{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:7BK3RCLJJXRQZXPCUFEUJMFGZH","short_pith_number":"pith:7BK3RCLJ","canonical_record":{"source":{"id":"1310.3545","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-14T02:13:05Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"9aa2433741b3025fe237134719ec758d7825a46b23d2eb080b2fcff32cd29a16","abstract_canon_sha256":"46c0b8d87d9c715cab4e4dd3e2f51564a0094857e916464f8b5ad3b5b6e9e59d"},"schema_version":"1.0"},"canonical_sha256":"f855b889694de30cdde2a14944b0a6c9f2166921a9db0f9ec1cb6d954dd82fe5","source":{"kind":"arxiv","id":"1310.3545","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.3545","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"arxiv_version","alias_value":"1310.3545v2","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3545","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"pith_short_12","alias_value":"7BK3RCLJJXRQ","created_at":"2026-05-18T12:27:36Z"},{"alias_kind":"pith_short_16","alias_value":"7BK3RCLJJXRQZXPC","created_at":"2026-05-18T12:27:36Z"},{"alias_kind":"pith_short_8","alias_value":"7BK3RCLJ","created_at":"2026-05-18T12:27:36Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:7BK3RCLJJXRQZXPCUFEUJMFGZH","target":"record","payload":{"canonical_record":{"source":{"id":"1310.3545","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-14T02:13:05Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"9aa2433741b3025fe237134719ec758d7825a46b23d2eb080b2fcff32cd29a16","abstract_canon_sha256":"46c0b8d87d9c715cab4e4dd3e2f51564a0094857e916464f8b5ad3b5b6e9e59d"},"schema_version":"1.0"},"canonical_sha256":"f855b889694de30cdde2a14944b0a6c9f2166921a9db0f9ec1cb6d954dd82fe5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:05.971727Z","signature_b64":"6+3obVv0spCb2kYmCjc6NENWvjZMfeLNk1ckuk0bmxT7HbIqCCSG7vUhVgXWym30Z2BWFVzoVy4O3UmtSuxoAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f855b889694de30cdde2a14944b0a6c9f2166921a9db0f9ec1cb6d954dd82fe5","last_reissued_at":"2026-05-18T01:47:05.971214Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:05.971214Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1310.3545","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":"2026-05-18T01:47:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"M2dO+2kMSywQUMkJqjOOs5pJmahunUsn8lHVrE3xR66XlSUTxskCjJjbLlUzvLuaetz4u/f9y4rgE+1I9dtMCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T12:37:11.291564Z"},"content_sha256":"903b43af90a609aaef8419ba643b2bc63f65418694577fd786f3a2ff3d414456","schema_version":"1.0","event_id":"sha256:903b43af90a609aaef8419ba643b2bc63f65418694577fd786f3a2ff3d414456"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:7BK3RCLJJXRQZXPCUFEUJMFGZH","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Gamma-Ray Emission in Dissipative Pulsar Magnetospheres: From Theory to Fermi Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alice K. Harding, Constantinos Kalapotharakos, Demosthenes Kazanas","submitted_at":"2013-10-14T02:13:05Z","abstract_excerpt":"We compute the patterns of $\\gamma$-ray emission due to curvature radiation in dissipative pulsar magnetospheres. Our ultimate goal is to construct macrophysical models that are able to reproduce the observed $\\gamma$-ray light-curve phenomenology recently published in the Second Fermi Pulsar Catalog. We apply specific forms of Ohm's law on the open field lines using a broad range for the macroscopic conductivity values that result in solutions ranging, from near-vacuum to near Force-Free. Using these solutions, we generate model $\\gamma$-ray light curves by calculating realistic trajectories "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3545","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":"2026-05-18T01:47:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WnERDtZQcjXkWwHf1ODaO3lpdHIEHKcsI/xTwIh+sEJFkV24jhLCe08l/ya7KjWOG/ETmZXJaBBLSfMwupTUAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T12:37:11.291946Z"},"content_sha256":"dc6c986664fd8058e1b5c8c878c8bfac84294870d985d171dfb9f7d26f7ba8ee","schema_version":"1.0","event_id":"sha256:dc6c986664fd8058e1b5c8c878c8bfac84294870d985d171dfb9f7d26f7ba8ee"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/bundle.json","state_url":"https://pith.science/