{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:4TTKOLIDJKGZ2BN24QTL6TMDR5","short_pith_number":"pith:4TTKOLID","schema_version":"1.0","canonical_sha256":"e4e6a72d034a8d9d05bae426bf4d838f5be90e42146802f772071bf499b35b56","source":{"kind":"arxiv","id":"1506.05461","version":2},"attestation_state":"computed","paper":{"title":"Hadronic origin of multi-TeV gamma rays and neutrinos from low-luminosity active galactic nuclei: implications of past activities of the Galactic center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Kohta Murase, Shigeo S. Kimura, Yutaka Fujita","submitted_at":"2015-06-17T20:00:39Z","abstract_excerpt":"Radiatively inefficient accretion flows (RIAFs) in low-luminosity active galactic nuclei (LLAGNs) have been suggested as cosmic-ray and neutrino sources that may largely contribute to the observed diffuse neutrino intensity. We show that this scenario naturally predicts hadronic multi-TeV gamma-ray excesses around Galactic centers. The protons accelerated in the RIAF in Sagittarius A$^*$ (Sgr A$^*$) escape and interact with dense molecular gas surrounding Sgr A$^*$, which is known as the central molecular zone (CMZ), and produce gamma rays as well as neutrinos. Based on a theoretical model tha"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1506.05461","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-06-17T20:00:39Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"525dbaebe9e4e01a3d36ba57b92f64718b4f7120435719afca4f7902b5c8931a","abstract_canon_sha256":"052ed2d744f62a21388ec6cc7b25be7ec8d594eac75baee410d41353ed81077e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:01.352405Z","signature_b64":"XuJvo41rwYRIvvIZEhjMUmKnPsVX7SGcoFZ95SEiIBmWKFDBjhcNtQGJmFhXtEjulpXfQVuVzME1hivxEMs6Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e4e6a72d034a8d9d05bae426bf4d838f5be90e42146802f772071bf499b35b56","last_reissued_at":"2026-05-18T01:37:01.351888Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:01.351888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hadronic origin of multi-TeV gamma rays and neutrinos from low-luminosity active galactic nuclei: implications of past activities of the Galactic center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Kohta Murase, Shigeo S. Kimura, Yutaka Fujita","submitted_at":"2015-06-17T20:00:39Z","abstract_excerpt":"Radiatively inefficient accretion flows (RIAFs) in low-luminosity active galactic nuclei (LLAGNs) have been suggested as cosmic-ray and neutrino sources that may largely contribute to the observed diffuse neutrino intensity. We show that this scenario naturally predicts hadronic multi-TeV gamma-ray excesses around Galactic centers. The protons accelerated in the RIAF in Sagittarius A$^*$ (Sgr A$^*$) escape and interact with dense molecular gas surrounding Sgr A$^*$, which is known as the central molecular zone (CMZ), and produce gamma rays as well as neutrinos. Based on a theoretical model tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.05461","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1506.05461","created_at":"2026-05-18T01:37:01.351971+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.05461v2","created_at":"2026-05-18T01:37:01.351971+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.05461","created_at":"2026-05-18T01:37:01.351971+00:00"},{"alias_kind":"pith_short_12","alias_value":"4TTKOLIDJKGZ","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_16","alias_value":"4TTKOLIDJKGZ2BN2","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_8","alias_value":"4TTKOLID","created_at":"2026-05-18T12:29:05.191682+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5","json":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5.json","graph_json":"https://pith.science/api/pith-number/4TTKOLIDJKGZ2BN24QTL6TMDR5/graph.json","events_json":"https://pith.science/api/pith-number/4TTKOLIDJKGZ2BN24QTL6TMDR5/events.json","paper":"https://pith.science/paper/4TTKOLID"},"agent_actions":{"view_html":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5","download_json":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5.json","view_paper":"https://pith.science/paper/4TTKOLID","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.05461&json=true","fetch_graph":"https://pith.science/api/pith-number/4TTKOLIDJKGZ2BN24QTL6TMDR5/graph.json","fetch_events":"https://pith.science/api/pith-number/4TTKOLIDJKGZ2BN24QTL6TMDR5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5/action/storage_attestation","attest_author":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5/action/author_attestation","sign_citation":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5/action/citation_signature","submit_replication":"https://pith.science/pith/4TTKOLIDJKGZ2BN24QTL6TMDR5/action/replication_record"}},"created_at":"2026-05-18T01:37:01.351971+00:00","updated_at":"2026-05-18T01:37:01.351971+00:00"}