{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:DBWKC4FLLEGQZT7FV7TOGECURA","short_pith_number":"pith:DBWKC4FL","canonical_record":{"source":{"id":"1411.3588","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-13T15:54:18Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"4073708f6f8981d1dd03790b3e695f4a07cfcc86bd804025fb2a97040da25ad8","abstract_canon_sha256":"28869d26cd1829c430b47d4851eb3a4f1540362ec284745f352f5dbc71ab872e"},"schema_version":"1.0"},"canonical_sha256":"186ca170ab590d0ccfe5afe6e310548820ae74ba16fd52fdaaa34452b3251496","source":{"kind":"arxiv","id":"1411.3588","version":4},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.3588","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"arxiv_version","alias_value":"1411.3588v4","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.3588","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"pith_short_12","alias_value":"DBWKC4FLLEGQ","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_16","alias_value":"DBWKC4FLLEGQZT7F","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_8","alias_value":"DBWKC4FL","created_at":"2026-05-18T12:28:25Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:DBWKC4FLLEGQZT7FV7TOGECURA","target":"record","payload":{"canonical_record":{"source":{"id":"1411.3588","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-13T15:54:18Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"4073708f6f8981d1dd03790b3e695f4a07cfcc86bd804025fb2a97040da25ad8","abstract_canon_sha256":"28869d26cd1829c430b47d4851eb3a4f1540362ec284745f352f5dbc71ab872e"},"schema_version":"1.0"},"canonical_sha256":"186ca170ab590d0ccfe5afe6e310548820ae74ba16fd52fdaaa34452b3251496","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:44.649439Z","signature_b64":"ad3fUnBo7pBCJFCbwz8N94rsm6FeJtAoJjK99adJ0QTAWsslx7ZH17eurQic+eFWHM5TPo2jomNrrmb0ziAfAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"186ca170ab590d0ccfe5afe6e310548820ae74ba16fd52fdaaa34452b3251496","last_reissued_at":"2026-05-18T01:37:44.648960Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:44.648960Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1411.3588","source_version":4,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:37:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Z3uagk/UsLuUiRhuJIy63/X/wWc3uGkcvNy4Q2OkJrfOqUbKQskamOgnI9kMsCnvhWWZFY+TOrITFwzuYnaEAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-07T11:45:39.198346Z"},"content_sha256":"b034494e142b206bddee8223173923a7e403fe0b380c2734a1a3cdb29cfcae47","schema_version":"1.0","event_id":"sha256:b034494e142b206bddee8223173923a7e403fe0b380c2734a1a3cdb29cfcae47"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:DBWKC4FLLEGQZT7FV7TOGECURA","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Neutrino and Cosmic-Ray Emission and Cumulative Background from Radiatively Inefficient Accretion Flows in Low-Luminosity Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Kenji Toma, Kohta Murase, Shigeo S. Kimura","submitted_at":"2014-11-13T15:54:18Z","abstract_excerpt":"We study high-energy neutrino and cosmic-ray (CR) emission from the cores of low-luminosity active galactic nuclei (LLAGN). In LLAGN, the thermalization of particles is expected to be incomplete in radiatively inefficient accretion flows (RIAFs), allowing the existence of non-thermal particles. In this work, assuming stochastic particle acceleration due to turbulence in RIAFs, we solve the Fokker-Planck equation and calculate spectra of escaping neutrinos and CRs. The RIAF in LLAGN can emit CR protons with $\\gtrsim10$ PeV energies and TeV-PeV neutrinos generated via $pp$ and/or $p\\gamma$ react"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.3588","kind":"arxiv","version":4},"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":"2026-05-18T01:37:44Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HwSogpDkd9GYCsIpaP6nFrrG8MYMYmstuBk0K+z7n2Z//ZY7+wp8LeqPBtPirvOp2YyYIs3s4ELvY5lwrDayAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-07T11:45:39.199056Z"},"content_sha256":"c0be0fa6a2ea8bd7f361193363037f162bc742d89d1c6b24eb978edfb7caecba","schema_version":"1.0","event_id":"sha256:c0be0fa6a2ea8bd7f361193363037f162bc742d89d1c6b24eb978edfb7caecba"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/DBWKC4FLLEGQZT7FV7TOGECURA/bundle.json","state_url":"https://pith.science/pith/DBWKC4FLLEGQZT7FV7TOGECURA/