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/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":"2026-05-27T12:37:11Z","links":{"resolver":"https://pith.science/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH","bundle":"https://pith.science/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/bundle.json","state":"https://pith.science/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7BK3RCLJJXRQZXPCUFEUJMFGZH/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:7BK3RCLJJXRQZXPCUFEUJMFGZH","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":"46c0b8d87d9c715cab4e4dd3e2f51564a0094857e916464f8b5ad3b5b6e9e59d","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-14T02:13:05Z","title_canon_sha256":"9aa2433741b3025fe237134719ec758d7825a46b23d2eb080b2fcff32cd29a16"},"schema_version":"1.0","source":{"id":"1310.3545","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.3545","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"arxiv_version","alias_value":"1310.3545v2","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3545","created_at":"2026-05-18T01:47:05Z"},{"alias_kind":"pith_short_12","alias_value":"7BK3RCLJJXRQ","created_at":"2026-05-18T12:27:36Z"},{"alias_kind":"pith_short_16","alias_value":"7BK3RCLJJXRQZXPC","created_at":"2026-05-18T12:27:36Z"},{"alias_kind":"pith_short_8","alias_value":"7BK3RCLJ","created_at":"2026-05-18T12:27:36Z"}],"graph_snapshots":[{"event_id":"sha256:dc6c986664fd8058e1b5c8c878c8bfac84294870d985d171dfb9f7d26f7ba8ee","target":"graph","created_at":"2026-05-18T01:47:05Z","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":"We compute the patterns of $\\gamma$-ray emission due to curvature radiation in dissipative pulsar magnetospheres. Our ultimate goal is to construct macrophysical models that are able to reproduce the observed $\\gamma$-ray light-curve phenomenology recently published in the Second Fermi Pulsar Catalog. We apply specific forms of Ohm's law on the open field lines using a broad range for the macroscopic conductivity values that result in solutions ranging, from near-vacuum to near Force-Free. Using these solutions, we generate model $\\gamma$-ray light curves by calculating realistic trajectories ","authors_text":"Alice K. Harding, Constantinos Kalapotharakos, Demosthenes Kazanas","cross_cats":["hep-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-14T02:13:05Z","title":"Gamma-Ray Emission in Dissipative Pulsar Magnetospheres: From Theory to Fermi Observations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3545","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":"sha256:903b43af90a609aaef8419ba643b2bc63f65418694577fd786f3a2ff3d414456","target":"record","created_at":"2026-05-18T01:47:05Z","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":"46c0b8d87d9c715cab4e4dd3e2f51564a0094857e916464f8b5ad3b5b6e9e59d","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-14T02:13:05Z","title_canon_sha256":"9aa2433741b3025fe237134719ec758d7825a46b23d2eb080b2fcff32cd29a16"},"schema_version":"1.0","source":{"id":"1310.3545","kind":"arxiv","version":2}},"canonical_sha256":"f855b889694de30cdde2a14944b0a6c9f2166921a9db0f9ec1cb6d954dd82fe5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f855b889694de30cdde2a14944b0a6c9f2166921a9db0f9ec1cb6d954dd82fe5","first_computed_at":"2026-05-18T01:47:05.971214Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:47:05.971214Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"6+3obVv0spCb2kYmCjc6NENWvjZMfeLNk1ckuk0bmxT7HbIqCCSG7vUhVgXWym30Z2BWFVzoVy4O3UmtSuxoAg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:47:05.971727Z","signed_message":"canonical_sha256_bytes"},"source_id":"1310.3545","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:903b43af90a609aaef8419ba643b2bc63f65418694577fd786f3a2ff3d414456","sha256:dc6c986664fd8058e1b5c8c878c8bfac84294870d985d171dfb9f7d26f7ba8ee"],"state_sha256":"4b9c5fcef9a515f09aa4384cf51451c049e5152d67420abd3707b9e1f6ad2bc8"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"woJqJtdDpOKdKNrMPOmutpJvJUkqbyjEvMh0CrdXrc4tUpmHIk2+1Q7sk+HKWmXrS/Nui8UPlnmmt6T9r6V6DQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T12:37:11.296032Z","bundle_sha256":"0afac6011f3db0f0e94560ac1e26a77db2f6cdb2646be027fc1c02f4903cc174"}}