{"as_of":"2026-08-07T16:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e64b529bbf3757a0436ce7d5d28ba7f9284865463927fbd2298593b4700750c4","coverage":[{"denominator":112,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T17:49:09.486240Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/2508.16693/citation-record","integrity":"/paper/2508.16693/integrity","json":"/paper/2508.16693/citation-record.json","paper":"/paper/2508.16693"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.336670Z","title":"Shankaranarayanan and J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.336670Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0a1377b7108777c5242b245221c092647f62ded698ce18db8701de7425d62611","observation_id":"ca74ed96-dc4f-4500-85f4-bc7be4be3408","resolution":{"observed_at":"2026-08-05T17:48:59.336670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.396102Z","title":"Clifton, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.396102Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:91deaaa469de43efb38d015b724a57ea71cbccc5ad25f3141d004bca5774d5d3","observation_id":"58bdbadb-9567-4288-ae4e-eae8a9f41486","resolution":{"observed_at":"2026-08-05T17:48:59.396102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.453393Z","title":"Nojiri and S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.453393Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:48c9b8440402ab41bd02e805b1d6bca2e3bf65440059fb2cd5aa0055e37fed18","observation_id":"ebce4a28-d506-403c-8810-3054a43aa60c","resolution":{"observed_at":"2026-08-05T17:48:59.453393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.530551Z","title":"Myrzakulov, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.530551Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:3f715aff9c8cad3a9abcf574ce6cdc6b4b6de91751a92e35e3e9523f517b7ee4","observation_id":"349b1513-fed3-43bc-a8eb-9e8e34cf5f76","resolution":{"observed_at":"2026-08-05T17:48:59.530551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.630737Z","title":"Ahmed, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.630737Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:77536d07a36057ec234a69f8b27af40edae8b7e0592a642c50f6e82c8ba4f9f6","observation_id":"0b30b93d-2b74-409d-9cb1-dbd10d22a66a","resolution":{"observed_at":"2026-08-05T17:48:59.630737Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.686389Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.686389Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:d45ba01ea43098ffe68565a968f5e6cd82d3e9fbd4bba510a0d7ea370aa1cda4","observation_id":"3daa2a72-92f2-47d3-82f8-c3db8f2873f9","resolution":{"observed_at":"2026-08-05T17:48:59.686389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.774568Z","title":"Weinberg, Rev","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.774568Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:e17942ecf60c0295071a4bb5ab69191e295098a0a09ffbb90e35f5d5f25fc254","observation_id":"8dcdf324-ac8a-4a98-a234-69f30e9e0f05","resolution":{"observed_at":"2026-08-05T17:48:59.774568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.826311Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.826311Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:141828c0040e8aa8dfe075e7c8bdbd7f21428f19ad9c055dade41b0679468da2","observation_id":"2c7c53ef-d3cd-4a81-a80f-cd025a226ce7","resolution":{"observed_at":"2026-08-05T17:48:59.826311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.898617Z","title":"Padmanabhan, Phys","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.898617Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:7e7440e6ea2fbcc2eabd6b03ab50e9d4d138c5ced36a618545012728319fec46","observation_id":"45247266-bd0a-4a4b-ba03-f42357939184","resolution":{"observed_at":"2026-08-05T17:48:59.898617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.952899Z","title":"Tangphati, I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.952899Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:18b35da6666ba2705d400186b24f8b9bc6111e1a77652755f09c1efbf75e2903","observation_id":"4798d300-29bb-4521-9838-f8a037fce3b2","resolution":{"observed_at":"2026-08-05T17:48:59.952899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:48:59.999825Z","title":"al-Badawi, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-05T17:48:59.999825Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:61343bc4478afd0030b5f0ef15a6066af1a3f1f77f300d23309ddc7f6c290388","observation_id":"afec2376-04a8-48ba-8739-fffd13ee7aea","resolution":{"observed_at":"2026-08-05T17:48:59.999825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.110577Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.110577Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:6c679704718f465e26f0037dc3d7b37404e01f2594edb179f763268fe9c75ddc","observation_id":"3c7c02d3-25b0-4ce2-9320-5c88dbf35f6d","resolution":{"observed_at":"2026-08-05T17:49:00.110577Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.184489Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.184489Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:90a9ff81cfc947c848ff962001c421df64f8bb410129f48b21262a1c79eb0296","observation_id":"d0c823ad-0d8a-48ca-82d8-cd0d8bd24bf2","resolution":{"observed_at":"2026-08-05T17:49:00.184489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.277792Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.277792Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:211ec6440e2876f692c390718d0f88a8083e20b52303da875c4e262dac137de8","observation_id":"50705918-8332-4477-a36a-7fb20b890ebb","resolution":{"observed_at":"2026-08-05T17:49:00.277792Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.340157Z","title":"Kalb