{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:WGRT3DJICWXJ5KTTEGHKKNYDMB","short_pith_number":"pith:WGRT3DJI","canonical_record":{"source":{"id":"1411.7241","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-26T14:26:40Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"db2937e9262881690111dc0e63eb8d6c9783f848d035228c8cb0bb932af9506e","abstract_canon_sha256":"50e7d982314605b55a99ef6d9bd8f74fa6f427a580481113cc12ea639a8f3753"},"schema_version":"1.0"},"canonical_sha256":"b1a33d8d2815ae9eaa73218ea537036052fe070333d844c2632823e3ffd0fc26","source":{"kind":"arxiv","id":"1411.7241","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.7241","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"arxiv_version","alias_value":"1411.7241v3","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.7241","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"pith_short_12","alias_value":"WGRT3DJICWXJ","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_16","alias_value":"WGRT3DJICWXJ5KTT","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_8","alias_value":"WGRT3DJI","created_at":"2026-05-18T12:28:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:WGRT3DJICWXJ5KTTEGHKKNYDMB","target":"record","payload":{"canonical_record":{"source":{"id":"1411.7241","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-26T14:26:40Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"db2937e9262881690111dc0e63eb8d6c9783f848d035228c8cb0bb932af9506e","abstract_canon_sha256":"50e7d982314605b55a99ef6d9bd8f74fa6f427a580481113cc12ea639a8f3753"},"schema_version":"1.0"},"canonical_sha256":"b1a33d8d2815ae9eaa73218ea537036052fe070333d844c2632823e3ffd0fc26","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:35.156840Z","signature_b64":"zbFQQz8GJVUKpz0/Zb03uUNQfj06mqC8QIjnPQG6oXyONF797bLq8/jlzhcevg4bBeV+kpSQYIMTCxd2FFcEDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b1a33d8d2815ae9eaa73218ea537036052fe070333d844c2632823e3ffd0fc26","last_reissued_at":"2026-05-18T02:03:35.156202Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:35.156202Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1411.7241","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:03:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VSEWI/WjbNEu5Abp/k6F3sVRKtMq7zW2dA1NSlX3foYCEwiwN0vEeTakKxg8VqSFfeIwD27dpu2N95RyOpUfDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T13:39:46.376828Z"},"content_sha256":"2aacb74ca60c4f25670d1ed473fee8cca0fec66a67f52b2f7d642db2a9ef8b3f","schema_version":"1.0","event_id":"sha256:2aacb74ca60c4f25670d1ed473fee8cca0fec66a67f52b2f7d642db2a9ef8b3f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:WGRT3DJICWXJ5KTTEGHKKNYDMB","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the role of rotation in the outflows of the Crab pulsar","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Andria Rogava, Irakli Gudavadze, Zaza Osmanov","submitted_at":"2014-11-26T14:26:40Z","abstract_excerpt":"In order to study constraints imposed on kinematics of the Crab pulsar's jet we consider motion of particles along co-rotating field lines in the magnetosphere of the Crab pulsar. It is shown that particles following the co-rotating magnetic field lines may attain velocities close to observable values. In particular, we demonstrate that if the magnetic field lines are within the light cylinder, the maximum value of the velocity component parallel to the rotation axis is limited by $0.5c$. This result in the context of the $X$-ray observations performed by {\\it Chandra X-ray Observatory} seems "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.7241","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:03:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"k8+v1eqzbCQnG3NuLDqMEcOLsjOyLuJSwWLNlYK3JYQzjUEmL3WxBFWauP9rmv0fWWy0ZL3ZdPyP3jOmzK/NBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T13:39:46.377190Z"},"content_sha256":"fc9060379bfc66177c7eef51600c3503416b111645a60f7cb1f2f04a14451595","schema_version":"1.0","event_id":"sha256:fc9060379bfc66177c7eef51600c3503416b111645a60f7cb1f2f04a14451595"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/bundle.json","state_url":"https://pith.science/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/