{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:KGZK7EA4WJH7FKANRKNOVIH6KT","short_pith_number":"pith:KGZK7EA4","canonical_record":{"source":{"id":"1604.03179","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-04-12T00:04:10Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"560fc40745e5beea7e5775833173466501f29176772ee46a87ae70384cf121e4","abstract_canon_sha256":"474632d4984fe452402c185d082ff0aec689cf5d36961b084a89d687dc5c3e12"},"schema_version":"1.0"},"canonical_sha256":"51b2af901cb24ff2a80d8a9aeaa0fe54c5e50492a92e9459d773b6197bdfcccf","source":{"kind":"arxiv","id":"1604.03179","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.03179","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"arxiv_version","alias_value":"1604.03179v2","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.03179","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"pith_short_12","alias_value":"KGZK7EA4WJH7","created_at":"2026-05-18T12:30:25Z"},{"alias_kind":"pith_short_16","alias_value":"KGZK7EA4WJH7FKAN","created_at":"2026-05-18T12:30:25Z"},{"alias_kind":"pith_short_8","alias_value":"KGZK7EA4","created_at":"2026-05-18T12:30:25Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:KGZK7EA4WJH7FKANRKNOVIH6KT","target":"record","payload":{"canonical_record":{"source":{"id":"1604.03179","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-04-12T00:04:10Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"560fc40745e5beea7e5775833173466501f29176772ee46a87ae70384cf121e4","abstract_canon_sha256":"474632d4984fe452402c185d082ff0aec689cf5d36961b084a89d687dc5c3e12"},"schema_version":"1.0"},"canonical_sha256":"51b2af901cb24ff2a80d8a9aeaa0fe54c5e50492a92e9459d773b6197bdfcccf","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:04:20.986844Z","signature_b64":"baaQyEb3VdyRq86kC/R12pSiaakkEAarli7RB72K2E4ZCuj4r5hRicyeh38Jz95RtWJXDhP4HC0CFCe27Ni3Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"51b2af901cb24ff2a80d8a9aeaa0fe54c5e50492a92e9459d773b6197bdfcccf","last_reissued_at":"2026-05-18T01:04:20.986403Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:04:20.986403Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1604.03179","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:04:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"am5Orq78Dz9DlHPH4purEjCphWKuf8rKoK02uVHch1bdPrdTIuVUjPNqqrtmTGTUbKrOIUQ87sUf3granyhcBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T15:16:38.075329Z"},"content_sha256":"3bed726a3b0a74dc3d7270b00ad0e2f3082b580f69e49b3af0fcc8d902270686","schema_version":"1.0","event_id":"sha256:3bed726a3b0a74dc3d7270b00ad0e2f3082b580f69e49b3af0fcc8d902270686"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:KGZK7EA4WJH7FKANRKNOVIH6KT","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Kinetic study of radiation-reaction-limited particle acceleration during the relaxation of unstable force-free equilibria","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"2), (2) Nicolaus Copernicus Astronomical Center), Jonathan Zrake (1), Krzysztof Nalewajko (1, Roger D. Blandford (1) ((1) KIPAC, SLAC, Stanford University, William E. East (1), Yajie Yuan (1)","submitted_at":"2016-04-12T00:04:10Z","abstract_excerpt":"Many powerful and variable gamma-ray sources, including pulsar wind nebulae, active galactic nuclei and gamma-ray bursts, seem capable of accelerating particles to gamma-ray emitting energies efficiently over very short time scales. These are likely due to rapid dissipation of electromagnetic energy in a highly magnetized, relativistic plasma. In order to understand the generic features of such processes, we have investigated simple models based on relaxation of unstable force-free magnetostatic equilibria. In this work, we make the connection between the corresponding plasma dynamics and