{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:AYU5VHT2HHNP7RHB24WGK2AWVP","short_pith_number":"pith:AYU5VHT2","schema_version":"1.0","canonical_sha256":"0629da9e7a39daffc4e1d72c656816abe3d3c25371df9698a90579fc25eb1477","source":{"kind":"arxiv","id":"2404.19037","version":2},"attestation_state":"computed","paper":{"title":"BSMPT v3 A Tool for Phase Transitions and Primordial Gravitational Waves in Extended Higgs Sectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Jo\\~ao Viana, Jonas M\\\"uller, Lisa Biermann, Margarete M\\\"uhlleitner, Philipp Basler, Rui Santos","submitted_at":"2024-04-29T18:24:41Z","abstract_excerpt":"Strong first-order phase transitions (SFOPT) during the evolution of the Higgs potential in the early universe not only allow for the dynamical generation of the observed matter-antimatter asymmetry, they can also source a stochastic gravitational wave (GW) background possibly detectable with future space-based GW interferometers. As SFOPTs are phenomenologically incompatible with the Standard Model (SM) Higgs sector, the observation of GWs from SFOPTs provides an exciting interplay between cosmology and particle physics in the search for new physics. With the C++ code BSMPTv3, we present for "},"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":"2404.19037","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-04-29T18:24:41Z","cross_cats_sorted":[],"title_canon_sha256":"676b460079492baaf8503ed641b6da13bed7eafdc9821d41da7ab3d9d862d8bd","abstract_canon_sha256":"8abd6a9845b53c29060664570a926d59897477973119efed0a26b36bda8ab586"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:09:09.699444Z","signature_b64":"h/h7WMCG9kdYCsWg/2daTU1gml7Q3wo4u3uoOEN4UtcbKMwj5CcgUZZsnWUh6OeCPVwzcOBKSqphXsHgtuT8Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0629da9e7a39daffc4e1d72c656816abe3d3c25371df9698a90579fc25eb1477","last_reissued_at":"2026-07-05T12:09:09.698936Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:09:09.698936Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"BSMPT v3 A Tool for Phase Transitions and Primordial Gravitational Waves in Extended Higgs Sectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Jo\\~ao Viana, Jonas M\\\"uller, Lisa Biermann, Margarete M\\\"uhlleitner, Philipp Basler, Rui Santos","submitted_at":"2024-04-29T18:24:41Z","abstract_excerpt":"Strong first-order phase transitions (SFOPT) during the evolution of the Higgs potential in the early universe not only allow for the dynamical generation of the observed matter-antimatter asymmetry, they can also source a stochastic gravitational wave (GW) background possibly detectable with future space-based GW interferometers. As SFOPTs are phenomenologically incompatible with the Standard Model (SM) Higgs sector, the observation of GWs from SFOPTs provides an exciting interplay between cosmology and particle physics in the search for new physics. With the C++ code BSMPTv3, we present for "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.19037","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/2404.19037/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":"2404.19037","created_at":"2026-07-05T12:09:09.698995+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.19037v2","created_at":"2026-07-05T12:09:09.698995+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.19037","created_at":"2026-07-05T12:09:09.698995+00:00"},{"alias_kind":"pith_short_12","alias_value":"AYU5VHT2HHNP","created_at":"2026-07-05T12:09:09.698995+00:00"},{"alias_kind":"pith_short_16","alias_value":"AYU5VHT2HHNP7RHB","created_at":"2026-07-05T12:09:09.698995+00:00"},{"alias_kind":"pith_short_8","alias_value":"AYU5VHT2","created_at":"2026-07-05T12:09:09.698995+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06203","citing_title":"Polyakov Loops Tame Phase Transitions","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04229","citing_title":"A Deep Dive into Baryon Asymmetry -- the C2HDM","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27775","citing_title":"HydroGrav: Precise hydrodynamics and gravitational waves for cosmological phase transitions","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2509.01682","citing_title":"Towards a Unified Framework for Pseudo-Nambu-Goldstone Dark Matter and Electroweak Baryogenesis","ref_index":137,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25557","citing_title":"Jarvis-HEP: A lightweight Python framework for workflow composition and parameter scans in high-energy physics","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14099","citing_title":"Electro-Weak Phase Transitions and Collider Signals in the Aligned 2-Higgs Doublet Model","ref_index":92,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP","json":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP.json","graph_json":"https://pith.science/api/pith-number/AYU5VHT2HHNP7RHB24WGK2AWVP/graph.json","events_json":"https://pith.science/api/pith-number/AYU5VHT2HHNP7RHB24WGK2AWVP/events.json","paper":"https://pith.science/paper/AYU5VHT2"},"agent_actions":{"view_html":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP","download_json":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP.json","view_paper":"https://pith.science/paper/AYU5VHT2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.19037&json=true","fetch_graph":"https://pith.science/api/pith-number/AYU5VHT2HHNP7RHB24WGK2AWVP/graph.json","fetch_events":"https://pith.science/api/pith-number/AYU5VHT2HHNP7RHB24WGK2AWVP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP/action/storage_attestation","attest_author":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP/action/author_attestation","sign_citation":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP/action/citation_signature","submit_replication":"https://pith.science/pith/AYU5VHT2HHNP7RHB24WGK2AWVP/action/replication_record"}},"created_at":"2026-07-05T12:09:09.698995+00:00","updated_at":"2026-07-05T12:09:09.698995+00:00"}