{"as_of":"2026-08-21T16:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7c79356cc959a8a647d9f2bb926480a36abe733de91d3761a07f9580be58f425","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T16:55:48.201115Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T14:47:14.270737Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-08-08T23:50:15.048220Z","title":"Mahdavian Yekta, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04041","last_updated":"2025-04-09T09:32:16Z","snapshot_observed_at":"2026-08-14T10:18:44.484758Z","submitted_at":"2025-02-06T13:02:33Z","title":"$\\tt GrayHawk$: A public code for calculating the Gray Body Factors of massless fields around spherically symmetric Black Holes","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-08T23:50:15.048220Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2502.04041"},"observation_digest":"sha256:9c7049658c2aadedfa96d90ab00f95ed9750ffec5466abdffeb72854df390203","observation_id":"1ca26169-ffc9-47ae-acb9-439e26650365","resolution":{"observed_at":"2026-08-08T23:50:15.048220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-08-15T16:55:48.201115Z","title":"Mahdavian Yekta, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.19989","last_updated":"2025-08-27T15:48:09Z","snapshot_observed_at":"2026-08-16T17:22:42.528144Z","submitted_at":"2025-08-27T15:48:09Z","title":"Gravitational quasinormal modes of the Hayward spacetime","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T16:55:48.201115Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2508.19989"},"observation_digest":"sha256:a5bfbeabfbb15ee7ad889babf9f2ec41aef02dcdd9754d9b3dd9bb124551b159","observation_id":"f717b066-b181-462b-b5e3-1f860f6f1233","resolution":{"observed_at":"2026-08-15T16:55:48.201115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-17T14:14:00.331787Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-21T14:22:03.468102Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:1269e384fd5ffd36f3efc3076ad336cf9167bebf787a863036dd9be0cf86a25d","observation_id":"c42188b3-db73-4699-8659-d79bc3557f7e","resolution":{"observed_at":"2026-05-21T14:24:13.468615Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-17T14:14:00.331787Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":3},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-25T07:20:50.943166Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:ffe2adbede1e890cc5a4418b766fb78ee228def6a19e889d2a10d4c56878e631","observation_id":"82dbf9f7-d94d-49a9-a1c6-b0f98ee3638e","resolution":{"observed_at":"2026-05-25T07:25:29.650268Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-08-13T03:24:34.464269Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:ba92da228543486f32ce5bbc32f28b06086effded5b2f8209a03ab92ab3453ff","observation_id":"2ec468c6-44aa-4955-bf9c-73ca697c6849","resolution":{"observed_at":"2026-05-11T22:51:28.660734Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-08-13T03:24:34.464269Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:85f95932cb7f37892a89c67e6731c50f1dd3ef781a8a9c66d4897420679cd67b","observation_id":"60bd44dd-ef0c-4210-abe8-6fb1faa68e55","resolution":{"observed_at":"2026-05-14T22:19:31.337598Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2604.25471","last_updated":"2026-04-28T10:23:30Z","snapshot_observed_at":"2026-08-02T11:44:34.483229Z","submitted_at":"2026-04-28T10:23:30Z","title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:d878c5f0e5c88391c60485237695f0eb43f96c2c851ed11065e77835a0995f12","observation_id":"330f5772-2832-4762-bd40-f99d3b4b59ac","resolution":{"observed_at":"2026-05-12T00:21:17.327933Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2605.03137","last_updated":"2026-05-04T20:22:29Z","snapshot_observed_at":"2026-08-19T12:49:15.979433Z","submitted_at":"2026-05-04T20:22:29Z","title":"Scattering of scalar, electromagnetic, and Dirac fields in an asymptotically flat regular black hole supported by primordial dark