{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:LJWAHHHSD77DKJRSYUHAYWSCGW","short_pith_number":"pith:LJWAHHHS","schema_version":"1.0","canonical_sha256":"5a6c039cf21ffe352632c50e0c5a4235a30a4fd009c369daaa5bfe85abc95faa","source":{"kind":"arxiv","id":"1909.02824","version":2},"attestation_state":"computed","paper":{"title":"The impact of non-dipolar magnetic fields in core-collapse supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"J. Guilet, M. \\'A. Aloy, M. Bugli, M. Obergaulinger, P. Cerd\\'a-Dur\\'an","submitted_at":"2019-09-06T11:35:56Z","abstract_excerpt":"The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\\,\\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core"},"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":"1909.02824","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-09-06T11:35:56Z","cross_cats_sorted":[],"title_canon_sha256":"97bd80ff44977f38f50273dc3ddb92de6bf568402111fa504b99b6351b435ebf","abstract_canon_sha256":"dba7185def90500191ec38f8650ff21c87aafe2aebdfa62747e059e8053228c5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:33:53.938481Z","signature_b64":"RASSsHV0SwrMCXoUb2T7Zl0oprwL1J6luy11H2NT8LZEJ8a0vMUGI8xknRRk+bI/hf8d7LYxRy6khsWOfm8vAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5a6c039cf21ffe352632c50e0c5a4235a30a4fd009c369daaa5bfe85abc95faa","last_reissued_at":"2026-07-05T00:33:53.937986Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:33:53.937986Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The impact of non-dipolar magnetic fields in core-collapse supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"J. Guilet, M. \\'A. Aloy, M. Bugli, M. Obergaulinger, P. Cerd\\'a-Dur\\'an","submitted_at":"2019-09-06T11:35:56Z","abstract_excerpt":"The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\\,\\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.02824","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/1909.02824/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":"1909.02824","created_at":"2026-07-05T00:33:53.938060+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.02824v2","created_at":"2026-07-05T00:33:53.938060+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.02824","created_at":"2026-07-05T00:33:53.938060+00:00"},{"alias_kind":"pith_short_12","alias_value":"LJWAHHHSD77D","created_at":"2026-07-05T00:33:53.938060+00:00"},{"alias_kind":"pith_short_16","alias_value":"LJWAHHHSD77DKJRS","created_at":"2026-07-05T00:33:53.938060+00:00"},{"alias_kind":"pith_short_8","alias_value":"LJWAHHHS","created_at":"2026-07-05T00:33:53.938060+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/LJWAHHHSD77DKJRSYUHAYWSCGW","json":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW.json","graph_json":"https://pith.science/api/pith-number/LJWAHHHSD77DKJRSYUHAYWSCGW/graph.json","events_json":"https://pith.science/api/pith-number/LJWAHHHSD77DKJRSYUHAYWSCGW/events.json","paper":"https://pith.science/paper/LJWAHHHS"},"agent_actions":{"view_html":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW","download_json":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW.json","view_paper":"https://pith.science/paper/LJWAHHHS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.02824&json=true","fetch_graph":"https://pith.science/api/pith-number/LJWAHHHSD77DKJRSYUHAYWSCGW/graph.json","fetch_events":"https://pith.science/api/pith-number/LJWAHHHSD77DKJRSYUHAYWSCGW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW/action/storage_attestation","attest_author":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW/action/author_attestation","sign_citation":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW/action/citation_signature","submit_replication":"https://pith.science/pith/LJWAHHHSD77DKJRSYUHAYWSCGW/action/replication_record"}},"created_at":"2026-07-05T00:33:53.938060+00:00","updated_at":"2026-07-05T00:33:53.938060+00:00"}