{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:MVAB5FZRL43MS452CP5EH4EJ4Y","short_pith_number":"pith:MVAB5FZR","schema_version":"1.0","canonical_sha256":"65401e97315f36c973ba13fa43f089e601f9d16c6f2bbb5573a05672986afc74","source":{"kind":"arxiv","id":"2012.15284","version":1},"attestation_state":"computed","paper":{"title":"Light Dark Matter through Resonance Scanning","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Djuna Croon, Gilly Elor, Graham White, Hitoshi Murayama, Rachel Houtz","submitted_at":"2020-12-30T18:58:09Z","abstract_excerpt":"We propose a new out-of-equilibrium production mechanism of light dark matter: resonance scanning. If the dark matter mass evolved in the early Universe, resonant production may have occurred for a wide range of light dark matter masses today. We show that the dark matter relic abundance may be produced through the Higgs portal, in a manner consistent with current experimental constraints."},"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":"2012.15284","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-12-30T18:58:09Z","cross_cats_sorted":[],"title_canon_sha256":"83f6867a5f23a95d5888f4b09586caaa2a291a8d367acc47033b5d14016bdf46","abstract_canon_sha256":"d57ec9f94b26e7a94385f3176910cc2edd9f862087995e3da52460743596668d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:03:16.926499Z","signature_b64":"S5IZZeMrcyRSJrMUpzYKOsEsgRGJvYlS5O4YYGAkIa//1toVzbqq7hL60ArtLr6SmMjfdFz5odZ43DMbmls8CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65401e97315f36c973ba13fa43f089e601f9d16c6f2bbb5573a05672986afc74","last_reissued_at":"2026-07-05T02:03:16.926054Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:03:16.926054Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Light Dark Matter through Resonance Scanning","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Djuna Croon, Gilly Elor, Graham White, Hitoshi Murayama, Rachel Houtz","submitted_at":"2020-12-30T18:58:09Z","abstract_excerpt":"We propose a new out-of-equilibrium production mechanism of light dark matter: resonance scanning. If the dark matter mass evolved in the early Universe, resonant production may have occurred for a wide range of light dark matter masses today. We show that the dark matter relic abundance may be produced through the Higgs portal, in a manner consistent with current experimental constraints."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.15284","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/2012.15284/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":"2012.15284","created_at":"2026-07-05T02:03:16.926112+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.15284v1","created_at":"2026-07-05T02:03:16.926112+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.15284","created_at":"2026-07-05T02:03:16.926112+00:00"},{"alias_kind":"pith_short_12","alias_value":"MVAB5FZRL43M","created_at":"2026-07-05T02:03:16.926112+00:00"},{"alias_kind":"pith_short_16","alias_value":"MVAB5FZRL43MS452","created_at":"2026-07-05T02:03:16.926112+00:00"},{"alias_kind":"pith_short_8","alias_value":"MVAB5FZR","created_at":"2026-07-05T02:03:16.926112+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.07070","citing_title":"Reviving WIMP dark matter with temperature-dependent couplings","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27099","citing_title":"Mesogenesis through the Ephemeral Dark Decay of Beauty","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27099","citing_title":"Mesogenesis through the Ephemeral Dark Decay of Beauty","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y","json":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y.json","graph_json":"https://pith.science/api/pith-number/MVAB5FZRL43MS452CP5EH4EJ4Y/graph.json","events_json":"https://pith.science/api/pith-number/MVAB5FZRL43MS452CP5EH4EJ4Y/events.json","paper":"https://pith.science/paper/MVAB5FZR"},"agent_actions":{"view_html":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y","download_json":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y.json","view_paper":"https://pith.science/paper/MVAB5FZR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.15284&json=true","fetch_graph":"https://pith.science/api/pith-number/MVAB5FZRL43MS452CP5EH4EJ4Y/graph.json","fetch_events":"https://pith.science/api/pith-number/MVAB5FZRL43MS452CP5EH4EJ4Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y/action/storage_attestation","attest_author":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y/action/author_attestation","sign_citation":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y/action/citation_signature","submit_replication":"https://pith.science/pith/MVAB5FZRL43MS452CP5EH4EJ4Y/action/replication_record"}},"created_at":"2026-07-05T02:03:16.926112+00:00","updated_at":"2026-07-05T02:03:16.926112+00:00"}