and P","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.340157Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:6f941bcbb86e8da42a04429c90ba0c87f1cdd00a2669c5474a7bbd980580aac0","observation_id":"3dcbb007-4e4f-49d3-8229-63897994219f","resolution":{"observed_at":"2026-08-05T17:49:00.340157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.443303Z","title":"Witten, Nucl","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.443303Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:af1d796000cc87ecaf8b1c23ceda3c39537e4ea5235ef0a6d38ec8e26fefb488","observation_id":"98b7d312-c948-4b89-8d44-c65ae33b8f66","resolution":{"observed_at":"2026-08-05T17:49:00.443303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.537643Z","title":"Al-Badawi, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.537643Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:d0aa760e21a8e4aac7b0b59c413e48c17c344f46212f11e511bae46ceefa0ed6","observation_id":"88745a30-6993-447b-9d8a-d0d763922b4a","resolution":{"observed_at":"2026-08-05T17:49:00.537643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.659721Z","title":"Colladay and V","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.659721Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:3a7b50f91555e49f840970f228136684263e8114b7b3ac90e27c98419daf7917","observation_id":"8399fd09-9738-4af6-8964-94e6cadf6899","resolution":{"observed_at":"2026-08-05T17:49:00.659721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.810260Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.810260Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:8d6627c02e701f042e09d663c766aa81e81719f1eb2aa3b277638dc9fa942b6a","observation_id":"e4f905a6-84d1-4de6-bc30-dfd2055f6f96","resolution":{"observed_at":"2026-08-05T17:49:00.810260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:00.926094Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:00.926094Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:1476f73936a690a23c24be8ea6245bc9ffb9e4689261e4cdcb367f170fddee1e","observation_id":"1105364d-72bc-456f-afd6-49d7e30bfac0","resolution":{"observed_at":"2026-08-05T17:49:00.926094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.013371Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.013371Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:8cfd9e1b5fe146b51db3739a41ecc6c3be6cb0391c8ce3daf9c216a5fc138ea3","observation_id":"347555fe-0ea6-4de5-8486-402af6b3a2b1","resolution":{"observed_at":"2026-08-05T17:49:01.013371Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.176280Z","title":"Sahni and A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.176280Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0d9ef40502983c9684fa48521db936a8060150d9d5947704eefb0f56d9a7e1a0","observation_id":"47cc5e1a-adb4-4958-9426-a7c3ea67a0cb","resolution":{"observed_at":"2026-08-05T17:49:01.176280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.320123Z","title":"Amendola, Phys","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.320123Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:cad432f59db77361d62cbb9664b78b186dabc52deb8dbbb12369a825b40f03eb","observation_id":"c1f1f102-dfa8-422a-a1cd-53feccfae717","resolution":{"observed_at":"2026-08-05T17:49:01.320123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.425300Z","title":"Tsujikawa, Class","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.425300Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:8c452e879df01f204552b4519195113e764ee497640c6fe00ad18669cb56af39","observation_id":"d87e5f79-84bd-41f4-853e-2f66dc21c343","resolution":{"observed_at":"2026-08-05T17:49:01.425300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.565904Z","title":"Jacobson and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.565904Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:711b33cb6587e20e8d04b7110f778828ce396155f912c00410e02739f57fb09c","observation_id":"be9829c5-efa9-420a-ad61-64388da940b5","resolution":{"observed_at":"2026-08-05T17:49:01.565904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.702222Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.702222Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:b4a0e04ffa32ccd878bd3460bd208fde444c2a9ed4763ff54fe0b4c4ed768c26","observation_id":"1923c1d1-24f3-4083-8f82-b35899bc743b","resolution":{"observed_at":"2026-08-05T17:49:01.702222Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.821720Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.821720Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:19146a63d77ab93aea85071ac003f39680c563c88ebddc06da7d77098cf2d2c8","observation_id":"acfb417a-3fbb-4495-a6a1-3b6a4a0c7675","resolution":{"observed_at":"2026-08-05T17:49:01.821720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:01.958171Z","title":"Fernando, Gen","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:01.958171Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:361af3e8289d704cdeb504acfea05a29ee82ec56e502eab0fca2375d5dfc9497","observation_id":"4a71fb03-33aa-4e32