{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:UIU2Y2A6HDJ45RSAXPNO7K65RZ","short_pith_number":"pith:UIU2Y2A6","canonical_record":{"source":{"id":"1101.1098","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-05T21:05:33Z","cross_cats_sorted":[],"title_canon_sha256":"45a8d1ce3f40ce0ccf73d6d4d3fb6b511ea5d5a815eb0d43160360c2814f023c","abstract_canon_sha256":"9bce116f524da491d4f36e7e566dc36a31cef8a74920819ee0094629d22122d7"},"schema_version":"1.0"},"canonical_sha256":"a229ac681e38d3cec640bbdaefabdd8e6ca52e8ad14903d690971b903f47ad5b","source":{"kind":"arxiv","id":"1101.1098","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.1098","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"arxiv_version","alias_value":"1101.1098v1","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.1098","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"pith_short_12","alias_value":"UIU2Y2A6HDJ4","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_16","alias_value":"UIU2Y2A6HDJ45RSA","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_8","alias_value":"UIU2Y2A6","created_at":"2026-05-18T12:26:42Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:UIU2Y2A6HDJ45RSAXPNO7K65RZ","target":"record","payload":{"canonical_record":{"source":{"id":"1101.1098","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-05T21:05:33Z","cross_cats_sorted":[],"title_canon_sha256":"45a8d1ce3f40ce0ccf73d6d4d3fb6b511ea5d5a815eb0d43160360c2814f023c","abstract_canon_sha256":"9bce116f524da491d4f36e7e566dc36a31cef8a74920819ee0094629d22122d7"},"schema_version":"1.0"},"canonical_sha256":"a229ac681e38d3cec640bbdaefabdd8e6ca52e8ad14903d690971b903f47ad5b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:59:36.905039Z","signature_b64":"07TOxvjw1jc9SvL/5cqeZYd7xpMctYEEaZuWMZL/ShF+u8bRRZWUW46el2zeBN9/gADOIuEGDcfBvm8tNXuiBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a229ac681e38d3cec640bbdaefabdd8e6ca52e8ad14903d690971b903f47ad5b","last_reissued_at":"2026-05-18T03:59:36.904239Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:59:36.904239Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1101.1098","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:59:36Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xM5o3KVar9oOfYzm3RSzeYuQzhNxCWmR7WgFoo5L6Khug+PSixdUSuaSB6eu1wVbV9BqC08l4RH348oeMP2MBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T21:36:31.747101Z"},"content_sha256":"b62b9efda9538b80057c1cd72eb464bf29e8a65596be7a7de0a598d912873d09","schema_version":"1.0","event_id":"sha256:b62b9efda9538b80057c1cd72eb464bf29e8a65596be7a7de0a598d912873d09"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:UIU2Y2A6HDJ45RSAXPNO7K65RZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A unified model of the magnetar and radio pulsar bursting phenomenology","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jose A. Pons (Universitat d'Alacant, Rosalba Perna (JILA/Colorado), Spain)","submitted_at":"2011-01-05T21:05:33Z","abstract_excerpt":"Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) are young neutron stars (NSs) characterized by high X-ray quiescent luminosities, outbursts, and, in the case of SGRs, sporadic giant flares. They are believed to be powered by ultra-strong magnetic fields (hence dubbed magnetars). The diversity of their observed behaviours is however not understood, and made even more puzzling by the discovery of magnetar-like bursts from \"low-field\" pulsars. Here we perform long-term 2D simulations that follow the evolution of magnetic stresses in the crust; these, together with recent