{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:I3TVDVUQPPK6ZCIQLAOCV6DICP","short_pith_number":"pith:I3TVDVUQ","schema_version":"1.0","canonical_sha256":"46e751d6907bd5ec8910581c2af86813f97af483eb31549830ddf9c63e498bd0","source":{"kind":"arxiv","id":"2011.13586","version":2},"attestation_state":"computed","paper":{"title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Lang Liu, {\\O}yvind Christiansen, Rong-Gen Cai, Sang Pyo Kim, Wen-Hong Ruan, Zong-Kuan Guo","submitted_at":"2020-11-27T07:23:23Z","abstract_excerpt":"Extending the electromagnetic and gravitational radiations from binary black holes with electric and magnetic charges in circular orbits in Phys. Rev. D {\\bf 102}, 103520 (2020), we calculate the total emission rates of energy and angular momentum due to gravitational and electromagnetic radiations from dyonic binary black holes in precessing elliptical orbits. It is shown that the emission rates of energy and angular momentum due to gravitational and electromagnetic radiations have the same dependence on the conic angle for different orbits. Moreover, we obtain the evolutions of orbits and fi"},"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":"2011.13586","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-11-27T07:23:23Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"9718d32d386e3ffd5a57fa345e140a9defe99db68f9d3e850f38c905a09f07ad","abstract_canon_sha256":"bab8ae6e61f5cf922c5603ec5076b08c5d490cb3f344e18a2fe91eadfb522aec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:36:35.481899Z","signature_b64":"QgIJ0R/CozNuSUKa/OhmFIlXmf5oZMfbb3LgUMch2esUJlw+7dgpmto/Nszk8cEl3rXdrJ/HJAgyhJ6iM7s+AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"46e751d6907bd5ec8910581c2af86813f97af483eb31549830ddf9c63e498bd0","last_reissued_at":"2026-07-05T03:36:35.481418Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:36:35.481418Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Lang Liu, {\\O}yvind Christiansen, Rong-Gen Cai, Sang Pyo Kim, Wen-Hong Ruan, Zong-Kuan Guo","submitted_at":"2020-11-27T07:23:23Z","abstract_excerpt":"Extending the electromagnetic and gravitational radiations from binary black holes with electric and magnetic charges in circular orbits in Phys. Rev. D {\\bf 102}, 103520 (2020), we calculate the total emission rates of energy and angular momentum due to gravitational and electromagnetic radiations from dyonic binary black holes in precessing elliptical orbits. It is shown that the emission rates of energy and angular momentum due to gravitational and electromagnetic radiations have the same dependence on the conic angle for different orbits. Moreover, we obtain the evolutions of orbits and fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.13586","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/2011.13586/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":"2011.13586","created_at":"2026-07-05T03:36:35.481477+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.13586v2","created_at":"2026-07-05T03:36:35.481477+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.13586","created_at":"2026-07-05T03:36:35.481477+00:00"},{"alias_kind":"pith_short_12","alias_value":"I3TVDVUQPPK6","created_at":"2026-07-05T03:36:35.481477+00:00"},{"alias_kind":"pith_short_16","alias_value":"I3TVDVUQPPK6ZCIQ","created_at":"2026-07-05T03:36:35.481477+00:00"},{"alias_kind":"pith_short_8","alias_value":"I3TVDVUQ","created_at":"2026-07-05T03:36:35.481477+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05909","citing_title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2305.15473","citing_title":"Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter","ref_index":140,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13036","citing_title":"Inspiral gravitational waveforms from charged compact binaries with scalar hair","ref_index":95,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP","json":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP.json","graph_json":"https://pith.science/api/pith-number/I3TVDVUQPPK6ZCIQLAOCV6DICP/graph.json","events_json":"https://pith.science/api/pith-number/I3TVDVUQPPK6ZCIQLAOCV6DICP/events.json","paper":"https://pith.science/paper/I3TVDVUQ"},"agent_actions":{"view_html":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP","download_json":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP.json","view_paper":"https://pith.science/paper/I3TVDVUQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.13586&json=true","fetch_graph":"https://pith.science/api/pith-number/I3TVDVUQPPK6ZCIQLAOCV6DICP/graph.json","fetch_events":"https://pith.science/api/pith-number/I3TVDVUQPPK6ZCIQLAOCV6DICP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP/action/storage_attestation","attest_author":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP/action/author_attestation","sign_citation":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP/action/citation_signature","submit_replication":"https://pith.science/pith/I3TVDVUQPPK6ZCIQLAOCV6DICP/action/replication_record"}},"created_at":"2026-07-05T03:36:35.481477+00:00","updated_at":"2026-07-05T03:36:35.481477+00:00"}