{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","short_pith_number":"pith:MVXLCIYZ","canonical_record":{"source":{"id":"2607.09240","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-10T09:36:20Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"61e95cf695d210969ea632371ece02453cc2a07acf23244d36193020e9b9368b","abstract_canon_sha256":"106b737fbf5932c2b9225063e656bd0817fc40894586966d5f4e2e2ee7c5948d"},"schema_version":"1.0"},"canonical_sha256":"656eb12319ec52e9127ee87d775dbf709a3d205fd96410399c32b3c2887d2be9","source":{"kind":"arxiv","id":"2607.09240","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2607.09240","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"arxiv_version","alias_value":"2607.09240v1","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.09240","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_12","alias_value":"MVXLCIYZ5RJO","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_16","alias_value":"MVXLCIYZ5RJOSET6","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_8","alias_value":"MVXLCIYZ","created_at":"2026-07-13T01:18:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"record","payload":{"canonical_record":{"source":{"id":"2607.09240","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-10T09:36:20Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"61e95cf695d210969ea632371ece02453cc2a07acf23244d36193020e9b9368b","abstract_canon_sha256":"106b737fbf5932c2b9225063e656bd0817fc40894586966d5f4e2e2ee7c5948d"},"schema_version":"1.0"},"canonical_sha256":"656eb12319ec52e9127ee87d775dbf709a3d205fd96410399c32b3c2887d2be9","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-13T01:18:54.877945Z","signature_b64":"H6cd5JgjO1fFrpfvI3s0P+ka3uS97om2uzNxX+uDip+PdVRqpXYdpgm8SqdH1zYd6G5dPN2pPhzbuAqr6l1aAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"656eb12319ec52e9127ee87d775dbf709a3d205fd96410399c32b3c2887d2be9","last_reissued_at":"2026-07-13T01:18:54.876526Z","signature_status":"signed_v1","first_computed_at":"2026-07-13T01:18:54.876526Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2607.09240","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T01:18:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"0r6CQMZRNAXPydFoSZ9HZRPWK6nC/rRD/RhZvT+vSg5fHo5M4+2JaXiN3wKPbK07NvJpZxE6EiHmYUownkOUDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.576014Z"},"content_sha256":"d84a2cc4658662661da7ea5b88ed64da597a0e64cbc18b145cc39dd8f1263deb","schema_version":"1.0","event_id":"sha256:d84a2cc4658662661da7ea5b88ed64da597a0e64cbc18b145cc39dd8f1263deb"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Xinyi Dai, Yicheng Wang, Yupeng Yang","submitted_at":"2026-07-10T09:36:20Z","abstract_excerpt":"We present updated constraints on both flat and non-flat Dvali-Gabadadze-Porrati (DGP) cosmological models using the latest baryon acoustic oscillation (BAO) measurements from the Dark Energy Spectroscopic Instrument Data Release 2 (DESI DR2), in combination with cosmic chronometer (CC), Type Ia supernova (SNIa), and cosmic microwave background (CMB) distance priors. For the non-flat DGP model, we obtain $H_0 = 64.05 \\pm 0.27\\, \\rm{kms^{-1}Mpc^{-1}}$, $\\Omega_m = 0.3264 \\pm 0.0043$, and $\\Omega_k = 0.0088 \\pm 0.0016$, corresponding to a transition redshift $z_t \\sim 0.41$. For the flat case, t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.09240","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2607.09240/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T01:18:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"jKbyzfKstwfvJGWD5Um0+MqQTeUhIG/55c6DBPQHxYKV9Y/RxeU6i/J6Q27zk++Dcr+algqbK7TZCV0F/902Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.576451Z"},"content_sha256":"32839f1b0daf48f4c43701c2142833eee46a70575b153249ed7483104c898151","schema_version":"1.0","event_id":"sha256:32839f1b0daf48f4c43701c2142833eee46a70575b153249ed7483104c898151"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1051/0004-6361/202452185.arXiv:2409.03523) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"G. Rácz, et al., Euclid preparation - LXIII. Simulations and non-linearities beyond Lambda cold dark matter. 