{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FNACG7MBMFLU3JEXWEKDP3VME6","short_pith_number":"pith:FNACG7MB","schema_version":"1.0","canonical_sha256":"2b40237d8161574da497b11437eeac27b3d5ae364bd42fc00f477ca5868a623b","source":{"kind":"arxiv","id":"1804.00044","version":2},"attestation_state":"computed","paper":{"title":"MadDM v.3.0: a Comprehensive Tool for Dark Matter Studies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Chiara Arina, Fabio Maltoni, Federico Ambrogi, Gopolang Mohlabeng, Jan Heisig, Luca Mantani, Mihailo Backovic, Olivier Mattelaer","submitted_at":"2018-03-30T20:00:42Z","abstract_excerpt":"We present MadDM v.3.0, a numerical tool to compute particle dark matter observables in generic new physics models. The new version features a comprehensive and automated framework for dark matter searches at the interface of collider physics, astrophysics and cosmology and is deployed as a plugin of the MadGraph5_aMC@NLO platform, inheriting most of its features. With respect to the previous version, MadDM v.3.0 can now provide predictions for indirect dark matter signatures in astrophysical environments, such as the annihilation cross section at present time and the energy spectra of prompt "},"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":"1804.00044","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-03-30T20:00:42Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e36b85e68b6c9adab0a755eff6f8c189e03011d14da66413f340ba24a4be8b76","abstract_canon_sha256":"32d3e1c2c5bd3a1d908239e2e7856cab2e9788cb44a8bfc8987ae915bd77feef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:56:05.424499Z","signature_b64":"8aSiT58erQfZY1t+/nixCVKddWAn1DBK+oyrwbds2A2A1e2N59AeMieCexVjM+psGzq2zaDMGxcUehL9LJdGCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b40237d8161574da497b11437eeac27b3d5ae364bd42fc00f477ca5868a623b","last_reissued_at":"2026-05-17T23:56:05.423816Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:56:05.423816Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"MadDM v.3.0: a Comprehensive Tool for Dark Matter Studies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Chiara Arina, Fabio Maltoni, Federico Ambrogi, Gopolang Mohlabeng, Jan Heisig, Luca Mantani, Mihailo Backovic, Olivier Mattelaer","submitted_at":"2018-03-30T20:00:42Z","abstract_excerpt":"We present MadDM v.3.0, a numerical tool to compute particle dark matter observables in generic new physics models. The new version features a comprehensive and automated framework for dark matter searches at the interface of collider physics, astrophysics and cosmology and is deployed as a plugin of the MadGraph5_aMC@NLO platform, inheriting most of its features. With respect to the previous version, MadDM v.3.0 can now provide predictions for indirect dark matter signatures in astrophysical environments, such as the annihilation cross section at present time and the energy spectra of prompt "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.00044","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":"1804.00044","created_at":"2026-05-17T23:56:05.423919+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.00044v2","created_at":"2026-05-17T23:56:05.423919+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.00044","created_at":"2026-05-17T23:56:05.423919+00:00"},{"alias_kind":"pith_short_12","alias_value":"FNACG7MBMFLU","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_16","alias_value":"FNACG7MBMFLU3JEX","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_8","alias_value":"FNACG7MB","created_at":"2026-05-18T12:32:22.470017+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2508.15891","citing_title":"Constraining light dark matter in vector-scalar portals with COSI and AMEGO-X","ref_index":53,"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":69,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6","json":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6.json","graph_json":"https://pith.science/api/pith-number/FNACG7MBMFLU3JEXWEKDP3VME6/graph.json","events_json":"https://pith.science/api/pith-number/FNACG7MBMFLU3JEXWEKDP3VME6/events.json","paper":"https://pith.science/paper/FNACG7MB"},"agent_actions":{"view_html":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6","download_json":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6.json","view_paper":"https://pith.science/paper/FNACG7MB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.00044&json=true","fetch_graph":"https://pith.science/api/pith-number/FNACG7MBMFLU3JEXWEKDP3VME6/graph.json","fetch_events":"https://pith.science/api/pith-number/FNACG7MBMFLU3JEXWEKDP3VME6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6/action/storage_attestation","attest_author":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6/action/author_attestation","sign_citation":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6/action/citation_signature","submit_replication":"https://pith.science/pith/FNACG7MBMFLU3JEXWEKDP3VME6/action/replication_record"}},"created_at":"2026-05-17T23:56:05.423919+00:00","updated_at":"2026-05-17T23:56:05.423919+00:00"}