{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:CFY7GQKXJFTZGJDNQKU2BW3OMX","short_pith_number":"pith:CFY7GQKX","schema_version":"1.0","canonical_sha256":"1171f34157496793246d82a9a0db6e65d456d256e01096773670f5e5a08e9f61","source":{"kind":"arxiv","id":"1503.04935","version":2},"attestation_state":"computed","paper":{"title":"Standard Model thermodynamics across the electroweak crossover","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat"],"primary_cat":"hep-ph","authors_text":"M. Laine, M. Meyer","submitted_at":"2015-03-17T06:37:44Z","abstract_excerpt":"Even though the Standard Model with a Higgs mass mH = 125 GeV possesses no bulk phase transition, its thermodynamics still experiences a \"soft point\" at temperatures around T = 160 GeV, with a deviation from ideal gas thermodynamics. Such a deviation may have an effect on precision computations of weakly interacting dark matter relic abundances if their mass is in the few TeV range, or on leptogenesis scenarios operating in this temperature range. By making use of results from lattice simulations based on a dimensionally reduced effective field theory, we estimate the relevant thermodynamic fu"},"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":"1503.04935","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-03-17T06:37:44Z","cross_cats_sorted":["hep-lat"],"title_canon_sha256":"2fedd46f578aa2d9973b3edf46b84d8b6c4483a41a2734ba7e945a0eb36d8e9d","abstract_canon_sha256":"b1dc0609c58b1bcd8887151b1c52a3d21d5d82b433069ea92d43f4a93c925ca6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:48.878348Z","signature_b64":"bN25xCCYu3NWGol8fuzLNTELc9oAIzCTn9LRT/n1RY/oMel0b5/B1Z42HKetY57/IID8lwKk3bWR0DCDAFWODg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1171f34157496793246d82a9a0db6e65d456d256e01096773670f5e5a08e9f61","last_reissued_at":"2026-05-18T01:35:48.877619Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:48.877619Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Standard Model thermodynamics across the electroweak crossover","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat"],"primary_cat":"hep-ph","authors_text":"M. Laine, M. Meyer","submitted_at":"2015-03-17T06:37:44Z","abstract_excerpt":"Even though the Standard Model with a Higgs mass mH = 125 GeV possesses no bulk phase transition, its thermodynamics still experiences a \"soft point\" at temperatures around T = 160 GeV, with a deviation from ideal gas thermodynamics. Such a deviation may have an effect on precision computations of weakly interacting dark matter relic abundances if their mass is in the few TeV range, or on leptogenesis scenarios operating in this temperature range. By making use of results from lattice simulations based on a dimensionally reduced effective field theory, we estimate the relevant thermodynamic fu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.04935","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":"1503.04935","created_at":"2026-05-18T01:35:48.877729+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.04935v2","created_at":"2026-05-18T01:35:48.877729+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.04935","created_at":"2026-05-18T01:35:48.877729+00:00"},{"alias_kind":"pith_short_12","alias_value":"CFY7GQKXJFTZ","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_16","alias_value":"CFY7GQKXJFTZGJDN","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_8","alias_value":"CFY7GQKX","created_at":"2026-05-18T12:29:14.074870+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2508.14535","citing_title":"Axion Star Bosenova in Axion Miniclusters","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2511.00157","citing_title":"Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look","ref_index":81,"is_internal_anchor":true},{"citing_arxiv_id":"2511.07511","citing_title":"Seasons of Dark Matter Freeze-In Shaped by the Weather of the Early Universe","ref_index":71,"is_internal_anchor":true},{"citing_arxiv_id":"2604.20768","citing_title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX","json":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX.json","graph_json":"https://pith.science/api/pith-number/CFY7GQKXJFTZGJDNQKU2BW3OMX/graph.json","events_json":"https://pith.science/api/pith-number/CFY7GQKXJFTZGJDNQKU2BW3OMX/events.json","paper":"https://pith.science/paper/CFY7GQKX"},"agent_actions":{"view_html":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX","download_json":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX.json","view_paper":"https://pith.science/paper/CFY7GQKX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.04935&json=true","fetch_graph":"https://pith.science/api/pith-number/CFY7GQKXJFTZGJDNQKU2BW3OMX/graph.json","fetch_events":"https://pith.science/api/pith-number/CFY7GQKXJFTZGJDNQKU2BW3OMX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX/action/storage_attestation","attest_author":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX/action/author_attestation","sign_citation":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX/action/citation_signature","submit_replication":"https://pith.science/pith/CFY7GQKXJFTZGJDNQKU2BW3OMX/action/replication_record"}},"created_at":"2026-05-18T01:35:48.877729+00:00","updated_at":"2026-05-18T01:35:48.877729+00:00"}