2. Results from non-standard simulations. Astron. Astrophys.695, A232 (2025). https://doi.org/10.1051/0004-6361/ 202452185. arXiv:2","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":78,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"G. Rácz, et al., Euclid preparation - LXIII. Simulations and non-linearities beyond Lambda cold dark matter. 2. Results from non-standard simulations. Astron. Astrophys.695, A232 (2025). https://doi.org/10.1051/0004-6361/ 202452185. arXiv:2","reconstructed_doi":"10.1051/0004-6361/202452185.arXiv:2409.03523"},"severity":"advisory","ref_index":78,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1051/0004-6361/202452185.arXiv:2409.03523","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"69dd482938d1bcf1e3ff1392dd830d847c6bb0ae6d970e0bc88d096d937da743","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12896,"payload_sha256":"1215926a232d68f0901fba1133c179321fc1f87aa88cce4d100ce9d6287a0351","signature_b64":"QEvhSVLInzGDV3UmhNPjcnStTtEGe5qGp7yj6i4l6pb2l+6IPmK/yO68m8YseNJcmbRD/EU2uCvGVmTDL08TAg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"oDcqBzuwfCvT8hcadBYLuauDIfmlneEjcVcZsRmfWQPc2nYRkxBp19tYPvV0A35Kq9h3HMtA4i0GDWMcaYIWDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.741687Z"},"content_sha256":"3f9bd2bdad006d477a8ff754d1509489e43fc584f39389bbd2a124feafae9ecc","schema_version":"1.0","event_id":"sha256:3f9bd2bdad006d477a8ff754d1509489e43fc584f39389bbd2a124feafae9ecc"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.3847/1538-4357/adce78.arXiv:2408.06153) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"W.L. Freedman, B.F. Madore, T.J. Hoyt, I.S. Jang, A.J.Lee,K.A.Owens,StatusReportontheChicago- Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes. Astrophys. J.985(2), 203 (202","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":77,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"W.L. Freedman, B.F. Madore, T.J. Hoyt, I.S. Jang, A.J.Lee,K.A.Owens,StatusReportontheChicago- Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes. Astrophys. J.985(2), 203 (202","reconstructed_doi":"10.3847/1538-4357/adce78.arXiv:2408.06153"},"severity":"advisory","ref_index":77,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.3847/1538-4357/adce78.arXiv:2408.06153","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"5b0178bc7ca4d924ccc4aaac4658b551a1f93ff7596d6f6f7ef26f49b110338c","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12895,"payload_sha256":"900d983ca970b1098efc6f215a5117c99352fd9e94909010afa5ae2586afd49c","signature_b64":"7vzZR+wpq6tzMCFzzK7mtM0+NJA6dekaMa5FXi/vDuYNb51vInut9qQ0H/80vaS0biUll9DlfWx/IujtoWIvDA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DAau16WtOQOZMImCCNlXtBicsqc/0VcMEPeMVvb9q+dwxhlBurkbcuvgGU5HqvPz+oAtpk1UKGMwY++E0LyuAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.742045Z"},"content_sha256":"a0b6a7fb2c06d5b7da809c59d5dd649a3bb61ab938a79caaa9740d879cba4c81","schema_version":"1.0","event_id":"sha256:a0b6a7fb2c06d5b7da809c59d5dd649a3bb61ab938a79caaa9740d879cba4c81"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevD.76.123007.arXiv:0708.2977) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"Y. Gong, X. Chen, Two Component Model of Dark Energy. Phys. Rev. D76, 123007 (2007). https://doi.org/10.1103/PhysRevD.76. 123007. arXiv:0708.2977 [astro-ph] 14","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":65,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"Y. Gong, X. Chen, Two Component Model of Dark Energy. Phys. Rev. D76, 123007 (2007). https://doi.org/10.1103/PhysRevD.76. 