{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FORT7CC7R4G2TDAWTB4TKPRGIT","short_pith_number":"pith:FORT7CC7","schema_version":"1.0","canonical_sha256":"2ba33f885f8f0da98c169879353e2644ee2d80c02af113d3781966babab33a5f","source":{"kind":"arxiv","id":"1803.01038","version":2},"attestation_state":"computed","paper":{"title":"Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Ken'ichi Saikawa, Satoshi Shirai","submitted_at":"2018-03-02T20:44:13Z","abstract_excerpt":"In this paper, we revisit the estimation of the spectrum of primordial gravitational waves originated from inflation, particularly focusing on the effect of thermodynamics in the Standard Model of particle physics. By collecting recent results of perturbative and non-perturbative analysis of thermodynamic quantities in the Standard Model, we obtain the effective degrees of freedom including the corrections due to non-trivial interaction properties of particles in the Standard Model for a wide temperature interval. The impact of such corrections on the spectrum of primordial gravitational waves"},"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":"1803.01038","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-03-02T20:44:13Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"ae3baf2b63b12117a30919534e23821aaf5dd074d716b01ed897d97ab0c2f500","abstract_canon_sha256":"2cfe19d76296841679cf8e0a154ecb0b83faefdc3ad73ec45a6acbd5b904dbc8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:15:46.538359Z","signature_b64":"STb1bkXp30AB+7iSi5KNjtEbOBNdgdAXT2O58eNMdw0LfSIG4AeNW142lq6USfKd/y/3xcM1jNS0O3L9GHIHBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2ba33f885f8f0da98c169879353e2644ee2d80c02af113d3781966babab33a5f","last_reissued_at":"2026-05-18T00:15:46.537568Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:15:46.537568Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Primordial gravitational waves, precisely: The role of thermodynamics in the Standard Model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Ken'ichi Saikawa, Satoshi Shirai","submitted_at":"2018-03-02T20:44:13Z","abstract_excerpt":"In this paper, we revisit the estimation of the spectrum of primordial gravitational waves originated from inflation, particularly focusing on the effect of thermodynamics in the Standard Model of particle physics. By collecting recent results of perturbative and non-perturbative analysis of thermodynamic quantities in the Standard Model, we obtain the effective degrees of freedom including the corrections due to non-trivial interaction properties of particles in the Standard Model for a wide temperature interval. The impact of such corrections on the spectrum of primordial gravitational waves"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.01038","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":"1803.01038","created_at":"2026-05-18T00:15:46.537691+00:00"},{"alias_kind":"arxiv_version","alias_value":"1803.01038v2","created_at":"2026-05-18T00:15:46.537691+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.01038","created_at":"2026-05-18T00:15:46.537691+00:00"},{"alias_kind":"pith_short_12","alias_value":"FORT7CC7R4G2","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"FORT7CC7R4G2TDAW","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"FORT7CC7","created_at":"2026-05-18T12:32:25.280505+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":13,"internal_anchor_count":8,"sample":[{"citing_arxiv_id":"1907.04473","citing_title":"CMB-S4 Science Case, Reference Design, and Project Plan","ref_index":222,"is_internal_anchor":true},{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":162,"is_internal_anchor":true},{"citing_arxiv_id":"2505.16820","citing_title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","ref_index":156,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15259","citing_title":"TransitionListener v2.0 -- Robust gravitational wave predictions for cosmological phase transitions","ref_index":146,"is_internal_anchor":true},{"citing_arxiv_id":"2507.09552","citing_title":"Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2508.00798","citing_title":"Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation","ref_index":96,"is_internal_anchor":true},{"citing_arxiv_id":"2511.02184","citing_title":"Dark Matter Freeze-in from a $Z^\\prime$ Reheaton","ref_index":74,"is_internal_anchor":true},{"citing_arxiv_id":"2109.01398","citing_title":"Scalar induced gravitational waves review","ref_index":295,"is_internal_anchor":true},{"citing_arxiv_id":"2605.04487","citing_title":"Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01992","citing_title":"Reviving Motivated Inflationary Potentials with $K$-inflation in the light of ACT","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20792","citing_title":"Irreducible Gravitational Wave Background as a Particle Detector","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05078","citing_title":"Gravitational Waves from Matter Perturbations of Spectator Scalar Fields","ref_index":97,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17478","citing_title":"A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating","ref_index":50,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT","json":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT.json","graph_json":"https://pith.science/api/pith-number/FORT7CC7R4G2TDAWTB4TKPRGIT/graph.json","events_json":"https://pith.science/api/pith-number/FORT7CC7R4G2TDAWTB4TKPRGIT/events.json","paper":"https://pith.science/paper/FORT7CC7"},"agent_actions":{"view_html":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT","download_json":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT.json","view_paper":"https://pith.science/paper/FORT7CC7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1803.01038&json=true","fetch_graph":"https://pith.science/api/pith-number/FORT7CC7R4G2TDAWTB4TKPRGIT/graph.json","fetch_events":"https://pith.science/api/pith-number/FORT7CC7R4G2TDAWTB4TKPRGIT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT/action/storage_attestation","attest_author":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT/action/author_attestation","sign_citation":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT/action/citation_signature","submit_replication":"https://pith.science/pith/FORT7CC7R4G2TDAWTB4TKPRGIT/action/replication_record"}},"created_at":"2026-05-18T00:15:46.537691+00:00","updated_at":"2026-05-18T00:15:46.537691+00:00"}