matter","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-07T02:21:14.281286Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2605.03137"},"observation_digest":"sha256:561c2e91f0d030e35239e6412b1cf530583c2ad97b31c083c02f18757a1479de","observation_id":"a6f6abf2-3e50-4796-a106-4bffd40633ee","resolution":{"observed_at":"2026-05-12T10:46:30.610278Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2605.11364","last_updated":"2026-05-12T00:34:59Z","snapshot_observed_at":"2026-08-15T02:00:23.926339Z","submitted_at":"2026-05-12T00:34:59Z","title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:42b8e1176073eb1aacfdda27cfb2d571899885e6554fc9f622e170a3886f221a","observation_id":"33868d85-d1a9-42fc-9dad-3ebd3cb98f99","resolution":{"observed_at":"2026-05-13T02:42:09.058795Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2605.19463","last_updated":"2026-05-19T07:13:32Z","snapshot_observed_at":"2026-08-14T20:58:16.408223Z","submitted_at":"2026-05-19T07:13:32Z","title":"Memory burden effect of regular primordial black holes","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-20T03:07:41.621066Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2605.19463"},"observation_digest":"sha256:09bb37d48db65687e3fde51862a0d0d757f9b2592ea7be07e3108ea6c2d6fb5c","observation_id":"b66c519c-6f11-49fe-a695-4151fd744208","resolution":{"observed_at":"2026-05-20T03:08:01.694425Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2606.08631","last_updated":"2026-06-07T13:50:43Z","snapshot_observed_at":"2026-08-16T13:21:23.697442Z","submitted_at":"2026-06-07T13:50:43Z","title":"Hawking Radiation from the Dymnikova Regular Black Hole","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-27T18:03:03.482642Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2606.08631"},"observation_digest":"sha256:cfc5638eba8914ca7b018a5083e2ed9d358ecfb4a2669879da7e6347acd659ec","observation_id":"123d9702-3042-45d8-831f-e68685446e5f","resolution":{"observed_at":"2026-07-02T23:37:28.076097Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":"Mahdavian Yekta, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:75e7ecaef69560f575a3ef03d399160886dd0e573824e09e7cba8fd21416c808","observation_id":"0b3c42c9-f062-4ada-95b3-28c8720ad8c6","resolution":{"observed_at":"2026-07-12T01:38:05.217536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-08-02T08:53:13.150828Z","title":"Mahdavian Yekta, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.150828Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:66c13dfbee79472af4898af9fbf3a16606b8d4b836fa544f1f37276960f3a081","observation_id":"8ae8b338-291e-4617-9ad9-f99e22c75497","resolution":{"observed_at":"2026-08-02T08:53:13.150828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius","version":3},"cited_work":{"arxiv_id":"1912.12017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.12017","snapshot_observed_at":"2026-07-10T14:47:14.270737Z","title":"Mahdavian Yekta, M","venue":"hep-th","work_id":"9a478adc-7c71-439d-8e48-320d5e0719e9","year":2019},"citing_paper":{"arxiv_id":"2607.07955","last_updated":"2026-07-08T22:22:08Z","snapshot_observed_at":"2026-08-16T03:05:03.842686Z","submitted_at":"2026-07-08T22:22:08Z","title":"Wave and particle probes of a regular T-duality-inspired black hole with gravitational self-energy","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-10T14:46:36.212660Z"},"links":{"cited_paper":"/paper/1912.12017","citing_paper":"/paper/2607.07955"},"observation_digest":"sha256:e6503e436d53f1f417775b607c85728c8b3ab17241cf9f94d30e41c74f48727f","observation_id":"ee49a623-8458-4dd5-a47d-b9e219dda586","resolution":{"observed_at":"2026-07-10T14:47:14.271985Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1912.12017/citation-record","integrity":"/paper/1912.12017/integrity","json":"/paper/1912.12017/citation-record.json","paper":"/paper/1912.12017"},"outbound":[],"paper":{"arxiv_id":"1912.12017","last_updated":"2021-10-22T16:45:20Z","latest_version":3,"primary_category":"hep-th","snapshot_observed_at":"2026-08-07T13:59:49.462065Z","submitted_at":"2019-12-27T08:01:41Z","title":"Quasinormal modes for non-minimally coupled scalar fields in regular black hole spacetimes: Grey-body factors, Area spectrum and Shadow radius"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1912.12017."}