{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:6K6XK66J3PLMJS3TV5OZ3UNN76","short_pith_number":"pith:6K6XK66J","schema_version":"1.0","canonical_sha256":"f2bd757bc9dbd6c4cb73af5d9dd1adff92e56408ef5c30a9b63cd9d348db818f","source":{"kind":"arxiv","id":"1903.11604","version":1},"attestation_state":"computed","paper":{"title":"Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-lat","hep-th"],"primary_cat":"hep-ph","authors_text":"David J. Weir, Jonathan Kozaczuk, Lauri Niemi, Michael J. Ramsey-Musolf, Oliver Gould, Tuomas V. I. Tenkanen","submitted_at":"2019-03-27T18:00:00Z","abstract_excerpt":"We present the first end-to-end nonperturbative analysis of the gravitational wave power spectrum from a thermal first-order electroweak phase transition (EWPT), using the framework of dimensionally reduced effective field theory and pre-existing nonperturbative simulation results. We are able to show that a first-order EWPT in any beyond the Standard Model (BSM) scenario that can be described by a Standard Model-like effective theory at long distances will produce gravitational wave signatures too weak to be observed at existing and planned detectors. This implies that colliders are likely to"},"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":"1903.11604","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-03-27T18:00:00Z","cross_cats_sorted":["astro-ph.CO","hep-lat","hep-th"],"title_canon_sha256":"f96549bd29241be1914221376b6246c30e112d6047fd8a5c54a4b27c889c1fdf","abstract_canon_sha256":"c2fc0f93d78b07639992e001601d926b10db048afe63cd803619d9fb2c89e6bc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:26:34.063693Z","signature_b64":"xFSlvVt3prJnHVPs0OPzzaFcANupzImSzlchn2OeCsVE6W9+ns1Fjj/NYM8PJAq31Nb7cRd70tRAvjhxHSz4Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f2bd757bc9dbd6c4cb73af5d9dd1adff92e56408ef5c30a9b63cd9d348db818f","last_reissued_at":"2026-07-05T00:26:34.063281Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:26:34.063281Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-lat","hep-th"],"primary_cat":"hep-ph","authors_text":"David J. Weir, Jonathan Kozaczuk, Lauri Niemi, Michael J. Ramsey-Musolf, Oliver Gould, Tuomas V. I. Tenkanen","submitted_at":"2019-03-27T18:00:00Z","abstract_excerpt":"We present the first end-to-end nonperturbative analysis of the gravitational wave power spectrum from a thermal first-order electroweak phase transition (EWPT), using the framework of dimensionally reduced effective field theory and pre-existing nonperturbative simulation results. We are able to show that a first-order EWPT in any beyond the Standard Model (BSM) scenario that can be described by a Standard Model-like effective theory at long distances will produce gravitational wave signatures too weak to be observed at existing and planned detectors. This implies that colliders are likely to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.11604","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/1903.11604/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":"1903.11604","created_at":"2026-07-05T00:26:34.063343+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.11604v1","created_at":"2026-07-05T00:26:34.063343+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.11604","created_at":"2026-07-05T00:26:34.063343+00:00"},{"alias_kind":"pith_short_12","alias_value":"6K6XK66J3PLM","created_at":"2026-07-05T00:26:34.063343+00:00"},{"alias_kind":"pith_short_16","alias_value":"6K6XK66J3PLMJS3T","created_at":"2026-07-05T00:26:34.063343+00:00"},{"alias_kind":"pith_short_8","alias_value":"6K6XK66J","created_at":"2026-07-05T00:26:34.063343+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06203","citing_title":"Polyakov Loops Tame Phase Transitions","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2606.12533","citing_title":"Constraining the real scalar singlet extension of the SM","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2607.02505","citing_title":"A critical look at low-scale cosmological phase transitions in the PTA era","ref_index":150,"is_internal_anchor":false},{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":91,"is_internal_anchor":false},{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":150,"is_internal_anchor":false},{"citing_arxiv_id":"2602.18286","citing_title":"On self-dualities for scalar $\\phi^4$ theory","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03007","citing_title":"Post-Recombination Fluctuations from a Sequestered Dark Sector","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21972","citing_title":"Matchotter: An Automated Tool for Dimensional Reduction at Finite Temperature","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06775","citing_title":"SIRENA -- Sum-Integral REductioN Algorithm","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76","json":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76.json","graph_json":"https://pith.science/api/pith-number/6K6XK66J3PLMJS3TV5OZ3UNN76/graph.json","events_json":"https://pith.science/api/pith-number/6K6XK66J3PLMJS3TV5OZ3UNN76/events.json","paper":"https://pith.science/paper/6K6XK66J"},"agent_actions":{"view_html":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76","download_json":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76.json","view_paper":"https://pith.science/paper/6K6XK66J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.11604&json=true","fetch_graph":"https://pith.science/api/pith-number/6K6XK66J3PLMJS3TV5OZ3UNN76/graph.json","fetch_events":"https://pith.science/api/pith-number/6K6XK66J3PLMJS3TV5OZ3UNN76/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76/action/storage_attestation","attest_author":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76/action/author_attestation","sign_citation":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76/action/citation_signature","submit_replication":"https://pith.science/pith/6K6XK66J3PLMJS3TV5OZ3UNN76/action/replication_record"}},"created_at":"2026-07-05T00:26:34.063343+00:00","updated_at":"2026-07-05T00:26:34.063343+00:00"}