calcul"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.1098","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:59:36Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5s/i7aybzAl0wbhBRcMRmNdv9rvpm1cIP7F764I+cKpiKAUV8am4oXEMGQm3MMNwyMATs9GH0wXZESReawQiDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T21:36:31.747459Z"},"content_sha256":"bd21b44a6584d1944e1c3f2cf4bc3a56ca87ce95dcb8813d6ed74ea8aaa982b4","schema_version":"1.0","event_id":"sha256:bd21b44a6584d1944e1c3f2cf4bc3a56ca87ce95dcb8813d6ed74ea8aaa982b4"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/bundle.json","state_url":"https://pith.science/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-02T21:36:31Z","links":{"resolver":"https://pith.science/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ","bundle":"https://pith.science/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/bundle.json","state":"https://pith.science/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/UIU2Y2A6HDJ45RSAXPNO7K65RZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:UIU2Y2A6HDJ45RSAXPNO7K65RZ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"9bce116f524da491d4f36e7e566dc36a31cef8a74920819ee0094629d22122d7","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-05T21:05:33Z","title_canon_sha256":"45a8d1ce3f40ce0ccf73d6d4d3fb6b511ea5d5a815eb0d43160360c2814f023c"},"schema_version":"1.0","source":{"id":"1101.1098","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.1098","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"arxiv_version","alias_value":"1101.1098v1","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.1098","created_at":"2026-05-18T03:59:36Z"},{"alias_kind":"pith_short_12","alias_value":"UIU2Y2A6HDJ4","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_16","alias_value":"UIU2Y2A6HDJ45RSA","created_at":"2026-05-18T12:26:42Z"},{"alias_kind":"pith_short_8","alias_value":"UIU2Y2A6","created_at":"2026-05-18T12:26:42Z"}],"graph_snapshots":[{"event_id":"sha256:bd21b44a6584d1944e1c3f2cf4bc3a56ca87ce95dcb8813d6ed74ea8aaa982b4","target":"graph","created_at":"2026-05-18T03:59:36Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) are young neutron stars (NSs) characterized by high X-ray quiescent luminosities, outbursts, and, in the case of SGRs, sporadic giant flares. They are believed to be powered by ultra-strong magnetic fields (hence dubbed magnetars). The diversity of their observed behaviours is however not understood, and made even more puzzling by the discovery of magnetar-like bursts from \"low-field\" pulsars. Here we perform long-term 2D simulations that follow the evolution of magnetic stresses in the crust; these, together with recent calcul","authors_text":"Jose A. Pons (Universitat d'Alacant, Rosalba Perna (JILA/Colorado), Spain)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-05T21:05:33Z","title":"A unified model of the magnetar and radio pulsar bursting phenomenology"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.1098","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:b62b9efda9538b80057c1cd72eb464bf29e8a65596be7a7de0a598d912873d09","target":"record","created_at":"2026-05-18T03:59:36Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"9bce116f524da491d4f36e7e566dc36a31cef8a74920819ee0094629d22122d7","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-05T21:05:33Z","title_canon_sha256":"45a8d1ce3f40ce0ccf73d6d4d3fb6b511ea5d5a815eb0d43160360c2814f023c"},"schema_version":"1.0","source":{"id":"1101.1098","kind":"arxiv","version":1}},"canonical_sha256":"a229ac681e38d3cec640bbdaefabdd8e6ca52e8ad14903d690971b903f47ad5b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a229ac681e38d3cec640bbdaefabdd8e6ca52e8ad14903d690971b903f47ad5b","first_computed_at":"2026-05-18T03:59:36.904239Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:59:36.904239Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"07TOxvjw1jc9SvL/5cqeZYd7xpMctYEEaZuWMZL/ShF+u8bRRZWUW46el2zeBN9/gADOIuEGDcfBvm8tNXuiBA==","signature_status":"signed_v1","signed_at":"2026-05-18T03:59:36.905039Z","signed_message":"canonical_sha256_bytes"},"source_id":"1101.1098","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b62b9efda9538b80057c1cd72eb464bf29e8a65596be7a7de0a598d912873d09","sha256:bd21b44a6584d1944e1c3f2cf4bc3a56ca87ce95dcb8813d6ed74ea8aaa982b4"],"state_sha256":"37f443d988dce304fdfba455dc594591926e5e3450805b84420a32f41b3c24e8"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"hMWXofgkqJRl66qP1hAD6K+9x5IKM+YwWigPE+25/b7LO7lbvP75TL2sM846GqDXPACDzsT0D0PnlNwH3K/GCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T21:36:31.749296Z","bundle_sha256":"bed1cab0aef0cd067b2c0e4912336f827e798b805c97fd9f3f3927dd715ba632"}}