123007. arXiv:0708.2977 [astro-ph] 14","reconstructed_doi":"10.1103/PhysRevD.76.123007.arXiv:0708.2977"},"severity":"advisory","ref_index":65,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1103/PhysRevD.76.123007.arXiv:0708.2977","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"3b6052d4078cc35072cace2dadd422187681297d893dcc79a47a28ea51d60359","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12894,"payload_sha256":"b9cb086d8c1b08f23aa32fee42cc581b2f85d166c9c26d3493c21240c958e9b0","signature_b64":"37k+KFrdDyH9c/jHGKJtXcWnfg+A+E4Rbo+F0eMFVLfTgOWg0BnHC/IsCZAUBiRwUa2YFJclhOLSZSrEWwKhCw==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"y+3pFQf6scqITrOOmUhBK/z2udvaaA5Zy7PbaHU9O8ffy/iDNq5PrfNmvZKDMxbR3B9adFzaNqcht4NRXfPwCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.742368Z"},"content_sha256":"19bfdc1685261503e8891ce3f20a39f52f53b08b8fe656e6f763f478a65db53b","schema_version":"1.0","event_id":"sha256:19bfdc1685261503e8891ce3f20a39f52f53b08b8fe656e6f763f478a65db53b"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.asr.2024.04.045.arXiv:2404.15982) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. Koussour, N. Myrzakulov, J. Rayimbaev, Cos- mological constraints on time-varying cosmologi- cal terms: A study of FLRW universe models with Λ(t)CDM cosmology. Adv. Space Res.74, 1343– 1351 (2024). https://doi.org/10.1016/j.asr. 2024.04.","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":56,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. Koussour, N. Myrzakulov, J. Rayimbaev, Cos- mological constraints on time-varying cosmologi- cal terms: A study of FLRW universe models with Λ(t)CDM cosmology. Adv. Space Res.74, 1343– 1351 (2024). https://doi.org/10.1016/j.asr. 2024.04.","reconstructed_doi":"10.1016/j.asr.2024.04.045.arXiv:2404.15982"},"severity":"advisory","ref_index":56,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.asr.2024.04.045.arXiv:2404.15982","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"72331f173f4107e31f0dd74e055fe99bee7078f04bdad512b698c193ed3be7d2","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12893,"payload_sha256":"92dd6b1a8d664fad4ee156c79ab64135d4742b07b537d6a8ec09ac22af04e22f","signature_b64":"TD94/BXHVWEl+GUd3d/n+ZCSHDcev2/jRn1RhCKOSRT247FmYacmKnNrN7HDvGlN+EinHM85d06Y9XCiNLDzAA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"RMgs0rLo9jcPp3Jv4gHL9w7UKtst3hqqyeUX/SOxIm0AZg+nkFF4sL9x8rqR0rC+ZuGNxe5+nXPieik3N1scDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.742735Z"},"content_sha256":"f96c82f6e523b19e6e3bc95f8ccf2f60ba83e4ec0ba3ad76b002c1121a1287e5","schema_version":"1.0","event_id":"sha256:f96c82f6e523b19e6e3bc95f8ccf2f60ba83e4ec0ba3ad76b002c1121a1287e5"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevD.110.123524.arXiv:2407.02558) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Chudaykin, M. Kunz, Modified gravity inter- pretation of the evolving dark energy in light of DESI data. Phys. Rev. D110(12), 123524 (2024). https://doi.org/10.1103/PhysRevD. 110.123524. arXiv:2407.02558 [astro-ph.CO]","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":53,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Chudaykin, M. Kunz, Modified gravity inter- pretation of the evolving dark energy in light of DESI data. Phys. Rev. D110(12), 123524 (2024). https://doi.org/10.1103/PhysRevD. 110.123524. arXiv:2407.02558 [astro-ph.CO]","reconstructed_doi":"10.1103/PhysRevD.110.123524.arXiv:2407.02558"},"severity":"advisory","ref_index":53,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1103/PhysRevD.110.123524.arXiv:2407.02558","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"557fcd865e640500f59b6a0f463b4fac1ccded8914bb56fd43e1fb76b6021c81","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12892,"payload_sha256":"a85b041d7caa615c8297f29cef818cffc438bf693bba611860425d3b75eecf41","signature_b64":"koFA6eDwASMnAIHIp+nfdL/DekKwRqgTYTuUVAORIGXipXfnRM3mIDRSIj0o5SfyRkvh8QYeuloFyGqDIQeVBA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"raXaGfI0lxXaWsreqOo7Vl1UDSDP1F0fT1EicyXo6UgT1duP4o0asL7FAxlwkvyfD5pe55WOIW5P9lFQ/Eu1DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.743142Z"},"content_sha256":"f9cef09e749c3179b94c267dd40c37d65864ced3dbc653f5848e4ca955538c03","schema_version":"1.0","event_id":"sha256:f9cef09e749c3179b94c267dd40c37d65864ced3dbc653f5848e4ca955538c03"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevD.66.024019.arXiv:astro-ph/020116413) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"C. Deffayet, S.J. Landau, J. Raux, M. Zaldarriaga, P. Astier, Supernovae, CMB, and gravitational leak- age into extra dimensions. Phys. Rev. D66, 024019 (2002). https://doi.org/10.1103/PhysRevD.66. 