{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GDUL6KCWHJSTXOZA3VBSBP3KJL","short_pith_number":"pith:GDUL6KCW","schema_version":"1.0","canonical_sha256":"30e8bf28563a653bbb20dd4320bf6a4aee8f68e0d16451c36f99f320794427ba","source":{"kind":"arxiv","id":"2410.17501","version":2},"attestation_state":"computed","paper":{"title":"Scalar quasinormal modes in emergent modified gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Erick I. Duque, Martin Bojowald, S. Shankaranarayanan","submitted_at":"2024-10-23T01:53:08Z","abstract_excerpt":"Emergent modified gravity is a post-Einsteinian gravitational theory where spacetime geometry is not fundamental but rather emerges from the gravitational degrees of freedom in a non-trivial way. The specific relationship between geometry and these degrees of freedom is unique for each theory, but it is not predetermined. Instead, it is derived from constraints and equations of motion, relying on key aspects of the canonical formulation of gravity, such as structure functions in Poisson brackets of constraints and covariance conditions. As shown in previous work, these new theories allow for t"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2410.17501","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-10-23T01:53:08Z","cross_cats_sorted":[],"title_canon_sha256":"bc40ec1b453b4576ffa9568a503b007423aad4064a2ccbf4997c5764319a15bb","abstract_canon_sha256":"27a28aa1f3f88596601d0092cf99d42e720130863e0667c8b7f49521daf78a4e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:52:17.315400Z","signature_b64":"c7zN7uCFQ8a/usvwv6hv30KRjAEg1OXcBSuifeaNcQL1obPs+Hy/PinHsW/LvVI3dDnZuvp7tFE8RIFWNCItCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"30e8bf28563a653bbb20dd4320bf6a4aee8f68e0d16451c36f99f320794427ba","last_reissued_at":"2026-07-05T09:52:17.314913Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:52:17.314913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalar quasinormal modes in emergent modified gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Erick I. Duque, Martin Bojowald, S. Shankaranarayanan","submitted_at":"2024-10-23T01:53:08Z","abstract_excerpt":"Emergent modified gravity is a post-Einsteinian gravitational theory where spacetime geometry is not fundamental but rather emerges from the gravitational degrees of freedom in a non-trivial way. The specific relationship between geometry and these degrees of freedom is unique for each theory, but it is not predetermined. Instead, it is derived from constraints and equations of motion, relying on key aspects of the canonical formulation of gravity, such as structure functions in Poisson brackets of constraints and covariance conditions. As shown in previous work, these new theories allow for t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.17501","kind":"arxiv","version":2},"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/2410.17501/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2410.17501","created_at":"2026-07-05T09:52:17.314971+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.17501v2","created_at":"2026-07-05T09:52:17.314971+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.17501","created_at":"2026-07-05T09:52:17.314971+00:00"},{"alias_kind":"pith_short_12","alias_value":"GDUL6KCWHJST","created_at":"2026-07-05T09:52:17.314971+00:00"},{"alias_kind":"pith_short_16","alias_value":"GDUL6KCWHJSTXOZA","created_at":"2026-07-05T09:52:17.314971+00:00"},{"alias_kind":"pith_short_8","alias_value":"GDUL6KCW","created_at":"2026-07-05T09:52:17.314971+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2511.14047","citing_title":"Exact, non-singular black holes from a phantom DBI Field as primordial dark matter","ref_index":72,"is_internal_anchor":false},{"citing_arxiv_id":"2511.20425","citing_title":"Canonical form of a deformed Poisson bracket spacetime","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL","json":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL.json","graph_json":"https://pith.science/api/pith-number/GDUL6KCWHJSTXOZA3VBSBP3KJL/graph.json","events_json":"https://pith.science/api/pith-number/GDUL6KCWHJSTXOZA3VBSBP3KJL/events.json","paper":"https://pith.science/paper/GDUL6KCW"},"agent_actions":{"view_html":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL","download_json":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL.json","view_paper":"https://pith.science/paper/GDUL6KCW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.17501&json=true","fetch_graph":"https://pith.science/api/pith-number/GDUL6KCWHJSTXOZA3VBSBP3KJL/graph.json","fetch_events":"https://pith.science/api/pith-number/GDUL6KCWHJSTXOZA3VBSBP3KJL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL/action/storage_attestation","attest_author":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL/action/author_attestation","sign_citation":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL/action/citation_signature","submit_replication":"https://pith.science/pith/GDUL6KCWHJSTXOZA3VBSBP3KJL/action/replication_record"}},"created_at":"2026-07-05T09:52:17.314971+00:00","updated_at":"2026-07-05T09:52:17.314971+00:00"}