{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:RC7HCWOZE2KG2MNI4JECFSXJEY","short_pith_number":"pith:RC7HCWOZ","schema_version":"1.0","canonical_sha256":"88be7159d926946d31a8e24822cae92619ded726a108f34d94b187cee9a0cacc","source":{"kind":"arxiv","id":"1101.5306","version":1},"attestation_state":"computed","paper":{"title":"Gravitational and electromagnetic emission by magnetized coalescing binary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"astro-ph.HE","authors_text":"D. Vernieri, I. De Martino, M. De Laurentis, M. Formisano, S. Capozziello","submitted_at":"2011-01-27T14:52:33Z","abstract_excerpt":"We discuss the possibility to obtain an electromagnetic emission accompanying the gravitational waves emitted in the coalescence of a compact binary system. Motivated by the existence of black hole configurations with open magnetic field lines along the rotation axis, we consider a magnetic dipole in the system, the evolution of which leads to (i) electromagnetic radiation, and (ii) a contribution to the gravitational radiation, the luminosity of both being evaluated. Starting from the observations on magnetars, we impose upper limits for both the electromagnetic emission and the contribution "},"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":"1101.5306","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-27T14:52:33Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-th"],"title_canon_sha256":"aa5a53153aee1f092cea85eaddf4ccad627bbc2cb17577737a7a7dc1e78944d9","abstract_canon_sha256":"e50f8d224cc348bd2287324d8bad53b11121b7f99d1ba0a34d862ba8a8af6b68"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:21.343882Z","signature_b64":"nxjmwzPIZNF6aEl7mzygiOlbuTyTgZZXvdbAYcOsNsOjBMmAd3JCS38WunYc3aKbHr6yzBE0q6y7eT5llyYZDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88be7159d926946d31a8e24822cae92619ded726a108f34d94b187cee9a0cacc","last_reissued_at":"2026-05-18T02:03:21.343356Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:21.343356Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational and electromagnetic emission by magnetized coalescing binary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th"],"primary_cat":"astro-ph.HE","authors_text":"D. Vernieri, I. De Martino, M. De Laurentis, M. Formisano, S. Capozziello","submitted_at":"2011-01-27T14:52:33Z","abstract_excerpt":"We discuss the possibility to obtain an electromagnetic emission accompanying the gravitational waves emitted in the coalescence of a compact binary system. Motivated by the existence of black hole configurations with open magnetic field lines along the rotation axis, we consider a magnetic dipole in the system, the evolution of which leads to (i) electromagnetic radiation, and (ii) a contribution to the gravitational radiation, the luminosity of both being evaluated. Starting from the observations on magnetars, we impose upper limits for both the electromagnetic emission and the contribution "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5306","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1101.5306","created_at":"2026-05-18T02:03:21.343438+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.5306v1","created_at":"2026-05-18T02:03:21.343438+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5306","created_at":"2026-05-18T02:03:21.343438+00:00"},{"alias_kind":"pith_short_12","alias_value":"RC7HCWOZE2KG","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"RC7HCWOZE2KG2MNI","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"RC7HCWOZ","created_at":"2026-05-18T12:26:41.206345+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY","json":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY.json","graph_json":"https://pith.science/api/pith-number/RC7HCWOZE2KG2MNI4JECFSXJEY/graph.json","events_json":"https://pith.science/api/pith-number/RC7HCWOZE2KG2MNI4JECFSXJEY/events.json","paper":"https://pith.science/paper/RC7HCWOZ"},"agent_actions":{"view_html":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY","download_json":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY.json","view_paper":"https://pith.science/paper/RC7HCWOZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.5306&json=true","fetch_graph":"https://pith.science/api/pith-number/RC7HCWOZE2KG2MNI4JECFSXJEY/graph.json","fetch_events":"https://pith.science/api/pith-number/RC7HCWOZE2KG2MNI4JECFSXJEY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY/action/storage_attestation","attest_author":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY/action/author_attestation","sign_citation":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY/action/citation_signature","submit_replication":"https://pith.science/pith/RC7HCWOZE2KG2MNI4JECFSXJEY/action/replication_record"}},"created_at":"2026-05-18T02:03:21.343438+00:00","updated_at":"2026-05-18T02:03:21.343438+00:00"}