{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:TUCG2UMOEBOKAY3AE5PBCRF6K4","short_pith_number":"pith:TUCG2UMO","schema_version":"1.0","canonical_sha256":"9d046d518e205ca06360275e1144be5729b0c4a64afd4f99179b23cf67cda1e6","source":{"kind":"arxiv","id":"1705.04761","version":2},"attestation_state":"computed","paper":{"title":"On the production of heavy axion-like particles in the accretion disks of gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Matias M. Reynoso","submitted_at":"2017-05-12T22:13:15Z","abstract_excerpt":"Heavy axion-like particles have been introduced in several scenarios beyond the Standard Model and their production in some astrophysical systems should be possible. In this work, we re-examine the possibility that these type of particles can be generated in the accretion disks of gamma-ray bursts (GRB), the most powerful events in the universe. If the produced axions decay into photons or $e^+e-$ pairs at the correct distances, a fireball is generated. We calculate the structure transient accretion disks in GRBs (density, temperature and thickness profiles) taking into account the effect of h"},"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":"1705.04761","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-12T22:13:15Z","cross_cats_sorted":[],"title_canon_sha256":"4666634cfcdf0abc4c9fd3949f75f3c3059c28bbf89a68a046c13197224bbefb","abstract_canon_sha256":"e3410f0d3df69ebaaea1302e12ce984023598dbf59690fc08183b08ff36430ec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:55.746263Z","signature_b64":"Msdmw8wdp/kKmHpxoNd9dSvCCKUKmpMn3ij0s9tp/Ho0j4sA2S7Z5VfbBHjidbuXs0GhZtQH61PXD1AGG9CuBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d046d518e205ca06360275e1144be5729b0c4a64afd4f99179b23cf67cda1e6","last_reissued_at":"2026-05-18T00:28:55.745635Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:55.745635Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the production of heavy axion-like particles in the accretion disks of gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Matias M. Reynoso","submitted_at":"2017-05-12T22:13:15Z","abstract_excerpt":"Heavy axion-like particles have been introduced in several scenarios beyond the Standard Model and their production in some astrophysical systems should be possible. In this work, we re-examine the possibility that these type of particles can be generated in the accretion disks of gamma-ray bursts (GRB), the most powerful events in the universe. If the produced axions decay into photons or $e^+e-$ pairs at the correct distances, a fireball is generated. We calculate the structure transient accretion disks in GRBs (density, temperature and thickness profiles) taking into account the effect of h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.04761","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":"1705.04761","created_at":"2026-05-18T00:28:55.745746+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.04761v2","created_at":"2026-05-18T00:28:55.745746+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.04761","created_at":"2026-05-18T00:28:55.745746+00:00"},{"alias_kind":"pith_short_12","alias_value":"TUCG2UMOEBOK","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"TUCG2UMOEBOKAY3A","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"TUCG2UMO","created_at":"2026-05-18T12:31:46.661854+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07297","citing_title":"Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts","ref_index":47,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4","json":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4.json","graph_json":"https://pith.science/api/pith-number/TUCG2UMOEBOKAY3AE5PBCRF6K4/graph.json","events_json":"https://pith.science/api/pith-number/TUCG2UMOEBOKAY3AE5PBCRF6K4/events.json","paper":"https://pith.science/paper/TUCG2UMO"},"agent_actions":{"view_html":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4","download_json":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4.json","view_paper":"https://pith.science/paper/TUCG2UMO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.04761&json=true","fetch_graph":"https://pith.science/api/pith-number/TUCG2UMOEBOKAY3AE5PBCRF6K4/graph.json","fetch_events":"https://pith.science/api/pith-number/TUCG2UMOEBOKAY3AE5PBCRF6K4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4/action/storage_attestation","attest_author":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4/action/author_attestation","sign_citation":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4/action/citation_signature","submit_replication":"https://pith.science/pith/TUCG2UMOEBOKAY3AE5PBCRF6K4/action/replication_record"}},"created_at":"2026-05-18T00:28:55.745746+00:00","updated_at":"2026-05-18T00:28:55.745746+00:00"}