024019. arXiv:astro-ph/0201164 13","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":44,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"C. Deffayet, S.J. Landau, J. Raux, M. Zaldarriaga, P. Astier, Supernovae, CMB, and gravitational leak- age into extra dimensions. Phys. Rev. D66, 024019 (2002). https://doi.org/10.1103/PhysRevD.66. 024019. arXiv:astro-ph/0201164 13","reconstructed_doi":"10.1103/PhysRevD.66.024019.arXiv:astro-ph/020116413"},"severity":"advisory","ref_index":44,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1103/PhysRevD.66.024019.arXiv:astro-ph/020116413","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"6e0b0837e6c6cc690c4cbf84e72ad99391c74b9a9d4f794bd4df1a3638c64ffc","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12891,"payload_sha256":"ae8e58022722306b5b64763ab75ec8f9222ccdfeb1ed856acf455c04af9cd898","signature_b64":"Ewi5NxjnObHQ5LOU1oDAxFF4O6UeEt8cUkCly4yfUza9LdgHgY8GmfkPI/KA6ILW3ge785WQEhd/CnXg5hjFCA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UhCgxwP6/XwB6suyV2d+Rodnf77Z41XGQUyxcpga106/p2E7LxoayYmn/Qrjgrqn8tIo1qO2HSUcXRrgv3pHDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.743597Z"},"content_sha256":"8063c63a398665ef69f63d659ae23a170550cd67e6ae91a47a989ac52b34a0b3","schema_version":"1.0","event_id":"sha256:8063c63a398665ef69f63d659ae23a170550cd67e6ae91a47a989ac52b34a0b3"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.physrep.2005.10.007.arXiv:astro-ph/0510068) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"A. Lue, The phenomenology of dvali-gabadadze- porrati cosmologies. Phys. Rept.423, 1–48 (2006). https://doi.org/10.1016/j.physrep. 2005.10.007. arXiv:astro-ph/0510068","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":37,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"A. Lue, The phenomenology of dvali-gabadadze- porrati cosmologies. Phys. Rept.423, 1–48 (2006). https://doi.org/10.1016/j.physrep. 2005.10.007. arXiv:astro-ph/0510068","reconstructed_doi":"10.1016/j.physrep.2005.10.007.arXiv:astro-ph/0510068"},"severity":"advisory","ref_index":37,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.physrep.2005.10.007.arXiv:astro-ph/0510068","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"3eed544eda3f9b1aa2f96bcad978660b20cef6397b2654fe9609ce361f270819","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12890,"payload_sha256":"ead363165cbd5e5ccb6072fc0008bc49d51ed6dd788179b77098600673d5ba44","signature_b64":"br3i6Ools4Y91s/BdnDP312d3PAZpO7IJWU4MaLyVM85IykEPFvlxCvsdLAeWs+7z9tsF5gvgltvr/VYZ99SAw==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VheC82EWfTyElh0g+rAgzx5K+DQBptyFc4Sx3UflN96/+ZjDWetWQ5EuRXVgfU/STsNJjo3hpaMKxEWeyxeEBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.743902Z"},"content_sha256":"a8e49b1f7b006213c353706bc539320ca33d1eca1db78868a4b0173ff6842f2a","schema_version":"1.0","event_id":"sha256:a8e49b1f7b006213c353706bc539320ca33d1eca1db78868a4b0173ff6842f2a"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1103/PhysRevD.63.065007.arXiv:hep-th/0008054) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"G.R. Dvali, G. Gabadadze, Gravity on a brane in infinite volume extra space. Phys. Rev. D63, 065007 (2001). https://doi.org/10.1103/PhysRevD.63. 065007. arXiv:hep-th/0008054","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":36,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"G.R. Dvali, G. Gabadadze, Gravity on a brane in infinite volume extra space. Phys. Rev. D63, 065007 (2001). https://doi.org/10.1103/PhysRevD.63. 