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":"2026-05-30T13:39:46Z","links":{"resolver":"https://pith.science/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB","bundle":"https://pith.science/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/bundle.json","state":"https://pith.science/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/state.json","well_known_bundle":"https://pith.science/.well-known/pith/WGRT3DJICWXJ5KTTEGHKKNYDMB/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:WGRT3DJICWXJ5KTTEGHKKNYDMB","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":"50e7d982314605b55a99ef6d9bd8f74fa6f427a580481113cc12ea639a8f3753","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-26T14:26:40Z","title_canon_sha256":"db2937e9262881690111dc0e63eb8d6c9783f848d035228c8cb0bb932af9506e"},"schema_version":"1.0","source":{"id":"1411.7241","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.7241","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"arxiv_version","alias_value":"1411.7241v3","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.7241","created_at":"2026-05-18T02:03:35Z"},{"alias_kind":"pith_short_12","alias_value":"WGRT3DJICWXJ","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_16","alias_value":"WGRT3DJICWXJ5KTT","created_at":"2026-05-18T12:28:54Z"},{"alias_kind":"pith_short_8","alias_value":"WGRT3DJI","created_at":"2026-05-18T12:28:54Z"}],"graph_snapshots":[{"event_id":"sha256:fc9060379bfc66177c7eef51600c3503416b111645a60f7cb1f2f04a14451595","target":"graph","created_at":"2026-05-18T02:03:35Z","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":"In order to study constraints imposed on kinematics of the Crab pulsar's jet we consider motion of particles along co-rotating field lines in the magnetosphere of the Crab pulsar. It is shown that particles following the co-rotating magnetic field lines may attain velocities close to observable values. In particular, we demonstrate that if the magnetic field lines are within the light cylinder, the maximum value of the velocity component parallel to the rotation axis is limited by $0.5c$. This result in the context of the $X$-ray observations performed by {\\it Chandra X-ray Observatory} seems ","authors_text":"Andria Rogava, Irakli Gudavadze, Zaza Osmanov","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-26T14:26:40Z","title":"On the role of rotation in the outflows of the Crab pulsar"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.7241","kind":"arxiv","version":3},"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":"sha256:2aacb74ca60c4f25670d1ed473fee8cca0fec66a67f52b2f7d642db2a9ef8b3f","target":"record","created_at":"2026-05-18T02:03:35Z","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":"50e7d982314605b55a99ef6d9bd8f74fa6f427a580481113cc12ea639a8f3753","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-26T14:26:40Z","title_canon_sha256":"db2937e9262881690111dc0e63eb8d6c9783f848d035228c8cb0bb932af9506e"},"schema_version":"1.0","source":{"id":"1411.7241","kind":"arxiv","version":3}},"canonical_sha256":"b1a33d8d2815ae9eaa73218ea537036052fe070333d844c2632823e3ffd0fc26","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b1a33d8d2815ae9eaa73218ea537036052fe070333d844c2632823e3ffd0fc26","first_computed_at":"2026-05-18T02:03:35.156202Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:03:35.156202Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"zbFQQz8GJVUKpz0/Zb03uUNQfj06mqC8QIjnPQG6oXyONF797bLq8/jlzhcevg4bBeV+kpSQYIMTCxd2FFcEDg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:03:35.156840Z","signed_message":"canonical_sha256_bytes"},"source_id":"1411.7241","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2aacb74ca60c4f25670d1ed473fee8cca0fec66a67f52b2f7d642db2a9ef8b3f","sha256:fc9060379bfc66177c7eef51600c3503416b111645a60f7cb1f2f04a14451595"],"state_sha256":"1547978d7420b5f701440a164aa14eb355bf168ddf9b82b2c3efad7770c0c28d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uNgd5KF0XfeHnqlaKmeP5XdRrs+o+2BC1OBcRUHYpyO6VhUjg89bxWh7EtRzv26mulle/5XNE0R6q3YUNOUcDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-30T13:39:46.379137Z","bundle_sha256":"0caa520d2ac163f5de706ba6e9fd119d33ca7e1a65af0d5f05b7dfc85c414076"}}