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/DBWKC4FLLEGQZT7FV7TOGECURA/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":"2026-06-07T11:45:39Z","links":{"resolver":"https://pith.science/pith/DBWKC4FLLEGQZT7FV7TOGECURA","bundle":"https://pith.science/pith/DBWKC4FLLEGQZT7FV7TOGECURA/bundle.json","state":"https://pith.science/pith/DBWKC4FLLEGQZT7FV7TOGECURA/state.json","well_known_bundle":"https://pith.science/.well-known/pith/DBWKC4FLLEGQZT7FV7TOGECURA/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:DBWKC4FLLEGQZT7FV7TOGECURA","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":"28869d26cd1829c430b47d4851eb3a4f1540362ec284745f352f5dbc71ab872e","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-13T15:54:18Z","title_canon_sha256":"4073708f6f8981d1dd03790b3e695f4a07cfcc86bd804025fb2a97040da25ad8"},"schema_version":"1.0","source":{"id":"1411.3588","kind":"arxiv","version":4}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.3588","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"arxiv_version","alias_value":"1411.3588v4","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.3588","created_at":"2026-05-18T01:37:44Z"},{"alias_kind":"pith_short_12","alias_value":"DBWKC4FLLEGQ","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_16","alias_value":"DBWKC4FLLEGQZT7F","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_8","alias_value":"DBWKC4FL","created_at":"2026-05-18T12:28:25Z"}],"graph_snapshots":[{"event_id":"sha256:c0be0fa6a2ea8bd7f361193363037f162bc742d89d1c6b24eb978edfb7caecba","target":"graph","created_at":"2026-05-18T01:37:44Z","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 study high-energy neutrino and cosmic-ray (CR) emission from the cores of low-luminosity active galactic nuclei (LLAGN). In LLAGN, the thermalization of particles is expected to be incomplete in radiatively inefficient accretion flows (RIAFs), allowing the existence of non-thermal particles. In this work, assuming stochastic particle acceleration due to turbulence in RIAFs, we solve the Fokker-Planck equation and calculate spectra of escaping neutrinos and CRs. The RIAF in LLAGN can emit CR protons with $\\gtrsim10$ PeV energies and TeV-PeV neutrinos generated via $pp$ and/or $p\\gamma$ react","authors_text":"Kenji Toma, Kohta Murase, Shigeo S. Kimura","cross_cats":["hep-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-13T15:54:18Z","title":"Neutrino and Cosmic-Ray Emission and Cumulative Background from Radiatively Inefficient Accretion Flows in Low-Luminosity Active Galactic Nuclei"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.3588","kind":"arxiv","version":4},"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:b034494e142b206bddee8223173923a7e403fe0b380c2734a1a3cdb29cfcae47","target":"record","created_at":"2026-05-18T01:37:44Z","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":"28869d26cd1829c430b47d4851eb3a4f1540362ec284745f352f5dbc71ab872e","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-13T15:54:18Z","title_canon_sha256":"4073708f6f8981d1dd03790b3e695f4a07cfcc86bd804025fb2a97040da25ad8"},"schema_version":"1.0","source":{"id":"1411.3588","kind":"arxiv","version":4}},"canonical_sha256":"186ca170ab590d0ccfe5afe6e310548820ae74ba16fd52fdaaa34452b3251496","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"186ca170ab590d0ccfe5afe6e310548820ae74ba16fd52fdaaa34452b3251496","first_computed_at":"2026-05-18T01:37:44.648960Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:37:44.648960Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"ad3fUnBo7pBCJFCbwz8N94rsm6FeJtAoJjK99adJ0QTAWsslx7ZH17eurQic+eFWHM5TPo2jomNrrmb0ziAfAA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:37:44.649439Z","signed_message":"canonical_sha256_bytes"},"source_id":"1411.3588","source_kind":"arxiv","source_version":4}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b034494e142b206bddee8223173923a7e403fe0b380c2734a1a3cdb29cfcae47","sha256:c0be0fa6a2ea8bd7f361193363037f162bc742d89d1c6b24eb978edfb7caecba"],"state_sha256":"884d7244dbcc9b022e1705ab2b170c258ca80760794a4509fe1d01c341f13eb5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"qlX0fNjoNeA8Yr45Hem5V3qVvwGrJWgwm+0IFl3F2YYp1QHTzabVI7Nd7ZZfHCmHMFVloLFuq5eoiusQqfkmCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-07T11:45:39.202648Z","bundle_sha256":"adf451b9be7e94eb787c6d10b6ea1f67a7323926c9405797bfe9dbd5a7f1edcd"}}