065007. arXiv:hep-th/0008054","reconstructed_doi":"10.1103/PhysRevD.63.065007.arXiv:hep-th/0008054"},"severity":"advisory","ref_index":36,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1103/PhysRevD.63.065007.arXiv:hep-th/0008054","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"989df853b544fad81e16f4a089b0d30638966e64b58bcdfaca3b1dd35dd02333","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12889,"payload_sha256":"6453ccfa14c4231be111a2853e2e26d39f5e328d173ff7332fc214e5a2e1cd56","signature_b64":"nMuAmERcS9JRTRFaimlj2mXggWD9Pc8PJs7Oy6zCalGo3nL4pudHIXpP1/OfU0EJ3Bx98+5dCdU+nLwIPcFUAA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PMDHLsSMz8fIyllK0TVAA0Yd3QIbv3ZuiI5TNcDOT14On9boQpSB9CZKjznlySTfIpm+phz2nfz/xjdfDajOBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.744188Z"},"content_sha256":"458b587380a1575392ed1f966674805db5fe10fd4020225ee95eadf22113175f","schema_version":"1.0","event_id":"sha256:458b587380a1575392ed1f966674805db5fe10fd4020225ee95eadf22113175f"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.dark.2023.101339.arXiv:2309.14498) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"M. Koussour, N. Myrzakulov, A.H.A. Alfedeel, F. Awad, M. Bennai, Modeling cosmic accel- eration with a generalized varying deceleration parameter. Phys. Dark Univ.42, 101339 (2023). https://doi.org/10.1016/j.dark.2023. 101339. arXiv:2309.14","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":35,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"M. Koussour, N. Myrzakulov, A.H.A. Alfedeel, F. Awad, M. Bennai, Modeling cosmic accel- eration with a generalized varying deceleration parameter. Phys. Dark Univ.42, 101339 (2023). https://doi.org/10.1016/j.dark.2023. 101339. arXiv:2309.14","reconstructed_doi":"10.1016/j.dark.2023.101339.arXiv:2309.14498"},"severity":"advisory","ref_index":35,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.dark.2023.101339.arXiv:2309.14498","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"943ed7b406ccb7810ee59a4bce643b6904ae41253bebb5d2d5b40aae8b92abec","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12888,"payload_sha256":"9871dd46bec4dea8a68d39e3c795d81e8e930c88dbdc746fe754c99128480df4","signature_b64":"y2K3Wr+NTRxuAtQscozBkdX4hrg0j95eH8qnTg/FscCfJRu48qWjydHSVH6Iao6qzmVAxGkq33qHntkvQm24Dg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5QRVgQ2W7BXoIxAhEW7ZZlXv2ZJUDnNPt0BvFs1u2mfj+rcA6/2DQbVWzAaZ8hGSCWT5UW4CbKoqxffJj6neCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.744560Z"},"content_sha256":"59828ffe88f571a36f061f0c710caf02fe1305b93e13af5f2428f8fd73dd5f4c","schema_version":"1.0","event_id":"sha256:59828ffe88f571a36f061f0c710caf02fe1305b93e13af5f2428f8fd73dd5f4c"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.cjph.2023.07.003.arXiv:2308.15101) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"N. Myrzakulov, M. Koussour, A. Mussatayeva, Quintessence-like features in the late-time cos- mological evolution of f(Q) symmetric telepar- allel gravity. Chin. J. Phys.85, 345–358 (2023). https://doi.org/10.1016/j.cjph.2023. 07.003. arXiv:","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":30,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"N. Myrzakulov, M. Koussour, A. Mussatayeva, Quintessence-like features in the late-time cos- mological evolution of f(Q) symmetric telepar- allel gravity. Chin. J. Phys.85, 345–358 (2023). https://doi.org/10.1016/j.cjph.2023. 07.003. arXiv:","reconstructed_doi":"10.1016/j.cjph.2023.07.003.arXiv:2308.15101"},"severity":"advisory","ref_index":30,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.cjph.2023.07.003.arXiv:2308.15101","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"8c80975ec795d8f41a600cea85c204b973a74afe02742e2d50772bd5b9371cc7","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12887,"payload_sha256":"21539b075b87841c10f69b957eb90b445be4c3c33523f96ed226ad77cf9850d6","signature_b64":"8/VqZYlyzP2ZxcpXQsU6D2+DW/foutcdfUkYqeXBbf9ZvYT4J49njpvNhQsA93cHKS+TbAkZ1/aZejszMvyTAg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bjNMR0YquWgrUMR6oNA/ccQF4DDSWLldFCzv7b8nuJ4+tO+L1JQPgZk69h+FBtmt2PT4UYoMODi/Tro2KVtzAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.744872Z"},"content_sha256":"06128c16ae7d208ae379a9165382a0302ba71444b5dead40abb94801d5db2692","schema_version":"1.0","event_id":"sha256:06128c16ae7d208ae379a9165382a0302ba71444b5dead40abb94801d5db2692"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.dark.2025.102068.arXiv:2507.07798) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"T.N. Li, P.J. Wu, G.H. Du, Y.H. Yao, J.F. Zhang, X. Zhang, Exploring non-cold dark mat- ter in the scenario of dynamical dark energy with DESI DR2 data. Phys. Dark Univ.50, 102068 (2025). https://doi.org/10.1016/j.dark.2025. 