-97db-fa70fb7fcb94","resolution":{"observed_at":"2026-08-05T17:49:01.958171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.057271Z","title":"Azreg-Ainou, Eur","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.057271Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:a173eea688927685c25ea19c64fa7dbea13b3e354214e94d2e39a1937a933169","observation_id":"7bf74207-6684-4975-8bc9-9b7ac59f8cc8","resolution":{"observed_at":"2026-08-05T17:49:02.057271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.171642Z","title":"Ahmed, ˙I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.171642Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:ef349f6eea5484f586dc669d5a133ae64c953eafecb319f55045b236cc0ad435","observation_id":"7da2c135-e00f-49a0-9b6c-1d6e4312bcf8","resolution":{"observed_at":"2026-08-05T17:49:02.171642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.295579Z","title":"Mangut, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.295579Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:295eecb8c8fc55d554a96c6fdc44cbf2faa997a83b8eb58105b9f415fa458b11","observation_id":"bab5a601-946b-445a-8401-37f9fd633958","resolution":{"observed_at":"2026-08-05T17:49:02.295579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.349080Z","title":"Rovelli, Quantum gravity (Cambridge University Press, Cambridge, 2004)","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.349080Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:5460f81fc5fd41a78678d2eda51d3d17cc33d490e4e61ac025eee3fefdd40163","observation_id":"44f6d191-b512-4f6c-b92a-4b17c5c30bfb","resolution":{"observed_at":"2026-08-05T17:49:02.349080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.414650Z","title":"Kempf, G","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.414650Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:f46ea0c7312d5d23f9bc2eaf58614bc24553904d9730956680f6a73c87a7fcc2","observation_id":"c479d955-594a-44b1-a32c-825386d5a9e0","resolution":{"observed_at":"2026-08-05T17:49:02.414650Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:23.690096Z","title":"Ahmed, A","venue":null,"work_id":"9ba19726-80ab-42b4-afe6-f8ea3c626138","year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.460461Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0d418da7515956752d6edbd9249649b2e046172abd39157ec1b4d252dc887035","observation_id":"d67f8136-bb6c-47cd-8235-aabf03271dd2","resolution":{"observed_at":"2026-08-05T17:49:23.757573Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:23.482190Z","title":"Bambi, Rev","venue":null,"work_id":"f0c0eb84-c8d3-4e95-bfb1-eb70ac51552a","year":2017},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.520684Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:f32161633fb46dc85a085453d1f6b84ab51e00f39dce5fc8fde23ab17405252b","observation_id":"860c8445-c4e3-4ffe-9c90-908a2dae1a7a","resolution":{"observed_at":"2026-08-05T17:49:23.590529Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:23.262097Z","title":"Akiyama et al","venue":null,"work_id":"56392a24-a2fe-466a-b97c-8db1aa72ceda","year":2019},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.585952Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:88659aac67a1ded0a82e316cdba2b7ff4bf8ef9f0413bb1b3b18a179940948ff","observation_id":"3ddba59a-ad15-4af0-aff0-190181098946","resolution":{"observed_at":"2026-08-05T17:49:23.351798Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:23.068198Z","title":"Narayan, M","venue":null,"work_id":"8bc71412-f640-47b0-82a7-db9d60b56fb9","year":2019},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.663008Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:b9f2b1885a1f340630b1575f6445e2ad0f65dcba11ad4400f5303d7957ceb14b","observation_id":"1a6bc88c-98b3-4dc4-b22e-c77527c275fc","resolution":{"observed_at":"2026-08-05T17:49:23.174678Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:22.828158Z","title":"Hawking, Nature 248, 30 (1974)","venue":null,"work_id":"150d327b-98d0-4f50-b59c-9404ab24ff47","year":1974},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.723616Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:cc52a7d88a3e6b1fd9723d4a12ad29bfc2e9e28d8281d6a9b29859efaf149474","observation_id":"ae0fe546-418f-491e-a136-ac26671d545e","resolution":{"observed_at":"2026-08-05T17:49:22.954151Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:02.778450Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.778450Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0093e4c38f4a4cc5b53183f84f49799709766466c350fb5a2cc00175e3fb6f91","observation_id":"bc587f85-c4cf-4214-a4b2-9b1f12cbc688","resolution":{"observed_at":"2026-08-05T17:49:02.778450Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:22.605372Z","title":null,"venue":null,"work_id":"5c5658e3-a404-4485-862b-b3a013fcb5f8","year":2001},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.858481Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:4fe91c623bfb193597301200d24e4ff9607733cbb6ece4f50f5b9e3740122ca1","observation_id":"9bc59250-1d60-488c-b6d4-fd67e1943363","resolution":{"observed_at":"2026-08-05T17:49:22.722096Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:22.412246Z","title":"Bonder, Phys","venue":null,"work_id":"bdc91d07-d441-49be-af10-024a0ad3deac","year":2015},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.922462Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:5eccbbacfb15264e0ee62db623e8d4aa1b71ae1394f24a2a770762ebab8c514f","observation_id":"d185eb46-7bac-400f-865d-1ea6383e888c","resolution":{"observed_at":"2026-08-05T17:49:22.512558Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:22.184287Z","title":"Bluhm, Lect","venue":null,"work_id":"6597097d-9ab3-459a-b90c-3449c2a8df92","year":2006},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:02.985196Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:18a1377379ebe804b3663c2922cab691c4745e8be623e7658e1e0706d14f038c","observation_id":"abbda728-e9db-4d45-b383-eaf4f21cb053","resolution":{"observed_at":"2026-08-05T17:49:22.315098Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:21.942008Z","title":"Mattingly, Living