{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:XGI7A5MIPOQRJBYOL7U4AVXKZV","short_pith_number":"pith:XGI7A5MI","schema_version":"1.0","canonical_sha256":"b991f075887ba114870e5fe9c056eacd6e79f70380e33c34273f14fa489f1ca5","source":{"kind":"arxiv","id":"1310.4893","version":2},"attestation_state":"computed","paper":{"title":"A possible connection between Fast Radio Bursts and Gamma-Ray Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bing Zhang (UNLV)","submitted_at":"2013-10-18T03:06:35Z","abstract_excerpt":"The physical nature of Fast Radio Bursts (FRBs), a new type of cosmological transients discovered recently, is not known. It has been suggested that FRBs can be produced when a spinning supra-massive neutron star loses centrifugal support and collapses to a black hole. Here we suggest that such implosions can happen in supra-massive neutron stars shortly (hundreds to thousands of seconds) after their births, and an observational signature of such implosions may have been observed in the X-ray afterglows of some long and short gamma-ray bursts (GRBs). Within this picture, a small fraction of FR"},"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":"1310.4893","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-18T03:06:35Z","cross_cats_sorted":[],"title_canon_sha256":"2e6945ea37b279de399024c98fe447a59b544546deb4bd85225e3ddb37f99adf","abstract_canon_sha256":"b0fc04f6cba0a0818aeda8825d1edf0edf5815232c9d8ba5169b091ff74adf4e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:58.148287Z","signature_b64":"bfkmvrATbuj1OFyH+RR9fHU9a1YO8bL1sSayKdi4nXY+Fc3Vr/rCDZ2ZHbDUZb2xXZno5NLME2DprkQjCCQnBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b991f075887ba114870e5fe9c056eacd6e79f70380e33c34273f14fa489f1ca5","last_reissued_at":"2026-05-18T01:46:58.147676Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:58.147676Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A possible connection between Fast Radio Bursts and Gamma-Ray Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bing Zhang (UNLV)","submitted_at":"2013-10-18T03:06:35Z","abstract_excerpt":"The physical nature of Fast Radio Bursts (FRBs), a new type of cosmological transients discovered recently, is not known. It has been suggested that FRBs can be produced when a spinning supra-massive neutron star loses centrifugal support and collapses to a black hole. Here we suggest that such implosions can happen in supra-massive neutron stars shortly (hundreds to thousands of seconds) after their births, and an observational signature of such implosions may have been observed in the X-ray afterglows of some long and short gamma-ray bursts (GRBs). Within this picture, a small fraction of FR"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4893","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":""},"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":"1310.4893","created_at":"2026-05-18T01:46:58.147762+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.4893v2","created_at":"2026-05-18T01:46:58.147762+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4893","created_at":"2026-05-18T01:46:58.147762+00:00"},{"alias_kind":"pith_short_12","alias_value":"XGI7A5MIPOQR","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"XGI7A5MIPOQRJBYO","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"XGI7A5MI","created_at":"2026-05-18T12:28:06.772260+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.07567","citing_title":"The Transient program of the Cherenkov Telescope Array","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2604.12775","citing_title":"Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A","ref_index":9,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV","json":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV.json","graph_json":"https://pith.science/api/pith-number/XGI7A5MIPOQRJBYOL7U4AVXKZV/graph.json","events_json":"https://pith.science/api/pith-number/XGI7A5MIPOQRJBYOL7U4AVXKZV/events.json","paper":"https://pith.science/paper/XGI7A5MI"},"agent_actions":{"view_html":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV","download_json":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV.json","view_paper":"https://pith.science/paper/XGI7A5MI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.4893&json=true","fetch_graph":"https://pith.science/api/pith-number/XGI7A5MIPOQRJBYOL7U4AVXKZV/graph.json","fetch_events":"https://pith.science/api/pith-number/XGI7A5MIPOQRJBYOL7U4AVXKZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV/action/storage_attestation","attest_author":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV/action/author_attestation","sign_citation":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV/action/citation_signature","submit_replication":"https://pith.science/pith/XGI7A5MIPOQRJBYOL7U4AVXKZV/action/replication_record"}},"created_at":"2026-05-18T01:46:58.147762+00:00","updated_at":"2026-05-18T01:46:58.147762+00:00"}