102068. arXiv:2","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":21,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"T.N. Li, P.J. Wu, G.H. Du, Y.H. Yao, J.F. Zhang, X. Zhang, Exploring non-cold dark mat- ter in the scenario of dynamical dark energy with DESI DR2 data. Phys. Dark Univ.50, 102068 (2025). https://doi.org/10.1016/j.dark.2025. 102068. arXiv:2","reconstructed_doi":"10.1016/j.dark.2025.102068.arXiv:2507.07798"},"severity":"advisory","ref_index":21,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.dark.2025.102068.arXiv:2507.07798","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"052259e15862e12cefa40948225c4e1d4b736af3d0a67e53414e14947c1ec0de","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12886,"payload_sha256":"d127af36814587a9e1e64ac7eb75fa49c52498d2cad81b2df5f1704a263ee9aa","signature_b64":"E1bKRkUY2EB2/dTyCAJdFgtvjdd8qP8BWkzIPfYFKgvjapg7GakgREJtnHGsu+CrYj/4luK2VBqfaKOOeBi7DQ==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ihANWyaLUcKxd05ZMFMrlh5rF4RyFKmqt4ZVXoG70/4ihX1+BX2Kznq/Q7JoGpgOUFlZWlwc7RDR4w9ViapxDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.745174Z"},"content_sha256":"1c929e8fd5afe9ef61d293642fee555cff2e507ad0d4883165cbc48e5df56869","schema_version":"1.0","event_id":"sha256:1c929e8fd5afe9ef61d293642fee555cff2e507ad0d4883165cbc48e5df56869"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1140/epjc/s10052-025-15088-8.arXiv:2508.17848) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"Y. Yang, Constraining deviations fromΛCDM in the Hubble expansion rate. Eur. Phys. J. C85(11), 1350 (2025). https://doi.org/10.1140/epjc/ s10052-025-15088-8. arXiv:2508.17848 [astro- ph.CO]","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":20,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"Y. Yang, Constraining deviations fromΛCDM in the Hubble expansion rate. Eur. Phys. J. C85(11), 1350 (2025). https://doi.org/10.1140/epjc/ s10052-025-15088-8. arXiv:2508.17848 [astro- ph.CO]","reconstructed_doi":"10.1140/epjc/s10052-025-15088-8.arXiv:2508.17848"},"severity":"advisory","ref_index":20,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1140/epjc/s10052-025-15088-8.arXiv:2508.17848","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"25c7f386eb32435d5bd39903a918ba9c20e2001d0df4fd743b93393485109081","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12885,"payload_sha256":"909a020ccbe45bd88a1136422c89b9202e6fb67fd2e2e205c9b54dd1f30a8337","signature_b64":"mEZ2xDYlw6nJHLZNqbU05/IxROkOfTEHD3w56lK2i0B6xlzkhEgaXFwuGJ2c1YnDdtaTtmBNpzjq0NdKpZ+YAg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mX6yYabu4eTqpCDxtbDSul0ha2cUEoe6xM/TdXtD/XskEzRNMCeH1MuYM6vYTskPNAw644XS/1yqlapZR2i/Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.745462Z"},"content_sha256":"1d9153e6b4ae67098af439fd058a841a9e4d25bd38811ebd0d90206299552191","schema_version":"1.0","event_id":"sha256:1d9153e6b4ae67098af439fd058a841a9e4d25bd38811ebd0d90206299552191"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1016/j.dark.2026.102254.arXiv:2511.22512) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"T.N. Li, G.H. Du, S.H. Zhou, Y.H. Li, J.F. Zhang, X. Zhang, Robust evidence for dynamical dark en- ergy in light of DESI DR2 and joint ACT, SPT, and Planck data. Phys. Dark Univ.52, 102254 (2026). https://doi.org/10.1016/j.dark.2026. 102254","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":13,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"T.N. Li, G.H. Du, S.H. Zhou, Y.H. Li, J.F. Zhang, X. Zhang, Robust evidence for dynamical dark en- ergy in light of DESI DR2 and joint ACT, SPT, and Planck data. Phys. Dark Univ.52, 102254 (2026). https://doi.org/10.1016/j.dark.2026. 