{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FPA5TZM4GIQRBJK6UJ76AHHKSG","short_pith_number":"pith:FPA5TZM4","schema_version":"1.0","canonical_sha256":"2bc1d9e59c322110a55ea27fe01cea91b398b6322a20c01cafb818164047ec50","source":{"kind":"arxiv","id":"2407.00283","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waveforms from periodic orbits around a quantum-corrected black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Li Zhao, Sen Yang, Tao Zhu, Yu-Peng Zhang, Yu-Xiao Liu","submitted_at":"2024-06-29T02:25:32Z","abstract_excerpt":"Extreme mass-ratio inspirals are crucial sources for future space-based gravitational wave detections. Gravitational waveforms emitted by extreme mass-ratio inspirals are closely related to the orbital dynamics of small celestial objects, which vary with the underlying spacetime geometry. Despite the tremendous success of general relativity, there are unsolved issues such as singularities in both black holes and cosmology. Loop quantum gravity, a theory addressing these singularity problems, offers a framework for regular black holes. In this paper, we focus on periodic orbits of a small celes"},"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":"2407.00283","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-06-29T02:25:32Z","cross_cats_sorted":[],"title_canon_sha256":"9c963bda2f18d45bb708fbe87a4cf3364db772bf08024c67d1fa3ddb9499acb9","abstract_canon_sha256":"25f199ef9f7ef5eca9a012d4ab7218d1df119a387a0ace949f381edb3f3fbc7c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:45:09.657464Z","signature_b64":"/WQgvoKMGC2veXTa92wDLems5e0QAw5vj/U8Biv1l3rbViidhyOqVSTZbTBPh+fBeDthGlc/DPoM2lOqahjaCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2bc1d9e59c322110a55ea27fe01cea91b398b6322a20c01cafb818164047ec50","last_reissued_at":"2026-07-05T10:45:09.656898Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:45:09.656898Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waveforms from periodic orbits around a quantum-corrected black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Li Zhao, Sen Yang, Tao Zhu, Yu-Peng Zhang, Yu-Xiao Liu","submitted_at":"2024-06-29T02:25:32Z","abstract_excerpt":"Extreme mass-ratio inspirals are crucial sources for future space-based gravitational wave detections. Gravitational waveforms emitted by extreme mass-ratio inspirals are closely related to the orbital dynamics of small celestial objects, which vary with the underlying spacetime geometry. Despite the tremendous success of general relativity, there are unsolved issues such as singularities in both black holes and cosmology. Loop quantum gravity, a theory addressing these singularity problems, offers a framework for regular black holes. In this paper, we focus on periodic orbits of a small celes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.00283","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/2407.00283/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":"2407.00283","created_at":"2026-07-05T10:45:09.656964+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.00283v2","created_at":"2026-07-05T10:45:09.656964+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.00283","created_at":"2026-07-05T10:45:09.656964+00:00"},{"alias_kind":"pith_short_12","alias_value":"FPA5TZM4GIQR","created_at":"2026-07-05T10:45:09.656964+00:00"},{"alias_kind":"pith_short_16","alias_value":"FPA5TZM4GIQRBJK6","created_at":"2026-07-05T10:45:09.656964+00:00"},{"alias_kind":"pith_short_8","alias_value":"FPA5TZM4","created_at":"2026-07-05T10:45:09.656964+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23021","citing_title":"Periodic Timelike Motion and Gravitational Wave Signatures around a Magnetically Charged Black Hole Surrounded by Quintessence","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2606.21029","citing_title":"Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2606.11728","citing_title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2607.02017","citing_title":"Boson Stars in Teleparallel Gravity with a Nonminimally Coupled Field: The Violation of Energy Conditions and Gravitational Waveforms from EMRIs","ref_index":81,"is_internal_anchor":false},{"citing_arxiv_id":"2607.00812","citing_title":"Gravitational Wave Signatures of Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\\gamma)$ Dark Matter Halo","ref_index":99,"is_internal_anchor":false},{"citing_arxiv_id":"2509.23318","citing_title":"Gravitational waveforms from periodic orbits around a novel regular black hole","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2510.27320","citing_title":"The quasinormal modes of the rotating quantum corrected black holes","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2601.00550","citing_title":"Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2603.18963","citing_title":"Observational Signatures of Rotating Ay\\'{o}n-Beato-Garc\\'{i}a Black Holes: Shadows, Accretion Disks and Images","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11866","citing_title":"Equatorial periodic orbits and gravitational wave signatures in Euler-Heisenberg black holes surrounded by perfect fluid dark matter","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2605.07187","citing_title":"Probing Gravitational Wave Signatures from Periodic Orbits of Regular Black Holes in Asymptotically Safe Gravity","ref_index":50,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG","json":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG.json","graph_json":"https://pith.science/api/pith-number/FPA5TZM4GIQRBJK6UJ76AHHKSG/graph.json","events_json":"https://pith.science/api/pith-number/FPA5TZM4GIQRBJK6UJ76AHHKSG/events.json","paper":"https://pith.science/paper/FPA5TZM4"},"agent_actions":{"view_html":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG","download_json":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG.json","view_paper":"https://pith.science/paper/FPA5TZM4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.00283&json=true","fetch_graph":"https://pith.science/api/pith-number/FPA5TZM4GIQRBJK6UJ76AHHKSG/graph.json","fetch_events":"https://pith.science/api/pith-number/FPA5TZM4GIQRBJK6UJ76AHHKSG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG/action/storage_attestation","attest_author":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG/action/author_attestation","sign_citation":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG/action/citation_signature","submit_replication":"https://pith.science/pith/FPA5TZM4GIQRBJK6UJ76AHHKSG/action/replication_record"}},"created_at":"2026-07-05T10:45:09.656964+00:00","updated_at":"2026-07-05T10:45:09.656964+00:00"}