{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:WDYJAG5GIOX6QH45PUY3K26K7D","short_pith_number":"pith:WDYJAG5G","schema_version":"1.0","canonical_sha256":"b0f0901ba643afe81f9d7d31b56bcaf8c3257e931f9c1fef226b1bf496474018","source":{"kind":"arxiv","id":"gr-qc/0107033","version":1},"attestation_state":"computed","paper":{"title":"Gravitational Waves from Electroweak Phase Transitions","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"gr-qc","authors_text":"Alberto Nicolis, Antonio Riotto, Michele Maggiore, Riccardo Apreda","submitted_at":"2001-07-10T15:34:45Z","abstract_excerpt":"Gravitational waves are generated during first-order phase transitions, either by turbolence or by bubble collisions. If the transition takes place at temperatures of the order of the electroweak scale, the frequency of these gravitational waves is today just within the band of the planned space interferometer LISA. We present a detailed analysis of the production of gravitational waves during an electroweak phase transition in different supersymmetric models where, contrary to the case of the Standard Model, the transition can be first order. We find that the stochastic background of gravitat"},"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":"gr-qc/0107033","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2001-07-10T15:34:45Z","cross_cats_sorted":["astro-ph","hep-ph"],"title_canon_sha256":"18d2f481b806f9e13a0698142bde8a2cbfde71694595efdcf60fca95427b05b2","abstract_canon_sha256":"3b519e72a72cbb427676144ed8fcd5fee061b05c0d9af114c4999831bd6ad6fb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:26:55.660976Z","signature_b64":"X3U2+T/CAL4nyegRh4t+NQghu2G5q463wiHf9FdNIq17WTla2bBeuQ8oWSns/UErcKKGXb6sLAH7hhcCWIklBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b0f0901ba643afe81f9d7d31b56bcaf8c3257e931f9c1fef226b1bf496474018","last_reissued_at":"2026-07-04T16:26:55.660583Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:26:55.660583Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Waves from Electroweak Phase Transitions","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"gr-qc","authors_text":"Alberto Nicolis, Antonio Riotto, Michele Maggiore, Riccardo Apreda","submitted_at":"2001-07-10T15:34:45Z","abstract_excerpt":"Gravitational waves are generated during first-order phase transitions, either by turbolence or by bubble collisions. If the transition takes place at temperatures of the order of the electroweak scale, the frequency of these gravitational waves is today just within the band of the planned space interferometer LISA. We present a detailed analysis of the production of gravitational waves during an electroweak phase transition in different supersymmetric models where, contrary to the case of the Standard Model, the transition can be first order. We find that the stochastic background of gravitat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0107033","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/gr-qc/0107033/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":"gr-qc/0107033","created_at":"2026-07-04T16:26:55.660635+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0107033v1","created_at":"2026-07-04T16:26:55.660635+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0107033","created_at":"2026-07-04T16:26:55.660635+00:00"},{"alias_kind":"pith_short_12","alias_value":"WDYJAG5GIOX6","created_at":"2026-07-04T16:26:55.660635+00:00"},{"alias_kind":"pith_short_16","alias_value":"WDYJAG5GIOX6QH45","created_at":"2026-07-04T16:26:55.660635+00:00"},{"alias_kind":"pith_short_8","alias_value":"WDYJAG5G","created_at":"2026-07-04T16:26:55.660635+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2606.13514","citing_title":"Electroweak First-Order Phase Transition Triggered by Non-Gaussian Fluctuations of a $\\mathbb{Z}_2$-Symmetric Spectator Scalar","ref_index":117,"is_internal_anchor":true},{"citing_arxiv_id":"2606.13597","citing_title":"Natural Supercooling and Reheating along Supersymmetric Flat Directions and Observable Gravitational Waves at the Einstein Telescope and the Cosmic Explorer","ref_index":122,"is_internal_anchor":true},{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":133,"is_internal_anchor":true},{"citing_arxiv_id":"2410.23348","citing_title":"Observable CMB B-modes from Cosmological Phase Transitions","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D","json":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D.json","graph_json":"https://pith.science/api/pith-number/WDYJAG5GIOX6QH45PUY3K26K7D/graph.json","events_json":"https://pith.science/api/pith-number/WDYJAG5GIOX6QH45PUY3K26K7D/events.json","paper":"https://pith.science/paper/WDYJAG5G"},"agent_actions":{"view_html":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D","download_json":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D.json","view_paper":"https://pith.science/paper/WDYJAG5G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0107033&json=true","fetch_graph":"https://pith.science/api/pith-number/WDYJAG5GIOX6QH45PUY3K26K7D/graph.json","fetch_events":"https://pith.science/api/pith-number/WDYJAG5GIOX6QH45PUY3K26K7D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D/action/storage_attestation","attest_author":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D/action/author_attestation","sign_citation":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D/action/citation_signature","submit_replication":"https://pith.science/pith/WDYJAG5GIOX6QH45PUY3K26K7D/action/replication_record"}},"created_at":"2026-07-04T16:26:55.660635+00:00","updated_at":"2026-07-04T16:26:55.660635+00:00"}