102254","reconstructed_doi":"10.1016/j.dark.2026.102254.arXiv:2511.22512"},"severity":"advisory","ref_index":13,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1016/j.dark.2026.102254.arXiv:2511.22512","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"868b9b78ff1773a296b619403c7fcded4f996ff577752d7f3f4216ae41abb796","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12884,"payload_sha256":"70fabd66697a099b25f52b3abb37f9251615c1d00b37505d4d8e5c3aabcfef4f","signature_b64":"Gm+n28/lnNz7bPYFxSj+AGOKmvsxpU+SDq7ElTbBeUymmNbI5FqQfR5rLOFLPQrofDqDFSYYuDzb/Nq+ifNHDw==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"65q4TrRc0WQqAreImOrDdxdF2tbScy9Lmr779bW9DqXeLdpcsSgUg23TGDGtUtisH/jxN7trQ0+ZYxenssNrBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.745746Z"},"content_sha256":"ba44dbfad9c92c9c04382ba134994640146e1417c779c8be682e216611dd2817","schema_version":"1.0","event_id":"sha256:ba44dbfad9c92c9c04382ba134994640146e1417c779c8be682e216611dd2817"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","target":"integrity","payload":{"note":"DOI in the printed bibliography is fragmented by whitespace or line breaks. A longer candidate (10.1093/mnras/stx721.arXiv:1607.03155) was visible in the surrounding text but could not be confirmed against doi.org as printed.","snippet":"S. Alam, et al., The clustering of galaxies in the com- pleted SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. Mon. Not. Roy. Astron. Soc.470(3), 2617– 2652 (2017). https://doi.org/10.1093/","arxiv_id":"2607.09240","detector":"doi_compliance","evidence":{"ref_index":6,"verdict_class":"incontrovertible","resolved_title":null,"printed_excerpt":"S. Alam, et al., The clustering of galaxies in the com- pleted SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample. Mon. Not. Roy. Astron. Soc.470(3), 2617– 2652 (2017). https://doi.org/10.1093/","reconstructed_doi":"10.1093/mnras/stx721.arXiv:1607.03155"},"severity":"advisory","ref_index":6,"audited_at":"2026-07-13T04:38:38.553443Z","event_type":"pith.integrity.v1","detected_doi":"10.1093/mnras/stx721.arXiv:1607.03155","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"recoverable_identifier","evidence_hash":"5534b5d7bd259f0924b1ebc991853bf55c4076d9bf4e6741110e8ae3994304ee","paper_version":1,"verdict_class":"incontrovertible","resolved_title":null,"detector_version":"1.0.0","detected_arxiv_id":null,"integrity_event_id":12883,"payload_sha256":"efbad64d33dad620e64b5712da4030136c64e585cb7868924f4b189e20df15bd","signature_b64":"YoFJan+S8nK8mnfz9om1UF5Mg+uBJWmfsMKIqtdEG2vygC63NYPjL+NQCo1RKDXyop7ngRVNYv5pMNwqR325Cg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-13T04:38:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Lcc37tjoRrw8qw9fNE5n4fYOjrh67sasLlSPWQZYN8OSLmBfkv7XerHWDcQoRp7d6rDaF1xZDG1ywZJkRddTDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T05:43:44.746026Z"},"content_sha256":"9268c60fd26a5b4f84ba81ce547ba537881649e26ec9eb6afa77617449b8fe55","schema_version":"1.0","event_id":"sha256:9268c60fd26a5b4f84ba81ce547ba537881649e26ec9eb6afa77617449b8fe55"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/bundle.json","state_url":"https://pith.science/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-04T05:43:44Z","links":{"resolver":"https://pith.science/pith/MVXLCIYZ5RJOSET65B6XOXN7OC","bundle":"https://pith.science/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/bundle.json","state":"https://pith.science/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/MVXLCIYZ5RJOSET65B6XOXN7OC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:MVXLCIYZ5RJOSET65B6XOXN7OC","merge_version":"pith-open-graph-merge-v1","event_count":16,"valid_event_count":16,"invalid_event_count":0,"equivocation_count":1,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"106b737fbf5932c2b9225063e656bd0817fc40894586966d5f4e2e2ee7c5948d","cross_cats_sorted":["gr-qc"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-10T09:36:20Z","title_canon_sha256":"61e95cf695d210969ea632371ece02453cc2a07acf23244d36193020e9b9368b"},"schema_version":"1.0","source":{"id":"2607.09240","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2607.09240","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"arxiv_version","alias_value":"2607.09240v1","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.09240","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_12","alias_value":"MVXLCIYZ5RJO","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_16","alias_value":"MVXLCIYZ5RJOSET6","created_at":"2026-07-13T01:18:54Z"},{"alias_kind":"pith_short_8","alias_value":"MVXLCIYZ","created_at":"2026-07-13T01:18:54Z"}],"graph_snapshots":[{"event_id":"sha256:32839f1b0daf48f4c43701c2142833eee46a70575b153249ed7483104c898151","target":"graph","created_at":"2026-07-13T01:18:54Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2607.09240/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We