{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:LU6HVP67B4PZWEI225Z4UPXLDN","short_pith_number":"pith:LU6HVP67","schema_version":"1.0","canonical_sha256":"5d3c7abfdf0f1f9b111ad773ca3eeb1b65ed757597838bd0f43983951de59ff2","source":{"kind":"arxiv","id":"2103.06933","version":2},"attestation_state":"computed","paper":{"title":"The Benefits of Diligence: How Precise are Predicted Gravitational Wave Spectra in Models with Phase Transitions?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Daniel Vagie, Graham White, Huai-Ke Guo, Kuver Sinha","submitted_at":"2021-03-11T20:07:36Z","abstract_excerpt":"Models of particle physics that feature phase transitions typically provide predictions for stochastic gravitational wave signals at future detectors and such predictions are used to delineate portions of the model parameter space that can be constrained. The question is: how precise are such predictions? Uncertainties enter in the calculation of the macroscopic thermal parameters and the dynamics of the phase transition itself. We calculate such uncertainties with increasing levels of sophistication in treating the phase transition dynamics. Currently, the highest level of diligence correspon"},"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":"2103.06933","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-03-11T20:07:36Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"909782a00a009bde25f9abc61ab2c785281f7d8ed310b33b3cac79a44a515523","abstract_canon_sha256":"294fa29ab9d1a9bc71b96088a6583f06c62a6ed1f67320bc3d58143bd9f5e29e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:56:57.299551Z","signature_b64":"aNf+xa7eGsyzu4gvVAKwXcA+qDkDOoJU62+I63Xwz0RheiOtrBOTs4UX1Bxfc/MRSWtacj8YzIQVtdTOOfXXAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d3c7abfdf0f1f9b111ad773ca3eeb1b65ed757597838bd0f43983951de59ff2","last_reissued_at":"2026-07-05T02:56:57.299095Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:56:57.299095Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Benefits of Diligence: How Precise are Predicted Gravitational Wave Spectra in Models with Phase Transitions?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Daniel Vagie, Graham White, Huai-Ke Guo, Kuver Sinha","submitted_at":"2021-03-11T20:07:36Z","abstract_excerpt":"Models of particle physics that feature phase transitions typically provide predictions for stochastic gravitational wave signals at future detectors and such predictions are used to delineate portions of the model parameter space that can be constrained. The question is: how precise are such predictions? Uncertainties enter in the calculation of the macroscopic thermal parameters and the dynamics of the phase transition itself. We calculate such uncertainties with increasing levels of sophistication in treating the phase transition dynamics. Currently, the highest level of diligence correspon"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.06933","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/2103.06933/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":"2103.06933","created_at":"2026-07-05T02:56:57.299152+00:00"},{"alias_kind":"arxiv_version","alias_value":"2103.06933v2","created_at":"2026-07-05T02:56:57.299152+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2103.06933","created_at":"2026-07-05T02:56:57.299152+00:00"},{"alias_kind":"pith_short_12","alias_value":"LU6HVP67B4PZ","created_at":"2026-07-05T02:56:57.299152+00:00"},{"alias_kind":"pith_short_16","alias_value":"LU6HVP67B4PZWEI2","created_at":"2026-07-05T02:56:57.299152+00:00"},{"alias_kind":"pith_short_8","alias_value":"LU6HVP67","created_at":"2026-07-05T02:56:57.299152+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2408.03649","citing_title":"Probing radiative electroweak symmetry breaking with colliders and gravitational waves","ref_index":105,"is_internal_anchor":false},{"citing_arxiv_id":"2511.00996","citing_title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","ref_index":68,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN","json":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN.json","graph_json":"https://pith.science/api/pith-number/LU6HVP67B4PZWEI225Z4UPXLDN/graph.json","events_json":"https://pith.science/api/pith-number/LU6HVP67B4PZWEI225Z4UPXLDN/events.json","paper":"https://pith.science/paper/LU6HVP67"},"agent_actions":{"view_html":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN","download_json":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN.json","view_paper":"https://pith.science/paper/LU6HVP67","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2103.06933&json=true","fetch_graph":"https://pith.science/api/pith-number/LU6HVP67B4PZWEI225Z4UPXLDN/graph.json","fetch_events":"https://pith.science/api/pith-number/LU6HVP67B4PZWEI225Z4UPXLDN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN/action/storage_attestation","attest_author":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN/action/author_attestation","sign_citation":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN/action/citation_signature","submit_replication":"https://pith.science/pith/LU6HVP67B4PZWEI225Z4UPXLDN/action/replication_record"}},"created_at":"2026-07-05T02:56:57.299152+00:00","updated_at":"2026-07-05T02:56:57.299152+00:00"}