{"as_of":"2026-08-08T04:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:11c11d3d41e30f5209c32fd15c91256638ebd2ae5c8ac207774f2e965eb80f54","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:54:43.407504Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T22:30:10.416729Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-08-07T00:54:43.407504Z","title":"Montani, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.12709","last_updated":"2025-07-01T13:57:37Z","snapshot_observed_at":"2026-08-07T02:56:57.904130Z","submitted_at":"2025-06-15T03:43:47Z","title":"Constraints on Dark Energy Models Using Late Universe Probes","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T00:54:43.407504Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2506.12709"},"observation_digest":"sha256:e35b043c77fb517deab825ef3852bf54d4d24a7dd8434cabc8e57713a51abc53","observation_id":"65dc56ea-f1bb-401b-a993-b7c49e474938","resolution":{"observed_at":"2026-08-07T00:54:43.407504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-08-06T16:26:13.224523Z","title":"Montani, N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.13890","last_updated":"2026-07-08T08:28:20Z","snapshot_observed_at":"2026-08-06T16:11:58.333797Z","submitted_at":"2025-07-18T13:07:38Z","title":"Investigating $f(R)$-Inflation: background evolution and constraints","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T16:26:13.224523Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2507.13890"},"observation_digest":"sha256:39e5a08b2cabfa5b5d6d90f1a008f1c142b67d317d0d8520a1386a15f7ca1f74","observation_id":"3e336c10-cb83-4709-a0ce-4e7e696f7014","resolution":{"observed_at":"2026-08-06T16:26:13.224523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-08-06T05:29:02.010016Z","title":"Montani, N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-06T05:43:25.921944Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.010016Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:59521cd49ddba452f314d77bf7af317751ae0655e7a315fc42e190d48830a98f","observation_id":"ad815fa9-5887-4f99-88a4-7e868a3072d5","resolution":{"observed_at":"2026-08-06T05:29:02.010016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-08-04T12:53:53.726107Z","title":"Montani, N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":244,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:53.726107Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:958329a5cc9b1df0665f216f3dc7f058b1134690475824791c9803cab4c244be","observation_id":"5157ac6a-cb8f-4a92-b8f3-840b97f330ae","resolution":{"observed_at":"2026-08-04T12:53:53.726107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":"2404.15977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-04T22:30:10.416729Z","title":"Montani, N","venue":null,"work_id":"be6449c8-1294-4245-88f0-97198018d900","year":2024},"citing_paper":{"arxiv_id":"2511.09467","last_updated":"2026-03-30T07:50:13Z","snapshot_observed_at":"2026-08-03T06:16:33.350640Z","submitted_at":"2025-11-12T16:39:04Z","title":"Revisiting the Hubble tension problem in the framework of holographic dark energy","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-17T22:17:32.138764Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2511.09467"},"observation_digest":"sha256:e2ffe653ade99a14d1e6ea9f709d23a9633eda461b3821ee8fc54dee07070349","observation_id":"b1b803ce-a5fe-4e69-b281-ae264bb5b99e","resolution":{"observed_at":"2026-05-17T22:20:23.287326Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":"2404.15977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-04T22:30:10.416729Z","title":"Montani, N","venue":null,"work_id":"be6449c8-1294-4245-88f0-97198018d900","year":2024},"citing_paper":{"arxiv_id":"2601.14222","last_updated":"2026-04-27T15:45:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-20T18:32:34Z","title":"Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension","version":2},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-05-16T12:15:01.997389Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2601.14222"},"observation_digest":"sha256:1509f591adc668b6e590d6fb791831b7f610ee9acf667368d8379fa689c1c1e6","observation_id":"e9308d4e-3cb7-4b34-862e-e7be8b0a6a01","resolution":{"observed_at":"2026-05-16T12:17:52.476885Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":"2404.15977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-04T22:30:10.416729Z","title":"Montani, N","venue":null,"work_id":"be6449c8-1294-4245-88f0-97198018d900","year":2024},"citing_paper":{"arxiv_id":"2603.21125","last_updated":"2026-03-22T08:46:57Z","snapshot_observed_at":"2026-07-06T22:50:01.539214Z","submitted_at":"2026-03-22T08:46:57Z","title":"Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-15T01:30:47.614992Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2603.21125"},"observation_digest":"sha256:7a60c210170da699feef446dbeb294d958de23df136a9929c8f05900f11eb401","observation_id":"fe3fa85b-775f-43f0-a779-b817909e05c3","resolution":{"observed_at":"2026-05-15T01:33:27.423121Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":"2404.15977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-04T22:30:10.416729Z","title":"Montani, N","venue":null,"work_id":"be6449c8-1294-4245-88f0-97198018d900","year":2024},"citing_paper":{"arxiv_id":"2604.21670","last_updated":"2026-06-10T15:20:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-23T13:36:10Z","title":"Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-04T22:27:16.736476Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2604.21670"},"observation_digest":"sha256:b91b6c142861e55a8f884b0e4cac5891ae1d5015916df6ed93316346f5f653e6","observation_id":"658adbb7-7301-4c3d-bc93-1d566934e384","resolution":{"observed_at":"2026-07-04T22:30:10.418231Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":"2404.15977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-04T22:30:10.416729Z","title":"Montani, N","venue":null,"work_id":"be6449c8-1294-4245-88f0-97198018d900","year":2024},"citing_paper":{"arxiv_id":"2604.21671","last_updated":"2026-04-23T13:36:31Z","snapshot_observed_at":"2026-07-06T23:08:14.631453Z","submitted_at":"2026-04-23T13:36:31Z","title":"Saturation Mechanisms in the Interacting Dark Sector","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-08T14:11:14.739262Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2604.21671"},"observation_digest":"sha256:2ed8a9757d2de8b13249145d977a5c3dbe3ef31b66b659043c289a1232a074aa","observation_id":"3a85a182-e221-4f09-9beb-d42ce357f692","resolution":{"observed_at":"2026-05-11T18:46:07.192421Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-07-12T08:56:43.854989Z","title":"Montani, N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.01199","last_updated":"2026-07-08T16:43:07Z","snapshot_observed_at":"2026-07-12T08:56:43.337266Z","submitted_at":"2026-07-01T17:32:58Z","title":"Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition?","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-12T08:56:43.854989Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2607.01199"},"observation_digest":"sha256:4b5f8928d5ac5b255932bef97a8d96933c9a6975618e29778ac3a897d754926b","observation_id":"430eb667-7843-404c-b996-babe9c60c3ce","resolution":{"observed_at":"2026-07-12T08:56:43.854989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.15977/citation-record","integrity":"/paper/2404.15977/integrity","json":"/paper/2404.15977/citation-record.json","paper":"/paper/2404.15977"},"outbound":[],"paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2404.15977."}