{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:U2TPVNC4B23NXNMWKMMVNYXWJC","short_pith_number":"pith:U2TPVNC4","schema_version":"1.0","canonical_sha256":"a6a6fab45c0eb6dbb596531956e2f648ba92624c87772601129d62b8ef238fcb","source":{"kind":"arxiv","id":"hep-ph/0607059","version":1},"attestation_state":"computed","paper":{"title":"micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A.Pukhov, A.Semenov, F.Boudjema, G. Belanger","submitted_at":"2006-07-05T18:16:40Z","abstract_excerpt":"micrOMEGAs2.0 is a code which calculates the relic density of a stable massive particle in an arbitrary model. The underlying assumption is that there is a conservation law like R-parity in supersymmetry which guarantees the stability of the lightest odd particle. The new physics model must be incorporated in the notation of CalcHEP, a package for the automatic generation of squared matrix elements. Once this is done, all annihilation and coannihilation channels are included automatically in any model. Cross-sections at $v=0$, relevant for indirect detection of dark matter, are also computed a"},"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":"hep-ph/0607059","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2006-07-05T18:16:40Z","cross_cats_sorted":[],"title_canon_sha256":"22c0cb9aa093e4715c20fb14a93d43f26ad4a5fdd534b806b07ec81c3cb12d5c","abstract_canon_sha256":"fae6e6a1ea8712697c00a910a810136aab982c170eb3de93e41beca8959a86de"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:26:03.206353Z","signature_b64":"W+3BBUcwYOK5RAwDrrqQ2eN2wB/BIMDLdxVmX262nxgpoG5v+IUyX70T3xnNDj6JxgYiQslGt5i9FBAZfQThBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a6a6fab45c0eb6dbb596531956e2f648ba92624c87772601129d62b8ef238fcb","last_reissued_at":"2026-07-04T15:26:03.205915Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:26:03.205915Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A.Pukhov, A.Semenov, F.Boudjema, G. Belanger","submitted_at":"2006-07-05T18:16:40Z","abstract_excerpt":"micrOMEGAs2.0 is a code which calculates the relic density of a stable massive particle in an arbitrary model. The underlying assumption is that there is a conservation law like R-parity in supersymmetry which guarantees the stability of the lightest odd particle. The new physics model must be incorporated in the notation of CalcHEP, a package for the automatic generation of squared matrix elements. Once this is done, all annihilation and coannihilation channels are included automatically in any model. Cross-sections at $v=0$, relevant for indirect detection of dark matter, are also computed a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0607059","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/0607059/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"hep-ph/0607059","created_at":"2026-07-04T15:26:03.205986+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0607059v1","created_at":"2026-07-04T15:26:03.205986+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0607059","created_at":"2026-07-04T15:26:03.205986+00:00"},{"alias_kind":"pith_short_12","alias_value":"U2TPVNC4B23N","created_at":"2026-07-04T15:26:03.205986+00:00"},{"alias_kind":"pith_short_16","alias_value":"U2TPVNC4B23NXNMW","created_at":"2026-07-04T15:26:03.205986+00:00"},{"alias_kind":"pith_short_8","alias_value":"U2TPVNC4","created_at":"2026-07-04T15:26:03.205986+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":6,"sample":[{"citing_arxiv_id":"2606.23457","citing_title":"Charting Dark Matter down to the neutrino floor/fog in the 2HD+a scenario","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06645","citing_title":"micrOMEGAs 7: Beyond standard cosmology","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2605.29031","citing_title":"Twilight of the WIMP: Comprehensive Phenomenology of Electroweak Triplet Dark Matter","ref_index":71,"is_internal_anchor":true},{"citing_arxiv_id":"2409.16961","citing_title":"Correlative study of flavor anomalies and dark matter in the light of scalar leptoquark","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2509.01682","citing_title":"Towards a Unified Framework for Pseudo-Nambu-Goldstone Dark Matter and Electroweak Baryogenesis","ref_index":39,"is_internal_anchor":true},{"citing_arxiv_id":"2605.05312","citing_title":"Monochromatic neutrinos from scotogenic dark matter","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11082","citing_title":"Dark Matter as a Source for Lepton Flavor Violation","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC","json":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC.json","graph_json":"https://pith.science/api/pith-number/U2TPVNC4B23NXNMWKMMVNYXWJC/graph.json","events_json":"https://pith.science/api/pith-number/U2TPVNC4B23NXNMWKMMVNYXWJC/events.json","paper":"https://pith.science/paper/U2TPVNC4"},"agent_actions":{"view_html":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC","download_json":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC.json","view_paper":"https://pith.science/paper/U2TPVNC4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0607059&json=true","fetch_graph":"https://pith.science/api/pith-number/U2TPVNC4B23NXNMWKMMVNYXWJC/graph.json","fetch_events":"https://pith.science/api/pith-number/U2TPVNC4B23NXNMWKMMVNYXWJC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC/action/storage_attestation","attest_author":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC/action/author_attestation","sign_citation":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC/action/citation_signature","submit_replication":"https://pith.science/pith/U2TPVNC4B23NXNMWKMMVNYXWJC/action/replication_record"}},"created_at":"2026-07-04T15:26:03.205986+00:00","updated_at":"2026-07-04T15:26:03.205986+00:00"}