{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LOB7WKIVZXAKNXKBYFKBYMFWY5","short_pith_number":"pith:LOB7WKIV","schema_version":"1.0","canonical_sha256":"5b83fb2915cdc0a6dd41c1541c30b6c74548797c8f951ee737f3060b9934b1d0","source":{"kind":"arxiv","id":"1305.0237","version":2},"attestation_state":"computed","paper":{"title":"micrOMEGAs3.1 : a program for calculating dark matter observables","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","submitted_at":"2013-05-01T18:04:38Z","abstract_excerpt":"micrOMEGAs is a code to compute dark matter observables in generic extensions of the standard model. This new version of micrOMEGAs is a major update which includes a generalization of the Boltzmann equations to accommodate models with asymmetric dark matter or with semi-annihilation and a first approach to a generalization of the thermodynamics of the Universe in the relic density computation. Furthermore a switch to include virtual vector bosons in the final states in the annihilation cross sections or relic density computations is added. Effective operators to describe loop-induced coupling"},"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":"1305.0237","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-05-01T18:04:38Z","cross_cats_sorted":[],"title_canon_sha256":"5806bdf83c8d3e4c3747abccb38bda176f05d75529c7a97a36f996e852a3e406","abstract_canon_sha256":"5fd70f66f3b49777ccb4b13010e9dd6d0a60b92ba2cc30a05e193f685b74b4f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:13.612956Z","signature_b64":"ytVuJoKqYQA++mT9IR9SDLkA9+IXPzRT0ye1hDimth4340k1sKiSfc7HGrELw/tNDDqi5ZnBu59vBUBKGTpJAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b83fb2915cdc0a6dd41c1541c30b6c74548797c8f951ee737f3060b9934b1d0","last_reissued_at":"2026-05-18T01:50:13.612349Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:13.612349Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"micrOMEGAs3.1 : a program for calculating dark matter observables","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","submitted_at":"2013-05-01T18:04:38Z","abstract_excerpt":"micrOMEGAs is a code to compute dark matter observables in generic extensions of the standard model. This new version of micrOMEGAs is a major update which includes a generalization of the Boltzmann equations to accommodate models with asymmetric dark matter or with semi-annihilation and a first approach to a generalization of the thermodynamics of the Universe in the relic density computation. Furthermore a switch to include virtual vector bosons in the final states in the annihilation cross sections or relic density computations is added. Effective operators to describe loop-induced coupling"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.0237","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":"1305.0237","created_at":"2026-05-18T01:50:13.612440+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.0237v2","created_at":"2026-05-18T01:50:13.612440+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.0237","created_at":"2026-05-18T01:50:13.612440+00:00"},{"alias_kind":"pith_short_12","alias_value":"LOB7WKIVZXAK","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LOB7WKIVZXAKNXKB","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LOB7WKIV","created_at":"2026-05-18T12:27:51.066281+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2507.08927","citing_title":"Deciphering compressed electroweakino excesses with MadAnalysis 5","ref_index":102,"is_internal_anchor":true},{"citing_arxiv_id":"2511.16762","citing_title":"Radiative neutrino mass generation and dark matter through vectorlike leptons","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2511.21808","citing_title":"A Comprehensive Study of WIMP Models Explaining the Fermi-LAT Galactic Center Excess","ref_index":72,"is_internal_anchor":true},{"citing_arxiv_id":"2605.14447","citing_title":"Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11082","citing_title":"Dark Matter as a Source for Lepton Flavor Violation","ref_index":62,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5","json":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5.json","graph_json":"https://pith.science/api/pith-number/LOB7WKIVZXAKNXKBYFKBYMFWY5/graph.json","events_json":"https://pith.science/api/pith-number/LOB7WKIVZXAKNXKBYFKBYMFWY5/events.json","paper":"https://pith.science/paper/LOB7WKIV"},"agent_actions":{"view_html":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5","download_json":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5.json","view_paper":"https://pith.science/paper/LOB7WKIV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.0237&json=true","fetch_graph":"https://pith.science/api/pith-number/LOB7WKIVZXAKNXKBYFKBYMFWY5/graph.json","fetch_events":"https://pith.science/api/pith-number/LOB7WKIVZXAKNXKBYFKBYMFWY5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5/action/storage_attestation","attest_author":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5/action/author_attestation","sign_citation":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5/action/citation_signature","submit_replication":"https://pith.science/pith/LOB7WKIVZXAKNXKBYFKBYMFWY5/action/replication_record"}},"created_at":"2026-05-18T01:50:13.612440+00:00","updated_at":"2026-05-18T01:50:13.612440+00:00"}