{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:SQJS2MAYM6MGNOQXXBI7LORSGK","short_pith_number":"pith:SQJS2MAY","schema_version":"1.0","canonical_sha256":"94132d3018679866ba17b851f5ba3232907aca5f10c3147098a4ea030aa846aa","source":{"kind":"arxiv","id":"2101.08667","version":2},"attestation_state":"computed","paper":{"title":"Bound states of WIMP dark matter in Higgs-portal models. Part II. Thermal decoupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Kalliopi Petraki, Ruben Oncala","submitted_at":"2021-01-21T15:16:39Z","abstract_excerpt":"The Higgs doublet can mediate a long-range interaction between multi-TeV particles coupled to the Weak interactions of the Standard Model, while its emission can lead to very rapid bound-state formation processes and bound-to-bound transitions. Using the rates calculated in a companion paper, here we compute the thermal decoupling of multi-TeV WIMP dark matter coupled to the Higgs, and show that the formation of metastable dark matter bound states via Higgs-doublet emission and their decay decrease the relic density very significantly. This in turn implies that WIMP dark matter may be much hea"},"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":"2101.08667","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-01-21T15:16:39Z","cross_cats_sorted":[],"title_canon_sha256":"579b6bdefb8dc9a3849036bd5eeb872c224731c964a1b94191f13e32d3125e18","abstract_canon_sha256":"049c85a7f786110e84cf1fea28f52348cdace37170fa9de756d6f1e418a2b078"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:10:51.828343Z","signature_b64":"BEQBJykCGRpFsvObb7SwRUd6/0hPNrg1tUwk32/V12qCRBw8rztE8rBXDI7hB6LYyzce/2Th5pemKtCeITDABA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"94132d3018679866ba17b851f5ba3232907aca5f10c3147098a4ea030aa846aa","last_reissued_at":"2026-07-05T03:10:51.827866Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:10:51.827866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bound states of WIMP dark matter in Higgs-portal models. Part II. Thermal decoupling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Kalliopi Petraki, Ruben Oncala","submitted_at":"2021-01-21T15:16:39Z","abstract_excerpt":"The Higgs doublet can mediate a long-range interaction between multi-TeV particles coupled to the Weak interactions of the Standard Model, while its emission can lead to very rapid bound-state formation processes and bound-to-bound transitions. Using the rates calculated in a companion paper, here we compute the thermal decoupling of multi-TeV WIMP dark matter coupled to the Higgs, and show that the formation of metastable dark matter bound states via Higgs-doublet emission and their decay decrease the relic density very significantly. This in turn implies that WIMP dark matter may be much hea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.08667","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2101.08667/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":"2101.08667","created_at":"2026-07-05T03:10:51.827922+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.08667v2","created_at":"2026-07-05T03:10:51.827922+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.08667","created_at":"2026-07-05T03:10:51.827922+00:00"},{"alias_kind":"pith_short_12","alias_value":"SQJS2MAYM6MG","created_at":"2026-07-05T03:10:51.827922+00:00"},{"alias_kind":"pith_short_16","alias_value":"SQJS2MAYM6MGNOQX","created_at":"2026-07-05T03:10:51.827922+00:00"},{"alias_kind":"pith_short_8","alias_value":"SQJS2MAY","created_at":"2026-07-05T03:10:51.827922+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2511.09306","citing_title":"Self-Interaction of Super-Resonant Dark Matter","ref_index":48,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK","json":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK.json","graph_json":"https://pith.science/api/pith-number/SQJS2MAYM6MGNOQXXBI7LORSGK/graph.json","events_json":"https://pith.science/api/pith-number/SQJS2MAYM6MGNOQXXBI7LORSGK/events.json","paper":"https://pith.science/paper/SQJS2MAY"},"agent_actions":{"view_html":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK","download_json":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK.json","view_paper":"https://pith.science/paper/SQJS2MAY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.08667&json=true","fetch_graph":"https://pith.science/api/pith-number/SQJS2MAYM6MGNOQXXBI7LORSGK/graph.json","fetch_events":"https://pith.science/api/pith-number/SQJS2MAYM6MGNOQXXBI7LORSGK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK/action/storage_attestation","attest_author":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK/action/author_attestation","sign_citation":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK/action/citation_signature","submit_replication":"https://pith.science/pith/SQJS2MAYM6MGNOQXXBI7LORSGK/action/replication_record"}},"created_at":"2026-07-05T03:10:51.827922+00:00","updated_at":"2026-07-05T03:10:51.827922+00:00"}