{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:IXAHQNR2LFWKXB3X57FHZHDTZW","short_pith_number":"pith:IXAHQNR2","schema_version":"1.0","canonical_sha256":"45c078363a596cab8777efca7c9c73cd9682ee583a775ef7eb188342b401c925","source":{"kind":"arxiv","id":"2310.15979","version":1},"attestation_state":"computed","paper":{"title":"The Radiant Massive Magnetic Dipole","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Jos\\'e Ayala, Jos\\'e Diaz Polanco, Maximiliano Ujevic","submitted_at":"2023-10-24T16:28:49Z","abstract_excerpt":"We present an exact, time-dependent solution for the Einstein field equations that models the coupling between an anisotropic fluid and a magnetic field in an axially symmetric space-time. By carefully selecting the metric components, we achieve a convenient separation of variables that enables us to solve Einstein's field equations and obtain a solution that evolves into the Gutsunaev-Manko massive magnetic dipole. The analysis of the thermodynamic quantities suggests that this solution may represent a pulse of radiation emitted by a massive object with magnetic properties as for example puls"},"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":"2310.15979","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-10-24T16:28:49Z","cross_cats_sorted":["math-ph","math.MP"],"title_canon_sha256":"355038d50cae9fd02f656ee52d60edb1959b3e5114536cd4a9d04870fe489fea","abstract_canon_sha256":"925b47e213043498a0cbe7403765bca15d73dd9d9fbb3b7fdaa4521ad731297b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:04:33.278418Z","signature_b64":"WUrWivN+atSqaaLx9lHpOG13p4nPfMM3mcZo1XIrehyZtAa5RrME1LI5O4bd9PbczUks4aejHEPJsXu+NCyjDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"45c078363a596cab8777efca7c9c73cd9682ee583a775ef7eb188342b401c925","last_reissued_at":"2026-07-05T07:04:33.278050Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:04:33.278050Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Radiant Massive Magnetic Dipole","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["math-ph","math.MP"],"primary_cat":"gr-qc","authors_text":"Jos\\'e Ayala, Jos\\'e Diaz Polanco, Maximiliano Ujevic","submitted_at":"2023-10-24T16:28:49Z","abstract_excerpt":"We present an exact, time-dependent solution for the Einstein field equations that models the coupling between an anisotropic fluid and a magnetic field in an axially symmetric space-time. By carefully selecting the metric components, we achieve a convenient separation of variables that enables us to solve Einstein's field equations and obtain a solution that evolves into the Gutsunaev-Manko massive magnetic dipole. The analysis of the thermodynamic quantities suggests that this solution may represent a pulse of radiation emitted by a massive object with magnetic properties as for example puls"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.15979","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2310.15979/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":"2310.15979","created_at":"2026-07-05T07:04:33.278104+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.15979v1","created_at":"2026-07-05T07:04:33.278104+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.15979","created_at":"2026-07-05T07:04:33.278104+00:00"},{"alias_kind":"pith_short_12","alias_value":"IXAHQNR2LFWK","created_at":"2026-07-05T07:04:33.278104+00:00"},{"alias_kind":"pith_short_16","alias_value":"IXAHQNR2LFWKXB3X","created_at":"2026-07-05T07:04:33.278104+00:00"},{"alias_kind":"pith_short_8","alias_value":"IXAHQNR2","created_at":"2026-07-05T07:04:33.278104+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.11117","citing_title":"Stability of the spacetime of a magnetized compact object","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW","json":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW.json","graph_json":"https://pith.science/api/pith-number/IXAHQNR2LFWKXB3X57FHZHDTZW/graph.json","events_json":"https://pith.science/api/pith-number/IXAHQNR2LFWKXB3X57FHZHDTZW/events.json","paper":"https://pith.science/paper/IXAHQNR2"},"agent_actions":{"view_html":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW","download_json":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW.json","view_paper":"https://pith.science/paper/IXAHQNR2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.15979&json=true","fetch_graph":"https://pith.science/api/pith-number/IXAHQNR2LFWKXB3X57FHZHDTZW/graph.json","fetch_events":"https://pith.science/api/pith-number/IXAHQNR2LFWKXB3X57FHZHDTZW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW/action/storage_attestation","attest_author":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW/action/author_attestation","sign_citation":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW/action/citation_signature","submit_replication":"https://pith.science/pith/IXAHQNR2LFWKXB3X57FHZHDTZW/action/replication_record"}},"created_at":"2026-07-05T07:04:33.278104+00:00","updated_at":"2026-07-05T07:04:33.278104+00:00"}