{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:5CVYXTTWVXQ646QUCUMUAY3AEV","short_pith_number":"pith:5CVYXTTW","schema_version":"1.0","canonical_sha256":"e8ab8bce76ade1ee7a141519406360255a7721c11f216e763cb8e041ba884e2b","source":{"kind":"arxiv","id":"1009.4593","version":1},"attestation_state":"computed","paper":{"title":"Evolution of Universe to the present inert phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Sokolowska, I. F. Ginzburg, K.A. Kanishev, M. Krawczyk","submitted_at":"2010-09-23T12:35:01Z","abstract_excerpt":"We assume that current state of the Universe can be described by the Inert Doublet Model, containing two scalar doublets, one of which is responsible for EWSB and masses of particles and the second one having no couplings to fermions and being responsible for dark matter. We consider possible evolutions of the Universe to this state during cooling down of the Universe after inflation. We found that in the past Universe could pass through phase states having no DM candidate. In the evolution via such states in addition to a possible EWSB phase transition (2-nd order) the Universe sustained one "},"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":"1009.4593","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-09-23T12:35:01Z","cross_cats_sorted":[],"title_canon_sha256":"05fcc4f4cc5a078e9d22d3e1096f9fecb9857ffb147afd51fb9b811972e3f311","abstract_canon_sha256":"c875e7556b18189cf5f1879753d6a976548d2669da9e6693d5584c6f0da70ad4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:30:13.879834Z","signature_b64":"6Zval5ZBUJHVPVborYy/qB8b6zTC2cV3y4NtvluetEE+4Pfh4K6lxCNHgCD2jJx6MtF+Y4jumHfE+xK46qEfAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e8ab8bce76ade1ee7a141519406360255a7721c11f216e763cb8e041ba884e2b","last_reissued_at":"2026-05-18T04:30:13.879282Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:30:13.879282Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolution of Universe to the present inert phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Sokolowska, I. F. Ginzburg, K.A. Kanishev, M. Krawczyk","submitted_at":"2010-09-23T12:35:01Z","abstract_excerpt":"We assume that current state of the Universe can be described by the Inert Doublet Model, containing two scalar doublets, one of which is responsible for EWSB and masses of particles and the second one having no couplings to fermions and being responsible for dark matter. We consider possible evolutions of the Universe to this state during cooling down of the Universe after inflation. We found that in the past Universe could pass through phase states having no DM candidate. In the evolution via such states in addition to a possible EWSB phase transition (2-nd order) the Universe sustained one "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.4593","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":""},"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":"1009.4593","created_at":"2026-05-18T04:30:13.879366+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.4593v1","created_at":"2026-05-18T04:30:13.879366+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.4593","created_at":"2026-05-18T04:30:13.879366+00:00"},{"alias_kind":"pith_short_12","alias_value":"5CVYXTTWVXQ6","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"5CVYXTTWVXQ646QU","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"5CVYXTTW","created_at":"2026-05-18T12:26:04.259169+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.13614","citing_title":"Search for pair production of additional neutral scalars within the Inert Doublet Model in a final state with two electrons or two muons in proton-proton collisions at $\\sqrt{s}$ = 13 TeV and 13.6 TeV","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2605.07616","citing_title":"Probing the Inert Doublet Dark Matter with Stellar-Mass Black Hole Mini-Spikes","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV","json":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV.json","graph_json":"https://pith.science/api/pith-number/5CVYXTTWVXQ646QUCUMUAY3AEV/graph.json","events_json":"https://pith.science/api/pith-number/5CVYXTTWVXQ646QUCUMUAY3AEV/events.json","paper":"https://pith.science/paper/5CVYXTTW"},"agent_actions":{"view_html":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV","download_json":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV.json","view_paper":"https://pith.science/paper/5CVYXTTW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.4593&json=true","fetch_graph":"https://pith.science/api/pith-number/5CVYXTTWVXQ646QUCUMUAY3AEV/graph.json","fetch_events":"https://pith.science/api/pith-number/5CVYXTTWVXQ646QUCUMUAY3AEV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV/action/storage_attestation","attest_author":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV/action/author_attestation","sign_citation":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV/action/citation_signature","submit_replication":"https://pith.science/pith/5CVYXTTWVXQ646QUCUMUAY3AEV/action/replication_record"}},"created_at":"2026-05-18T04:30:13.879366+00:00","updated_at":"2026-05-18T04:30:13.879366+00:00"}