Rev","venue":null,"work_id":"967167c0-deee-4d2c-88e6-d88fa9f74560","year":2005},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.041603Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:335776003977b25f99d0b932ae4f189f5152494685fa4b8f70a2d3c863ccee06","observation_id":"fa3f1c49-b378-48da-9440-4de878eac088","resolution":{"observed_at":"2026-08-05T17:49:22.077140Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:03.164196Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.164196Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0d420b2c8e55e90bf15649105e3e5b92e33caf3dfbd3948d916d572ed4d35f02","observation_id":"1ea194d9-3866-44ee-a659-d9c6578e3614","resolution":{"observed_at":"2026-08-05T17:49:03.164196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:03.222849Z","title":"Padmanabhan, Gen","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.222849Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:88daacf0252c3a707a87c936408313fd0b0d7c4d40eab4bb49867fe278282dd9","observation_id":"9b48c319-6ada-4877-b028-4b90a49ea117","resolution":{"observed_at":"2026-08-05T17:49:03.222849Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:21.679292Z","title":null,"venue":null,"work_id":"ff55aa8c-1b78-495e-97f9-a96cf0699f18","year":2003},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.302598Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:cc2a73eda24f61698a0a6dec655f3cec10021142ced9cdf2c5d33bc7dfa2e137","observation_id":"82279518-6298-4d13-a9c1-0fbf680ef17c","resolution":{"observed_at":"2026-08-05T17:49:21.817958Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:21.456714Z","title":"Chen and J","venue":null,"work_id":"5404040b-bc17-467a-b9a9-c06271729115","year":2005},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.386389Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:fd1f13077b44dfaff2dc1f8636a21b136bcb71cc5d7961934f458dda7cfabc7c","observation_id":"737cb63f-1fd9-4e98-9de7-79e7d7f2903a","resolution":{"observed_at":"2026-08-05T17:49:21.565716Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:21.158800Z","title":null,"venue":null,"work_id":"0c4362a5-eb94-4ec4-a43a-1c39f264bf2a","year":2002},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.461086Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:e4f2184ecd1791aa978c9e41c86cdd3710be1eca0a787af75d0ce203bdf60895","observation_id":"809e2c28-6dda-4537-8e95-d61915a58796","resolution":{"observed_at":"2026-08-05T17:49:21.328402Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:20.920357Z","title":null,"venue":null,"work_id":"8de0ec28-fa19-4152-8116-91905771aeaf","year":1973},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.535548Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:145cc82bd9b5d324facc2186fb9b6f6b4e0907c4f5401e8b4e6b7abfc2d6f04a","observation_id":"bf6f47e5-1080-4f5b-94d3-52c72a261372","resolution":{"observed_at":"2026-08-05T17:49:21.041119Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:03.618863Z","title":"Penrose, Phys","venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.618863Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:10728c79e183a26530f4de610c17ee016e40fc9623826bbd208b9a5d5e5a85de","observation_id":"ad1f9504-cf72-47c4-a1f8-86a5ac72a3ac","resolution":{"observed_at":"2026-08-05T17:49:03.618863Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:20.634323Z","title":null,"venue":null,"work_id":"b2f69596-9147-408c-a305-b71da9a91a5a","year":1966},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.677700Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:d8056a23a215c93ae32a50852dcdf6e28b4eda7219674fce04770888a3dab205","observation_id":"8be83ce3-e6db-4e5e-adf8-d7fb20a27a76","resolution":{"observed_at":"2026-08-05T17:49:20.760887Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:20.358496Z","title":null,"venue":null,"work_id":"41869ada-7298-44ba-8b3e-f7211d350415","year":1984},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.777025Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:a3fb7908ee1d8a13e9345ee1b7f48015bdde1351a819d021dbca1ee0f34b966a","observation_id":"894f7a62-44f1-49f9-9401-f0139279edba","resolution":{"observed_at":"2026-08-05T17:49:20.503244Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:20.070259Z","title":"Kubiznak and