{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:QDLBJTHIVGU6X7LPZIJH6KZVCO","short_pith_number":"pith:QDLBJTHI","schema_version":"1.0","canonical_sha256":"80d614cce8a9a9ebfd6fca127f2b3513b74737e323679cd6fa2e11bbb6f6d93c","source":{"kind":"arxiv","id":"1301.7536","version":2},"attestation_state":"computed","paper":{"title":"Axino dark matter with R-parity violation and 130 GeV gamma-ray line","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Kazunori Nakayama, Koichi Hamaguchi, Kyohei Mukaida, Motoi Endo, Seng Pei Liew","submitted_at":"2013-01-31T07:59:54Z","abstract_excerpt":"We show that decaying axino dark matter with R-parity violation can explain the observed excess of the 130GeV gamma-ray line from the Galactic center in the Fermi data. The branching fraction of the axino decay into monochromatic photons can be O(1), and constraints from continuum gamma-rays and the anti-proton flux are ameliorated. The Peccei-Quinn scale of $O(10^{13}-10^{14})$\\,GeV and the R-parity violation parameter of $O(10^{-12}-10^{-11})$ are cosmologically favored."},"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":"1301.7536","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-01-31T07:59:54Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"e8c5bf6dde90f26a3dde950232ba1a5f54c93d24aaed299c2485196081ab4859","abstract_canon_sha256":"a78438e5d174b67961342d66607c7ae8fb43b64f0bef035dd1f6c149c43a988b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:29:40.376116Z","signature_b64":"j+svkvHqTTkYyLsnk1JT0c8VQgwb0QPmo+NikZSjjw/OjLvRtol6D/sbHY939R+bgB91ikvGLY6H6Bdpl0fFDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"80d614cce8a9a9ebfd6fca127f2b3513b74737e323679cd6fa2e11bbb6f6d93c","last_reissued_at":"2026-05-18T03:29:40.375644Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:29:40.375644Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Axino dark matter with R-parity violation and 130 GeV gamma-ray line","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Kazunori Nakayama, Koichi Hamaguchi, Kyohei Mukaida, Motoi Endo, Seng Pei Liew","submitted_at":"2013-01-31T07:59:54Z","abstract_excerpt":"We show that decaying axino dark matter with R-parity violation can explain the observed excess of the 130GeV gamma-ray line from the Galactic center in the Fermi data. The branching fraction of the axino decay into monochromatic photons can be O(1), and constraints from continuum gamma-rays and the anti-proton flux are ameliorated. The Peccei-Quinn scale of $O(10^{13}-10^{14})$\\,GeV and the R-parity violation parameter of $O(10^{-12}-10^{-11})$ are cosmologically favored."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.7536","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":"1301.7536","created_at":"2026-05-18T03:29:40.375713+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.7536v2","created_at":"2026-05-18T03:29:40.375713+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.7536","created_at":"2026-05-18T03:29:40.375713+00:00"},{"alias_kind":"pith_short_12","alias_value":"QDLBJTHIVGU6","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"QDLBJTHIVGU6X7LP","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"QDLBJTHI","created_at":"2026-05-18T12:27:57.521954+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/QDLBJTHIVGU6X7LPZIJH6KZVCO","json":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO.json","graph_json":"https://pith.science/api/pith-number/QDLBJTHIVGU6X7LPZIJH6KZVCO/graph.json","events_json":"https://pith.science/api/pith-number/QDLBJTHIVGU6X7LPZIJH6KZVCO/events.json","paper":"https://pith.science/paper/QDLBJTHI"},"agent_actions":{"view_html":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO","download_json":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO.json","view_paper":"https://pith.science/paper/QDLBJTHI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.7536&json=true","fetch_graph":"https://pith.science/api/pith-number/QDLBJTHIVGU6X7LPZIJH6KZVCO/graph.json","fetch_events":"https://pith.science/api/pith-number/QDLBJTHIVGU6X7LPZIJH6KZVCO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO/action/storage_attestation","attest_author":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO/action/author_attestation","sign_citation":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO/action/citation_signature","submit_replication":"https://pith.science/pith/QDLBJTHIVGU6X7LPZIJH6KZVCO/action/replication_record"}},"created_at":"2026-05-18T03:29:40.375713+00:00","updated_at":"2026-05-18T03:29:40.375713+00:00"}