{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:RAAX2FL4L4B4UDFKUIEQQ77JBE","short_pith_number":"pith:RAAX2FL4","schema_version":"1.0","canonical_sha256":"88017d157c5f03ca0caaa209087fe90914568c0e6602bf56498f7292ad4e31c4","source":{"kind":"arxiv","id":"2301.05915","version":2},"attestation_state":"computed","paper":{"title":"Detecting vector charge with extreme mass ratio inspirals onto Kerr black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bin Wang, Chao Zhang, Hong Guo, Yungui Gong","submitted_at":"2023-01-14T13:23:54Z","abstract_excerpt":"Extreme mass ratio inspirals (EMRIs) are excellent sources for space-based observatories to explore the properties of black holes and test no-hair theorems. We consider EMRIs with a charged compact object inspiralling onto a Kerr black hole in quasi-circular orbits. Using the Teukolsky and generalized Sasaki-Nakamura formalisms for the gravitational and vector perturbations about a Kerr black hole, we numerically calculate the energy fluxes for both gravitational and vector perturbations induced by a charged particle moving in equatorial circular orbits. With one-year observations of EMRIs, we"},"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":"2301.05915","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-01-14T13:23:54Z","cross_cats_sorted":[],"title_canon_sha256":"49708082411a0345c93a4179d1c44fc89b4f51ee94a7fe8ec3a3f8df6e365fa4","abstract_canon_sha256":"06deda8ec53ee0f6f9099030d63962954ebf7d8ce202e92b565453ac594c21e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:25:39.345952Z","signature_b64":"c0A9srZEc13sri4Z1cumnnTSm5L3ewNDmJJjfrcSMBZO33AH+98JIa811VOBQATcdbqXoHQkIVfTIPTZrz4TBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88017d157c5f03ca0caaa209087fe90914568c0e6602bf56498f7292ad4e31c4","last_reissued_at":"2026-07-05T06:25:39.345405Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:25:39.345405Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detecting vector charge with extreme mass ratio inspirals onto Kerr black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bin Wang, Chao Zhang, Hong Guo, Yungui Gong","submitted_at":"2023-01-14T13:23:54Z","abstract_excerpt":"Extreme mass ratio inspirals (EMRIs) are excellent sources for space-based observatories to explore the properties of black holes and test no-hair theorems. We consider EMRIs with a charged compact object inspiralling onto a Kerr black hole in quasi-circular orbits. Using the Teukolsky and generalized Sasaki-Nakamura formalisms for the gravitational and vector perturbations about a Kerr black hole, we numerically calculate the energy fluxes for both gravitational and vector perturbations induced by a charged particle moving in equatorial circular orbits. With one-year observations of EMRIs, we"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.05915","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/2301.05915/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":"2301.05915","created_at":"2026-07-05T06:25:39.345466+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.05915v2","created_at":"2026-07-05T06:25:39.345466+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.05915","created_at":"2026-07-05T06:25:39.345466+00:00"},{"alias_kind":"pith_short_12","alias_value":"RAAX2FL4L4B4","created_at":"2026-07-05T06:25:39.345466+00:00"},{"alias_kind":"pith_short_16","alias_value":"RAAX2FL4L4B4UDFK","created_at":"2026-07-05T06:25:39.345466+00:00"},{"alias_kind":"pith_short_8","alias_value":"RAAX2FL4","created_at":"2026-07-05T06:25:39.345466+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.15131","citing_title":"Probing time-dependent scalar wigs with extreme mass ratio inspirals","ref_index":59,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE","json":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE.json","graph_json":"https://pith.science/api/pith-number/RAAX2FL4L4B4UDFKUIEQQ77JBE/graph.json","events_json":"https://pith.science/api/pith-number/RAAX2FL4L4B4UDFKUIEQQ77JBE/events.json","paper":"https://pith.science/paper/RAAX2FL4"},"agent_actions":{"view_html":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE","download_json":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE.json","view_paper":"https://pith.science/paper/RAAX2FL4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.05915&json=true","fetch_graph":"https://pith.science/api/pith-number/RAAX2FL4L4B4UDFKUIEQQ77JBE/graph.json","fetch_events":"https://pith.science/api/pith-number/RAAX2FL4L4B4UDFKUIEQQ77JBE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE/action/storage_attestation","attest_author":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE/action/author_attestation","sign_citation":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE/action/citation_signature","submit_replication":"https://pith.science/pith/RAAX2FL4L4B4UDFKUIEQQ77JBE/action/replication_record"}},"created_at":"2026-07-05T06:25:39.345466+00:00","updated_at":"2026-07-05T06:25:39.345466+00:00"}