R","venue":null,"work_id":"d263f0f8-1030-4577-8131-235cbe435932","year":2012},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.842525Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:1227d34cad8889aa689f1004dd611b5abd3ad6a6a9e0e10ce7529a0fe08badc2","observation_id":"c06f7fa8-f292-47bd-b5ac-314766e0d7e7","resolution":{"observed_at":"2026-08-05T17:49:20.222529Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:19.737018Z","title":null,"venue":null,"work_id":"6be3af3d-4868-4e65-988e-e66be0944b9a","year":1973},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.910921Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:fc86e3f5cf22b71cc4ae6caafa09830234969de622594ca00085e380e628a93e","observation_id":"87f3b974-0bf5-44e7-937e-9097ea4b5f85","resolution":{"observed_at":"2026-08-05T17:49:19.898073Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:19.368060Z","title":"Strominger and C","venue":null,"work_id":"c9e81bc1-0d4a-46b8-8fed-5d4c77f7cc55","year":1996},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:03.972242Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:ddadc62fcba6636e04486a0574f0b76347b3d2803c5dc906d652e4b5dd8e1905","observation_id":"37177d31-f520-40f4-a314-9f0dc7115e1e","resolution":{"observed_at":"2026-08-05T17:49:19.521595Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:19.075774Z","title":"Bambi, Black holes: a laboratory for testing strong gravity(Springer, New York, 2017)","venue":null,"work_id":"ebce414c-edd4-437b-8c27-b87b0d034606","year":2017},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.052555Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:7223f09c8e7648511946145a73f8c0211f1f9e43d575ec79765addc185f609ef","observation_id":"cb721250-9866-4343-89c6-abfad3938d8d","resolution":{"observed_at":"2026-08-05T17:49:19.209683Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:18.743629Z","title":"Hegde, A","venue":null,"work_id":"75f28973-b821-452c-85b0-b903266034e7","year":2021},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.119211Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:3d3fc110108ff03cf0253e2bf5136d2c1942c74f4d96953b1164e9f679cd9812","observation_id":"206d1456-dd13-4671-a36a-a77e0013f04a","resolution":{"observed_at":"2026-08-05T17:49:18.887245Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:18.597363Z","title":"Perlick, O","venue":null,"work_id":"d671b407-3875-4356-b3bc-8ade01894649","year":2015},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.170781Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:c3d4157f7f047022530f54d3290e5bf2a4c8159d944b86c5110d81433eb22764","observation_id":"56cf02e9-a3b9-4d5d-867f-f9e801473019","resolution":{"observed_at":"2026-08-05T17:49:18.684195Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:18.312041Z","title":"Younsi, A","venue":null,"work_id":"2b9bd86d-530d-4123-ac0e-2397e22b7d87","year":2023},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.269648Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:ef42dc1141e8a3fa0f63bd3cd12bafa98eff878b2b40a5d177f48698ec8bfcb5","observation_id":"ea9ea5b4-2e26-440f-9333-e258937dcc0d","resolution":{"observed_at":"2026-08-05T17:49:18.440072Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:18.036209Z","title":null,"venue":null,"work_id":"09c31f85-1d2e-4ce0-97cb-e8426d10eef6","year":2015},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.346967Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:fd40388f9c106255fb04d5c60d7f9cb2f597da522c38a9a100c00822cbdad957","observation_id":"69c02708-edf5-4182-ab31-fa44780f9767","resolution":{"observed_at":"2026-08-05T17:49:18.181782Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:17.745410Z","title":"Wielgus et al","venue":null,"work_id":"8648b9b8-7442-44aa-b108-e307b2f19247","year":2020},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.405109Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:b08822aa4b8da8b07c9a38345d8d555655ef65ee5089d218589d1d6c50606bc3","observation_id":"5e80a8da-450d-477e-a711-8358cfc08788","resolution":{"observed_at":"2026-08-05T17:49:17.851008Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:17.484703Z","title":"Berti, V","venue":null,"work_id":"0907951d-8f70-489b-8562-e85b2f1b55fa","year":2009},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.488264Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:02b2b712923ffef7130adf53491a8351e627dfdd9edb8b663edcc92cd6a52523","observation_id":"00d4d7fa-7646-4e5a-81bd-9548249ecbfb","resolution":{"observed_at":"2026-08-05T17:49:17.578527Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:17.412991Z","title":null,"venue":null,"work_id":"2a7cbfbc-b15d-4362-bca4-83f5ae3c99f8","year":1999},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.569627Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:2cfe788628240a357ddac8357ece1a579f7637e0e99d56ac241069d95b752fdb","observation_id":"f63dc10a-f26f-403d-84a2-f3485e91c9c1","resolution":{"observed_at":"2026-08-05T17:49:17.477506Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:17.286891Z","title":null,"venue":null,"work_id":"28abc3f8-901f-4558-9c77-d49a0ab3890a","year":1999},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.661143Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:fc57eb221450a4e16cd49a5a448db3036a39b948adb0383628e2bdc815230a81","observation_id":"35d12e79-3a46-4372-aecd-43069740f211","resolution":{"observed_at":"2026-08-05T17:49:17.341748Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:17.126302Z","title":"Cardoso and