","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2510.21521","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:cf87327cd527d22e16a28ef5c4e24ebcb95ac500703de799ce841de4c097cd11","observation_id":"d4e428c2-de4f-41b4-998a-13914525fdfc","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.04494","last_updated":"2023-04-25T17:14:44Z","snapshot_observed_at":"2026-08-15T00:40:35.681086Z","submitted_at":"2022-12-08T18:59:31Z","title":"What it takes to solve the Hubble tension through modifications of cosmological recombination","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.04494","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2212.04494","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:8570967137906760bace6f5bca086f98769dfa595f754a5aae5411e70b701e04","observation_id":"58d68808-5dd3-45fc-afa1-54b05b7fb4e2","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10202","last_updated":"2024-06-14T17:37:29Z","snapshot_observed_at":"2026-08-14T14:10:26.312214Z","submitted_at":"2024-06-14T17:37:29Z","title":"DESI and the Hubble tension in light of modified recombination","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10202","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2406.10202","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:9efb5c5b701c9de73c0cc416d7a926bd0fc1729fb1a1c4271d869402e5da5177","observation_id":"46058504-4de8-4faa-bb99-98fb976e7075","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.10346","last_updated":"2025-05-20T07:28:28Z","snapshot_observed_at":"2026-08-09T08:30:01.289137Z","submitted_at":"2025-03-13T13:26:07Z","title":"Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.10346","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Song, J.-Z","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2503.10346","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:f9ab8d2fadc9a33ff7311fc8858e8a13a3eec45e6188d58075bc55934786f1f5","observation_id":"00cd1d9f-759a-4fc6-9d80-706a6319d56a","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.00133","last_updated":"2026-07-16T15:42:01Z","snapshot_observed_at":"2026-08-06T05:03:47.729461Z","submitted_at":"2026-06-30T20:12:11Z","title":"Modified Cosmology from Mass-to-Horizon Relation: Background Evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.00133","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Prasanthan, H","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2607.00133","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:1cc41180ae000b6722618ad65fde8ff7a4687c62f5939cd66d8c81fa43b5bae5","observation_id":"f23eac19-4595-41ec-83f5-4892fddbe07c","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08633","last_updated":"2025-07-28T08:54:28Z","snapshot_observed_at":"2026-08-13T00:31:06.923568Z","submitted_at":"2024-04-12T17:51:07Z","title":"Does DESI 2024 Confirm $\\Lambda$CDM?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08633","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2404.08633","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:f5006be399ff8f8af0dceb0d4b3f9416b59c546c12457878826aaf83b0bc18d9","observation_id":"7f4b088a-f296-4bd2-b180-a0b3c5ca5075","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-13T00:23:38.624395Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:c682c10d6954bbfc2212055cd0af100168fa32403bfd59b107a0a94dcca11caa","observation_id":"763e0bbc-5f4c-4f83-85da-c6b73c76ef71","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:6aa367a3d6a384aadd827b2d3ec21eac799070032c84c2cf402e16579629dc01","observation_id":"867f059f-6c89-4d73-b410-32337e597ef5","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14934","last_updated":"2024-11-12T01:42:43Z","snapshot_observed_at":"2026-08-12T23:18:03.705849Z","submitted_at":"2024-07-20T16:52:17Z","title":"Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14934","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, P.-J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2407.14934","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:b9d0903400f46c250d5c9a082a95773d12928f5df7c7b5e56f77565bb49ea3e9","observation_id":"7ae6dc0d-5ff6-4b37-8b07-9f20f87a418f","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02365","last_updated":"2024-12-11T15:46:18Z","snapshot_observed_at":"2026-08-14T16:11:05.202167Z","submitted_at":"2024-08-05T10:22:31Z","title":"Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.02365","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Jiang, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2408.02365","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:25cc7df2af1cb0367be9ce099c51b205fe53df3011a7ebd0909123b5fd40e207","observation_id":"ea5c8825-75e6-4cee-a45d-305fb30a6ace","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15640","last_updated":"2025-04-08T13:35:43Z","snapshot_observed_at":"2026-08-15T00:40:35.255401Z","submitted_at":"2024-07-22T13:59:21Z","title":"Impacts of dark energy on weighing neutrinos after DESI BAO","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15640","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Du, P.-J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2407.15640","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:993ab280eada3b378e15f8972470ebf71a38a1d7e01a61dfab8ccaadfc92d6fb","observation_id":"7c16a168-4194-4b0b-a5bb-98648cf28644","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15832","last_updated":"2025-05-11T17:25:00Z","snapshot_observed_at":"2026-08-14T08:41:49.423688Z","submitted_at":"2024-07-22T17:50:31Z","title":"Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15832","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2407.15832","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:7e5c14471822f0adf9b7082751b441c3ca935caff7b3c1217b17b531c1e15631","observation_id":"273e468f-3d0b-4d3e-92bd-fca706e7f522","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","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":"2026-07-12T04:18:55.037825Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:e9f6ad279a92e69ae7616f53f86c55256ff92119a6c63fdccf62b863816ee717","observation_id":"9f8befc0-31e0-4ea8-bcfc-d0adfcde44b3","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":239},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 100 of 239 outbound references and 1 inbound Pith citation observation for arXiv:2607.03183."}