{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RC5SYBJWEGE6BEJGIZLDXEOWAB","short_pith_number":"pith:RC5SYBJW","schema_version":"1.0","canonical_sha256":"88bb2c05362189e0912646563b91d6007d5ba243d612676218ffeb55d7235889","source":{"kind":"arxiv","id":"2401.08085","version":2},"attestation_state":"computed","paper":{"title":"Testing gravity with Extreme-Mass-Ratio Inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Alejandro C\\'ardenas-Avenda\\~no, Carlos F. Sopuerta","submitted_at":"2024-01-16T03:25:01Z","abstract_excerpt":"Extreme-mass-ratio inspirals consist of binary systems of compact objects, with orders of magnitude differences in their masses, in the regime where the dynamics are driven by gravitational wave emission. The unique nature of extreme-mass-ratio inspirals facilitates the exploration of diverse and stimulating tests related to various aspects of black holes and General Relativity. These tests encompass investigations into the spacetime geometry, the dissipation of the binary system energy and angular momentum, and the impact of the intrinsic non-linear effects of the gravitational interaction. 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":"2401.08085","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-01-16T03:25:01Z","cross_cats_sorted":["astro-ph.HE","hep-ph","hep-th"],"title_canon_sha256":"16cc8c57a0fe7f96769c97e9d9e0b43505a3bae40d2674d55d0dd04c6f143553","abstract_canon_sha256":"688acd03705c0b13437c53e84c2a83b0ac3eb344c597a482b8b09e8971b86e61"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:42:32.230792Z","signature_b64":"aE8GGjH4Mwy+EoDKpQeEimlrGJEvFAZKFAHJDE1TbnNhR9OtHM+txa5/HVLbkfcKnjg6aCSC5SGZWFMMG4HLCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88bb2c05362189e0912646563b91d6007d5ba243d612676218ffeb55d7235889","last_reissued_at":"2026-07-05T08:42:32.230341Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:42:32.230341Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing gravity with Extreme-Mass-Ratio Inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Alejandro C\\'ardenas-Avenda\\~no, Carlos F. Sopuerta","submitted_at":"2024-01-16T03:25:01Z","abstract_excerpt":"Extreme-mass-ratio inspirals consist of binary systems of compact objects, with orders of magnitude differences in their masses, in the regime where the dynamics are driven by gravitational wave emission. The unique nature of extreme-mass-ratio inspirals facilitates the exploration of diverse and stimulating tests related to various aspects of black holes and General Relativity. These tests encompass investigations into the spacetime geometry, the dissipation of the binary system energy and angular momentum, and the impact of the intrinsic non-linear effects of the gravitational interaction. T"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.08085","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/2401.08085/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":"2401.08085","created_at":"2026-07-05T08:42:32.230397+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.08085v2","created_at":"2026-07-05T08:42:32.230397+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.08085","created_at":"2026-07-05T08:42:32.230397+00:00"},{"alias_kind":"pith_short_12","alias_value":"RC5SYBJWEGE6","created_at":"2026-07-05T08:42:32.230397+00:00"},{"alias_kind":"pith_short_16","alias_value":"RC5SYBJWEGE6BEJG","created_at":"2026-07-05T08:42:32.230397+00:00"},{"alias_kind":"pith_short_8","alias_value":"RC5SYBJW","created_at":"2026-07-05T08:42:32.230397+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05909","citing_title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11728","citing_title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","ref_index":95,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27429","citing_title":"Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03756","citing_title":"Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2605.24905","citing_title":"QPEs from Warped Disk Collisions with EMRIs: Brightness-Recurrence Diagram and Gravitational-Wave Follow-up","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2507.04471","citing_title":"A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03756","citing_title":"Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26011","citing_title":"Parameter-estimation bias induced by transient orbital resonances in extreme-mass-ratio inspirals","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2604.10942","citing_title":"Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals","ref_index":6,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB","json":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB.json","graph_json":"https://pith.science/api/pith-number/RC5SYBJWEGE6BEJGIZLDXEOWAB/graph.json","events_json":"https://pith.science/api/pith-number/RC5SYBJWEGE6BEJGIZLDXEOWAB/events.json","paper":"https://pith.science/paper/RC5SYBJW"},"agent_actions":{"view_html":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB","download_json":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB.json","view_paper":"https://pith.science/paper/RC5SYBJW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.08085&json=true","fetch_graph":"https://pith.science/api/pith-number/RC5SYBJWEGE6BEJGIZLDXEOWAB/graph.json","fetch_events":"https://pith.science/api/pith-number/RC5SYBJWEGE6BEJGIZLDXEOWAB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB/action/storage_attestation","attest_author":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB/action/author_attestation","sign_citation":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB/action/citation_signature","submit_replication":"https://pith.science/pith/RC5SYBJWEGE6BEJGIZLDXEOWAB/action/replication_record"}},"created_at":"2026-07-05T08:42:32.230397+00:00","updated_at":"2026-07-05T08:42:32.230397+00:00"}