J","venue":null,"work_id":"72d3f6bd-bed5-46d6-b6d6-bb1c1cef2c43","year":2001},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.744025Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:5ef6cc0821a46f4784e23a595ab9a27978946a6643a361ae6c12b8facca52f36","observation_id":"f62d1f32-7fbb-419d-92db-fdc052ce013c","resolution":{"observed_at":"2026-08-05T17:49:17.206136Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:04.820772Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.820772Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:e31784c1ecc10fc7e1f18b825c99778f9ec63ee4e47e544e344194cf599f7f51","observation_id":"3951c8aa-341f-4ac3-b99f-efa4b5a5ec87","resolution":{"observed_at":"2026-08-05T17:49:04.820772Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:16.936490Z","title":"Chandrasekhar, The mathematical theory of black holes(Oxford University Press, Oxford, 1992)","venue":null,"work_id":"adf09184-bc1e-45fc-9674-753e59c73e0c","year":1992},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.824214Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:96e3905ab854b26f3e43d97a6f0e30e5d41549340b66bdaeb9071e696ffd14cb","observation_id":"e9c9fd94-cb8e-458c-a021-f7d67fa9ec92","resolution":{"observed_at":"2026-08-05T17:49:17.027023Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:04.828086Z","title":"Regge and J","venue":null,"work_id":null,"year":1957},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.828086Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:6882942badd8ff4724294ab1ed542f735a2d34cd0ed3411c070545fe5b11f83c","observation_id":"a95c0dc6-7438-49df-afde-4203fbc5de0c","resolution":{"observed_at":"2026-08-05T17:49:04.828086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:04.896362Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:04.896362Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:69c64e691e0087948e2a0a599742437712912b793992f28faef519aa427d2391","observation_id":"bb91ba24-1e31-4573-b0dc-07610935f3d3","resolution":{"observed_at":"2026-08-05T17:49:04.896362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:05.037353Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.037353Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:f216d7d43ef137573adc1a88db469d3a7e8723002e367c4e1c7de325853dc6ec","observation_id":"3cb07cbe-c723-44e6-bb2f-33ce72712053","resolution":{"observed_at":"2026-08-05T17:49:05.037353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:05.259528Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.259528Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:41725bcb0fc709763d4398edb13826812a898379bcd8cc87aa2a9f149499de33","observation_id":"810e046c-1aaf-41d4-b40c-5f1416b26a15","resolution":{"observed_at":"2026-08-05T17:49:05.259528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:05.440038Z","title":"Cardoso, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.440038Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:406946a6af2b46597341292dfcc63d80cb080e0095a3ee4431f0480c501ef897","observation_id":"d5ea14b8-87a4-45ab-b951-bbb6d5f2c86c","resolution":{"observed_at":"2026-08-05T17:49:05.440038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:05.553869Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.553869Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:09dd9c2503e93a1795b65285836fcfc504ce5b11baae61849f86298316858104","observation_id":"d5849699-c139-432c-bf43-316612aae8cd","resolution":{"observed_at":"2026-08-05T17:49:05.553869Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:16.740855Z","title":"Gundlach, R","venue":null,"work_id":"7d185823-9aa7-427e-972e-d535ba6ba9cc","year":1994},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.775986Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:c7ef007956fd25e3c213ba9d8cc22b5ff737f087c5fa2985393fd111a94259ea","observation_id":"1e1ad4fe-4208-4cf2-905b-b2c50e8da981","resolution":{"observed_at":"2026-08-05T17:49:16.801269Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:16.613628Z","title":null,"venue":null,"work_id":"1db7741b-2f5d-4add-80f9-16a1f292d352","year":1995},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:05.936915Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:2d5cb43692bd8aa7e2722374b7fcdb40df841f5bbdc4f30e2535fc005e8c9500","observation_id":"34b02717-15e7-456b-84b4-99eaf48679c8","resolution":{"observed_at":"2026-08-05T17:49:16.672102Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:16.461575Z","title":null,"venue":null,"work_id":"a018487f-302a-4578-806f-a13c821fbda5","year":1973},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:06.137403Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:2085c3a339252224a75a5d34b4b0022e0108f6f6c34dd54d58d24e3a288ca58f","observation_id":"7911da81-d806-405e-b8af-f7c73559ad6c","resolution":{"observed_at":"2026-08-05T17:49:16.514804Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:06.311888Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:06.311888Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:98a4fad0533e7be860c1d08beb23d7b99d51f62df4f206aec9208d76d4ecf6ea","observation_id":"1f433d1e-01eb-4c19-90f1-48d04584b3e3","resolution":{"observed_at":"2026-08-05T17:49:06.311888Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:15.391540Z","title":null,"venue":null,"work_id":"1db57689-22ba-4ed8-9041-9de7478c236e","year":1998},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:06.493738Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:15832f250756f1af2dddb3de7be1a694eb438929867adc93ef4b22781231b327","observation_id":"e694a83d-bbe2-462f-91c5-c1f52f0d1ce4","resolution":{"observed_at":"2026-08-05T17:49:15.981578Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:15.110677Z","title":"Abramowitz