{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7WLQDTLTGONEAVTSGH7IC5JPZS","short_pith_number":"pith:7WLQDTLT","schema_version":"1.0","canonical_sha256":"fd9701cd73339a40567231fe81752fccab1b417e19f6b67eafeb1a4577407774","source":{"kind":"arxiv","id":"1709.02734","version":3},"attestation_state":"computed","paper":{"title":"Could the low braking index pulsar PSR J1734-3333 evolve into a magnetar?","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D.-L. Song, H. Shan, N. Wang, X.-D. Li, Y.-L. Liu, Z.-F. Gao","submitted_at":"2017-09-07T12:33:46Z","abstract_excerpt":"The low braking-index pulsar PSR J1734$-$3333 could be born with superhigh internal magnetic fields $B_{\\rm in}\\sim10^{15}-10^{16}$ G, and undergo a supercritical accretion soon after its formation in a supernova explosion. The buried multipole magnetic fields will merger into a dipole magnetic field. Since the magnetic flow transfers from the core to the crust of the pulsar, its surface dipole field grows quickly at a power-law form assumed until it saturates at the level of internal dipole field. The increase in surface dipole magnetic field results in the observed low braking index of $n=0."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1709.02734","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-09-07T12:33:46Z","cross_cats_sorted":[],"title_canon_sha256":"8537bc6c548549fcb9de5629a72a17661c4692a3ee720d4957396060620ed466","abstract_canon_sha256":"2466700e9daa4c7f59e72b3f77c0873c06140d20b875a3a98ae1ad3d02d84f28"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:28.872939Z","signature_b64":"p6gw7E83u9EYxW5Wx//dt9zeOmxI0pdEjhCTjNC9ktzKanFjoD58udP8ayJXcngnq0eGNIT0o+foYxnG6iKxBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fd9701cd73339a40567231fe81752fccab1b417e19f6b67eafeb1a4577407774","last_reissued_at":"2026-05-18T00:26:28.872110Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:28.872110Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Could the low braking index pulsar PSR J1734-3333 evolve into a magnetar?","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D.-L. Song, H. Shan, N. Wang, X.-D. Li, Y.-L. Liu, Z.-F. Gao","submitted_at":"2017-09-07T12:33:46Z","abstract_excerpt":"The low braking-index pulsar PSR J1734$-$3333 could be born with superhigh internal magnetic fields $B_{\\rm in}\\sim10^{15}-10^{16}$ G, and undergo a supercritical accretion soon after its formation in a supernova explosion. The buried multipole magnetic fields will merger into a dipole magnetic field. Since the magnetic flow transfers from the core to the crust of the pulsar, its surface dipole field grows quickly at a power-law form assumed until it saturates at the level of internal dipole field. The increase in surface dipole magnetic field results in the observed low braking index of $n=0."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.02734","kind":"arxiv","version":3},"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":"1709.02734","created_at":"2026-05-18T00:26:28.872225+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.02734v3","created_at":"2026-05-18T00:26:28.872225+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.02734","created_at":"2026-05-18T00:26:28.872225+00:00"},{"alias_kind":"pith_short_12","alias_value":"7WLQDTLTGONE","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"7WLQDTLTGONEAVTS","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"7WLQDTLT","created_at":"2026-05-18T12:31:05.417338+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/7WLQDTLTGONEAVTSGH7IC5JPZS","json":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS.json","graph_json":"https://pith.science/api/pith-number/7WLQDTLTGONEAVTSGH7IC5JPZS/graph.json","events_json":"https://pith.science/api/pith-number/7WLQDTLTGONEAVTSGH7IC5JPZS/events.json","paper":"https://pith.science/paper/7WLQDTLT"},"agent_actions":{"view_html":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS","download_json":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS.json","view_paper":"https://pith.science/paper/7WLQDTLT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.02734&json=true","fetch_graph":"https://pith.science/api/pith-number/7WLQDTLTGONEAVTSGH7IC5JPZS/graph.json","fetch_events":"https://pith.science/api/pith-number/7WLQDTLTGONEAVTSGH7IC5JPZS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS/action/storage_attestation","attest_author":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS/action/author_attestation","sign_citation":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS/action/citation_signature","submit_replication":"https://pith.science/pith/7WLQDTLTGONEAVTSGH7IC5JPZS/action/replication_record"}},"created_at":"2026-05-18T00:26:28.872225+00:00","updated_at":"2026-05-18T00:26:28.872225+00:00"}