{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:PKQQPLAP2U23MJUT6VP72Q3SNE","short_pith_number":"pith:PKQQPLAP","schema_version":"1.0","canonical_sha256":"7aa107ac0fd535b62693f55ffd437269108bcd455a194933750f203f3b69129a","source":{"kind":"arxiv","id":"1004.1092","version":2},"attestation_state":"computed","paper":{"title":"Indirect search for dark matter with micrOMEGAs2.4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Pukhov, A. Semenov, F. Boudjema, G. Belanger, P. Brun, P. Salati, S. Rosier-Lees","submitted_at":"2010-04-07T13:55:33Z","abstract_excerpt":"We present a new module of micrOMEGAs devoted to the computation of indirect signals from dark matter annihilation in any new model with a stable weakly interacting particle. The code provides the mass spectrum, cross-sections, relic density and exotic fluxes of gamma rays, positrons and antiprotons. The propagation of charged particles in the Galactic halo is handled with a new module that allows to easily modify the propagation parameters."},"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":"1004.1092","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-04-07T13:55:33Z","cross_cats_sorted":[],"title_canon_sha256":"5e8cc81eceb809a2db43855d2d2a0db92fc294ac023c2466159ed1496b10d412","abstract_canon_sha256":"33e72b895db952f0560d9636726cca33dfa9504c3773a068ddb87246cdf1fd7f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:31:41.271210Z","signature_b64":"HNZQyjZmbiIHTRkdUhtJ8IVfR5J3r4e2R931f+EcTbyHQpitbLIBp0oiI3cE2yTRWkSZSJ/OUjpjQ8oIMliiCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7aa107ac0fd535b62693f55ffd437269108bcd455a194933750f203f3b69129a","last_reissued_at":"2026-05-18T04:31:41.270016Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:31:41.270016Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Indirect search for dark matter with micrOMEGAs2.4","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Pukhov, A. Semenov, F. Boudjema, G. Belanger, P. Brun, P. Salati, S. Rosier-Lees","submitted_at":"2010-04-07T13:55:33Z","abstract_excerpt":"We present a new module of micrOMEGAs devoted to the computation of indirect signals from dark matter annihilation in any new model with a stable weakly interacting particle. The code provides the mass spectrum, cross-sections, relic density and exotic fluxes of gamma rays, positrons and antiprotons. The propagation of charged particles in the Galactic halo is handled with a new module that allows to easily modify the propagation parameters."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.1092","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":"1004.1092","created_at":"2026-05-18T04:31:41.270199+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.1092v2","created_at":"2026-05-18T04:31:41.270199+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.1092","created_at":"2026-05-18T04:31:41.270199+00:00"},{"alias_kind":"pith_short_12","alias_value":"PKQQPLAP2U23","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"PKQQPLAP2U23MJUT","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"PKQQPLAP","created_at":"2026-05-18T12:26:12.377268+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.06645","citing_title":"micrOMEGAs 7: Beyond standard cosmology","ref_index":67,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05410","citing_title":"BSMArt 2: simpler and faster parameter space scans","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11082","citing_title":"Dark Matter as a Source for Lepton Flavor Violation","ref_index":61,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE","json":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE.json","graph_json":"https://pith.science/api/pith-number/PKQQPLAP2U23MJUT6VP72Q3SNE/graph.json","events_json":"https://pith.science/api/pith-number/PKQQPLAP2U23MJUT6VP72Q3SNE/events.json","paper":"https://pith.science/paper/PKQQPLAP"},"agent_actions":{"view_html":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE","download_json":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE.json","view_paper":"https://pith.science/paper/PKQQPLAP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.1092&json=true","fetch_graph":"https://pith.science/api/pith-number/PKQQPLAP2U23MJUT6VP72Q3SNE/graph.json","fetch_events":"https://pith.science/api/pith-number/PKQQPLAP2U23MJUT6VP72Q3SNE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE/action/storage_attestation","attest_author":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE/action/author_attestation","sign_citation":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE/action/citation_signature","submit_replication":"https://pith.science/pith/PKQQPLAP2U23MJUT6VP72Q3SNE/action/replication_record"}},"created_at":"2026-05-18T04:31:41.270199+00:00","updated_at":"2026-05-18T04:31:41.270199+00:00"}