and I","venue":null,"work_id":"50a076a4-39f8-4403-894f-9732c983c676","year":1965},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:06.696262Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:cd726d57f9f356e847f3182c9f8d0f7ca7466510740a0edbd195e23e5b2e0c4d","observation_id":"f9353521-5a1e-4ab7-9f62-0bc696fdf879","resolution":{"observed_at":"2026-08-05T17:49:15.210282Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.941422Z","title":"Pound, Fund","venue":null,"work_id":"8286f64d-45f6-4d6b-83d1-b1902b21ce9c","year":2015},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:06.835823Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:0befa1cb8b5fb032f2bf63f40d4c09cd4c180dc5e8a99fd3aabd24940e6ce8d0","observation_id":"86bb068e-7d16-46dd-a927-137e2cb1ae60","resolution":{"observed_at":"2026-08-05T17:49:14.999825Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.814859Z","title":"Detweiler, Class","venue":null,"work_id":"7261489a-b0ec-47cb-b5a5-6257f03e95a2","year":2005},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.002640Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:602ffbb37193eb52167874f2664f77de4ecfe3b1aa4f6f1ec2d281b6c880b3e7","observation_id":"eafc4959-eb13-435d-a74b-29102dd8fa0b","resolution":{"observed_at":"2026-08-05T17:49:14.869649Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.653195Z","title":"Barack, Class","venue":null,"work_id":"ff08db78-f921-4816-a237-102f059e7ca8","year":2009},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.142528Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:7b5e554c23ae5a8e902a4f049bbfb9dad1e94e45ceef2197a587e6cb6c553fb3","observation_id":"b0a6547e-bf86-4758-a14a-0aa768486e3a","resolution":{"observed_at":"2026-08-05T17:49:14.737457Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.04592","last_updated":"2024-01-25T01:29:56Z","snapshot_observed_at":"2026-08-05T17:07:29.093973Z","submitted_at":"2021-01-12T16:44:53Z","title":"Black hole perturbation theory and gravitational self-force","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.04592","snapshot_observed_at":"2026-08-05T17:49:07.221709Z","title":"Pound and B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.221709Z"},"links":{"cited_paper":"/paper/2101.04592","citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:db46a156c7566e1749bff3233a169af636f3071f40d97b617225629caec4aeb4","observation_id":"035b60d4-c84e-4f25-8f84-a5ce7b554506","resolution":{"observed_at":"2026-08-05T17:49:07.221709Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.471604Z","title":null,"venue":null,"work_id":"f0c66ada-4224-434f-b2d0-19f6784c7705","year":2012},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.414809Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:e227b3781b6d57e3de66b497c858cc3f5d10f0274140454511089073bb3e518a","observation_id":"b212434f-0061-4066-845d-09901c4bd667","resolution":{"observed_at":"2026-08-05T17:49:14.532348Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.324680Z","title":"Schneider, J","venue":null,"work_id":"7306dc1f-0a12-4244-8f60-3296d354c131","year":1992},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.546737Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:48e671a55d92ecec2498fd746d8a33ac88fd08fb9a2a8ee839f6b1fb3946c053","observation_id":"3a08575e-aca1-4f0e-9b54-7bed643c879c","resolution":{"observed_at":"2026-08-05T17:49:14.397763Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:14.130930Z","title":null,"venue":null,"work_id":"4d03e0f1-2da2-4e57-9972-86602208da36","year":2005},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.680320Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:b97db41c66e8cf6eb4558a7500fdbc5fda1d925226da575f17c67aa28cab35de","observation_id":"d897f076-01f2-4419-887f-099e8e8cd1c3","resolution":{"observed_at":"2026-08-05T17:49:14.244761Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:07.813316Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.813316Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:4f6a4921326608e829d01f5289b97b6419cfef7dc66f566aa0dec24f84076042","observation_id":"274de566-8815-4c17-b006-1a7505b35450","resolution":{"observed_at":"2026-08-05T17:49:07.813316Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.849259Z","title":null,"venue":null,"work_id":"986a6715-5633-4e7a-bb42-68374cce5520","year":2012},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:07.915584Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:2ef7c4e63a4323a9c3ae36caaa6b0a5dff76a01cad383fd562507ed2b2a1e324","observation_id":"ca96372c-b6d4-4f30-9438-462cd927b057","resolution":{"observed_at":"2026-08-05T17:49:14.052660Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.693159Z","title":null,"venue":null,"work_id":"35f9746e-f228-43b5-ab0b-f1cf3410393a","year":2019},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.082326Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:36b324f0187ad55425445ba6dd434750ed28a36bee721512c8f3bcf2b2d44652","observation_id":"c47119d2-4206-4532-a1f4-a44bdf0784b9","resolution":{"observed_at":"2026-08-05T17:49:13.767164Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.547158Z","title":"Sucu and ˙I","venue":null,"work_id":"52e3ffd3-69da-4e55-891e-a598da1b27d5","year":2025},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.215429Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:580ec3e57e7ae3d7effec7a1200226a6a3259b38de719bd09dc05d0fe9fb76b5","observation_id":"2f582b85-40f5-4b87-81d6-f454ebbdda63","resolution":{"observed_at":"2026-08-05T17:49:13.632312Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:08.371318Z","title":"Li and A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.371318Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:337ef6f0d538902c8f203133633bf5a9a755487d1210a1bf79c45046a63fbd35","observation_id":"dd36837b-28f5-41b0-bcf7-d2abaa7f8f65","resolution":{"observed_at":"2026-08-05T17:49:08.371318Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.398613Z","title":"Arakida, Gen","venue":null,"work_id":"2062ee05-0e4d-46c9-b97b-4ebb22cf26c9","year":2018},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.495190Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:c77a03fe917215d3f5016e6ff076d893f3188297003e66c7006fdbfd32b5f9ee","observation_id":"f7a3f33d-a52d-4e3f-b81d-775357f5b7a1","resolution":{"observed_at":"2026-08-05T17:49:13.475077Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.221637Z","title":null,"venue":null,"work_id":"c28dc567-fe9f-43ac-8a4b-d31a2f3b76e9","year":2018},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.614875Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:3f917d53aaf3204139e0671c50ea502c0ab084e01dcfada985d28d2b2d9d6aca","observation_id":"31e74280-7adf-4540-8850-3380a3d8bedd","resolution":{"observed_at":"2026-08-05T17:49:13.324480Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:13.084204Z","title":"Chamblin, R","venue":null,"work_id":"93edbf62-8f4b-45a0-ba5f-dfdb4fd0b8be","year":1999},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.792732Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:a5ac907eaefb36f19e12334b438c3f8be4761f0541e89e9f9d81ac7147409eab","observation_id":"17f4c0d3-c1f4-4620-962f-316af9cf0a8f","resolution":{"observed_at":"2026-08-05T17:49:13.151767Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:12.909714Z","title":null,"venue":null,"work_id":"0c2b8a37-bec5-4dd5-a817-c53c7942e859","year":2000},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:08.965790Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:98de70e2c4bee7f58389830af4954ca8c952baccd27a585b9ab151b48c2a6383","observation_id":"7c012ed6-6e15-4465-b3fb-770153f22d26","resolution":{"observed_at":"2026-08-05T17:49:12.990023Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:12.714731Z","title":"Kastor, S","venue":null,"work_id":"3f735ec3-bfca-4c5e-944b-0bd4a35bf259","year":2009},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:09.115562Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:537212f8069d44c8338244292fef86f714bcb641cb2e68c98e1d77e38b4cba83","observation_id":"048dc13f-a05f-4891-9b88-2a9dec94bd9c","resolution":{"observed_at":"2026-08-05T17:49:12.807510Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:12.499786Z","title":null,"venue":null,"work_id":"f79d6e24-e314-41a7-aff5-e19476e77bfb","year":2011},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:09.194618Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:a880230d3c0846d26cdbae27c31478723fbded36e83a7ef3682c6de957210959","observation_id":"8646eacb-a79d-4db4-93fd-50d4ee7c830b","resolution":{"observed_at":"2026-08-05T17:49:12.611834Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:12.354892Z","title":"Rajagopal, D","venue":null,"work_id":"e3d17a0c-c864-4407-989e-f0617f21b6f0","year":2014},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:09.291814Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:116d190410c1289628af4a8e39d0bbae763ccf390d27690cb60706ce5c2efd6b","observation_id":"3bb6d6ef-16cb-434b-a896-2db06be11b89","resolution":{"observed_at":"2026-08-05T17:49:12.405005Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:09.383816Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:09.383816Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:a7ce9c06c232a0ef59de45f7000bca61050542835a0a72ec5d7e0a596718b414","observation_id":"f19cfc8f-de9c-4b83-bcd7-cbc289d8afaf","resolution":{"observed_at":"2026-08-05T17:49:09.383816Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T17:49:12.205495Z","title":null,"venue":null,"work_id":"b17eefed-d5de-44b7-89bc-b2930ebc7fee","year":1976},"citing_paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-05T17:49:09.486240Z"},"links":{"citing_paper":"/paper/2508.16693"},"observation_digest":"sha256:48bf2193cbd6d10b2163d3dc2bd59cec8582803aad02cf1e3bdbad5852c6f633","observation_id":"b1fd1b83-caf6-4e7a-aff5-0318c302dff7","resolution":{"observed_at":"2026-08-05T17:49:12.278506Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2508.16693","last_updated":"2025-08-27T23:13:17Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-05T17:48:43.508342Z","submitted_at":"2025-08-21T21:51:31Z","title":"A Black Hole Solution in Kalb-Ramond Gravity with Quintessence Field: From Geodesic Dynamics to Thermal Criticality"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":70,"verified_exact":0,"verified_fuzzy":30},"total_outbound_references":112},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 100 of 112 outbound references and 0 inbound Pith citation observations for arXiv:2508.16693."}