the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.03179","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:04:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"l1w0dLw8/83kzdIzy2m5RTCQOujTnEXhwo9tSU6Q1DxwIPLaRpp6bE6EuX9kVOIxAYN5X1yLxYxHxmSHXYEaDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T15:16:38.075686Z"},"content_sha256":"363a16599d77b1cc5e558ba18f694b738e639bf2fcf1d5557d9c2d1f5705b500","schema_version":"1.0","event_id":"sha256:363a16599d77b1cc5e558ba18f694b738e639bf2fcf1d5557d9c2d1f5705b500"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/bundle.json","state_url":"https://pith.science/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/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":"2026-06-01T15:16:38Z","links":{"resolver":"https://pith.science/pith/KGZK7EA4WJH7FKANRKNOVIH6KT","bundle":"https://pith.science/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/bundle.json","state":"https://pith.science/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KGZK7EA4WJH7FKANRKNOVIH6KT/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:KGZK7EA4WJH7FKANRKNOVIH6KT","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":"474632d4984fe452402c185d082ff0aec689cf5d36961b084a89d687dc5c3e12","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-04-12T00:04:10Z","title_canon_sha256":"560fc40745e5beea7e5775833173466501f29176772ee46a87ae70384cf121e4"},"schema_version":"1.0","source":{"id":"1604.03179","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.03179","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"arxiv_version","alias_value":"1604.03179v2","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.03179","created_at":"2026-05-18T01:04:20Z"},{"alias_kind":"pith_short_12","alias_value":"KGZK7EA4WJH7","created_at":"2026-05-18T12:30:25Z"},{"alias_kind":"pith_short_16","alias_value":"KGZK7EA4WJH7FKAN","created_at":"2026-05-18T12:30:25Z"},{"alias_kind":"pith_short_8","alias_value":"KGZK7EA4","created_at":"2026-05-18T12:30:25Z"}],"graph_snapshots":[{"event_id":"sha256:363a16599d77b1cc5e558ba18f694b738e639bf2fcf1d5557d9c2d1f5705b500","target":"graph","created_at":"2026-05-18T01:04:20Z","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":"Many powerful and variable gamma-ray sources, including pulsar wind nebulae, active galactic nuclei and gamma-ray bursts, seem capable of accelerating particles to gamma-ray emitting energies efficiently over very short time scales. These are likely due to rapid dissipation of electromagnetic energy in a highly magnetized, relativistic plasma. In order to understand the generic features of such processes, we have investigated simple models based on relaxation of unstable force-free magnetostatic equilibria. In this work, we make the connection between the corresponding plasma dynamics and the ","authors_text":"2), (2) Nicolaus Copernicus Astronomical Center), Jonathan Zrake (1), Krzysztof Nalewajko (1, Roger D. Blandford (1) ((1) KIPAC, SLAC, Stanford University, William E. East (1), Yajie Yuan (1)","cross_cats":["physics.plasm-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-04-12T00:04:10Z","title":"Kinetic study of radiation-reaction-limited particle acceleration during the relaxation of unstable force-free equilibria"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.03179","kind":"arxiv","version":2},"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":"sha256:3bed726a3b0a74dc3d7270b00ad0e2f3082b580f69e49b3af0fcc8d902270686","target":"record","created_at":"2026-05-18T01:04:20Z","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":"474632d4984fe452402c185d082ff0aec689cf5d36961b084a89d687dc5c3e12","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-04-12T00:04:10Z","title_canon_sha256":"560fc40745e5beea7e5775833173466501f29176772ee46a87ae70384cf121e4"},"schema_version":"1.0","source":{"id":"1604.03179","kind":"arxiv","version":2}},"canonical_sha256":"51b2af901cb24ff2a80d8a9aeaa0fe54c5e50492a92e9459d773b6197bdfcccf","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"51b2af901cb24ff2a80d8a9aeaa0fe54c5e50492a92e9459d773b6197bdfcccf","first_computed_at":"2026-05-18T01:04:20.986403Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:04:20.986403Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"baaQyEb3VdyRq86kC/R12pSiaakkEAarli7RB72K2E4ZCuj4r5hRicyeh38Jz95RtWJXDhP4HC0CFCe27Ni3Bw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:04:20.986844Z","signed_message":"canonical_sha256_bytes"},"source_id":"1604.03179","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3bed726a3b0a74dc3d7270b00ad0e2f3082b580f69e49b3af0fcc8d902270686","sha256:363a16599d77b1cc5e558ba18f694b738e639bf2fcf1d5557d9c2d1f5705b500"],"state_sha256":"0f92d019c761c7aa0c6dcb17c29845ddfefe478263c51625dc7edd2035a3d46e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"q5RFZ/hjGbbcbHoFt4wm4++nCuSZtg+mCrEP6md5aoBC6ntpn5ywXRUYvvlnt19boV17+dzAVBygpmm2KWjeAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T15:16:38.077696Z","bundle_sha256":"0a50506729e582d4392adee3a8bfe4d982e505bf1f753e51c12aa0532dd99262"}}