present updated constraints on both flat and non-flat Dvali-Gabadadze-Porrati (DGP) cosmological models using the latest baryon acoustic oscillation (BAO) measurements from the Dark Energy Spectroscopic Instrument Data Release 2 (DESI DR2), in combination with cosmic chronometer (CC), Type Ia supernova (SNIa), and cosmic microwave background (CMB) distance priors. For the non-flat DGP model, we obtain $H_0 = 64.05 \\pm 0.27\\, \\rm{kms^{-1}Mpc^{-1}}$, $\\Omega_m = 0.3264 \\pm 0.0043$, and $\\Omega_k = 0.0088 \\pm 0.0016$, corresponding to a transition redshift $z_t \\sim 0.41$. For the flat case, t","authors_text":"Xinyi Dai, Yicheng Wang, Yupeng Yang","cross_cats":["gr-qc"],"headline":"","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-10T09:36:20Z","title":"Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.09240","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:d84a2cc4658662661da7ea5b88ed64da597a0e64cbc18b145cc39dd8f1263deb","target":"record","created_at":"2026-07-13T01:18:54Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"106b737fbf5932c2b9225063e656bd0817fc40894586966d5f4e2e2ee7c5948d","cross_cats_sorted":["gr-qc"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-07-10T09:36:20Z","title_canon_sha256":"61e95cf695d210969ea632371ece02453cc2a07acf23244d36193020e9b9368b"},"schema_version":"1.0","source":{"id":"2607.09240","kind":"arxiv","version":1}},"canonical_sha256":"656eb12319ec52e9127ee87d775dbf709a3d205fd96410399c32b3c2887d2be9","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"656eb12319ec52e9127ee87d775dbf709a3d205fd96410399c32b3c2887d2be9","first_computed_at":"2026-07-13T01:18:54.876526Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-13T01:18:54.876526Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"H6cd5JgjO1fFrpfvI3s0P+ka3uS97om2uzNxX+uDip+PdVRqpXYdpgm8SqdH1zYd6G5dPN2pPhzbuAqr6l1aAQ==","signature_status":"signed_v1","signed_at":"2026-07-13T01:18:54.877945Z","signed_message":"canonical_sha256_bytes"},"source_id":"2607.09240","source_kind":"arxiv","source_version":1}}},"equivocations":[{"signer_id":"pith.science","event_type":"integrity_finding","target":"integrity","event_ids":["sha256:06128c16ae7d208ae379a9165382a0302ba71444b5dead40abb94801d5db2692","sha256:19bfdc1685261503e8891ce3f20a39f52f53b08b8fe656e6f763f478a65db53b","sha256:1c929e8fd5afe9ef61d293642fee555cff2e507ad0d4883165cbc48e5df56869","sha256:1d9153e6b4ae67098af439fd058a841a9e4d25bd38811ebd0d90206299552191","sha256:3f9bd2bdad006d477a8ff754d1509489e43fc584f39389bbd2a124feafae9ecc","sha256:458b587380a1575392ed1f966674805db5fe10fd4020225ee95eadf22113175f","sha256:59828ffe88f571a36f061f0c710caf02fe1305b93e13af5f2428f8fd73dd5f4c","sha256:8063c63a398665ef69f63d659ae23a170550cd67e6ae91a47a989ac52b34a0b3","sha256:9268c60fd26a5b4f84ba81ce547ba537881649e26ec9eb6afa77617449b8fe55","sha256:a0b6a7fb2c06d5b7da809c59d5dd649a3bb61ab938a79caaa9740d879cba4c81","sha256:a8e49b1f7b006213c353706bc539320ca33d1eca1db78868a4b0173ff6842f2a","sha256:ba44dbfad9c92c9c04382ba134994640146e1417c779c8be682e216611dd2817","sha256:f96c82f6e523b19e6e3bc95f8ccf2f60ba83e4ec0ba3ad76b002c1121a1287e5","sha256:f9cef09e749c3179b94c267dd40c37d65864ced3dbc653f5848e4ca955538c03"]}],"invalid_events":[],"applied_event_ids":["sha256:d84a2cc4658662661da7ea5b88ed64da597a0e64cbc18b145cc39dd8f1263deb","sha256:32839f1b0daf48f4c43701c2142833eee46a70575b153249ed7483104c898151"],"state_sha256":"0153583ff8793afe11bc0d5f5abb6ebf78aae722b0dcd104cbfdb0b5174b7f4c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"RebUHtDn9oBg7d+HJQ0EwiJ9yrWsg6W9T3V1q7eCrvavajKGdcy1QGVf5jotEmfrCD7C4x2NnZX0UFA29UZvBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-04T05:43:44.751048Z","bundle_sha256":"f82aa7a060b2cbb150a7fac23eb74e8b4cbb5437b48fcf506618c92bcdb45ebf"}}