{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:MBNVKEYHDLEDCPGU3TJCMIXECL","short_pith_number":"pith:MBNVKEYH","schema_version":"1.0","canonical_sha256":"605b5513071ac8313cd4dcd22622e412fe6882c60092a24aa86578cf8366cd19","source":{"kind":"arxiv","id":"1302.1044","version":1},"attestation_state":"computed","paper":{"title":"An efficient approach to electroweak bubble velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Miguel Sopena, Stephan J. Huber","submitted_at":"2013-02-05T14:32:27Z","abstract_excerpt":"Extensions of the Standard Model are being considered as viable settings for a first-order electroweak phase transition which satisfy Sakharov's three conditions for the generation of the baryon asymmetry of the Universe. These extensions provide a sufficiently strong phase transition and remove the main obstacles which appear in the context of the Standard Model: A far-too-high lower bound on the Higgs mass, immediate wipeout of the newly-created baryon asymmetry, and insufficient CP violation. We describe the Universe hydrodynamically as a fluid coupled to the Higgs field via a phenomenologi"},"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":"1302.1044","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-02-05T14:32:27Z","cross_cats_sorted":[],"title_canon_sha256":"0eae4d63e53a1c4a0c2c007baafc229eed331ec03d0f30002eb421d50fd8cc2a","abstract_canon_sha256":"e1e34a29c262f9328e4251a5aa1ff5e68e5e73fa7c462a26c69597f5e7b91b22"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:34:26.333096Z","signature_b64":"nuURb5vERZKqGs1VJxbOcjIH5iYpI86Wo/XU6mv3sR4anqc9bcwtqpqABUDHbLk27FxUGo4CqW6q0VrmVSR2Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"605b5513071ac8313cd4dcd22622e412fe6882c60092a24aa86578cf8366cd19","last_reissued_at":"2026-05-18T03:34:26.332489Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:34:26.332489Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An efficient approach to electroweak bubble velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Miguel Sopena, Stephan J. Huber","submitted_at":"2013-02-05T14:32:27Z","abstract_excerpt":"Extensions of the Standard Model are being considered as viable settings for a first-order electroweak phase transition which satisfy Sakharov's three conditions for the generation of the baryon asymmetry of the Universe. These extensions provide a sufficiently strong phase transition and remove the main obstacles which appear in the context of the Standard Model: A far-too-high lower bound on the Higgs mass, immediate wipeout of the newly-created baryon asymmetry, and insufficient CP violation. We describe the Universe hydrodynamically as a fluid coupled to the Higgs field via a phenomenologi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.1044","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":""},"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":"1302.1044","created_at":"2026-05-18T03:34:26.332576+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.1044v1","created_at":"2026-05-18T03:34:26.332576+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.1044","created_at":"2026-05-18T03:34:26.332576+00:00"},{"alias_kind":"pith_short_12","alias_value":"MBNVKEYHDLED","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"MBNVKEYHDLEDCPGU","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"MBNVKEYH","created_at":"2026-05-18T12:27:51.066281+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":166,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL","json":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL.json","graph_json":"https://pith.science/api/pith-number/MBNVKEYHDLEDCPGU3TJCMIXECL/graph.json","events_json":"https://pith.science/api/pith-number/MBNVKEYHDLEDCPGU3TJCMIXECL/events.json","paper":"https://pith.science/paper/MBNVKEYH"},"agent_actions":{"view_html":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL","download_json":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL.json","view_paper":"https://pith.science/paper/MBNVKEYH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.1044&json=true","fetch_graph":"https://pith.science/api/pith-number/MBNVKEYHDLEDCPGU3TJCMIXECL/graph.json","fetch_events":"https://pith.science/api/pith-number/MBNVKEYHDLEDCPGU3TJCMIXECL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL/action/storage_attestation","attest_author":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL/action/author_attestation","sign_citation":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL/action/citation_signature","submit_replication":"https://pith.science/pith/MBNVKEYHDLEDCPGU3TJCMIXECL/action/replication_record"}},"created_at":"2026-05-18T03:34:26.332576+00:00","updated_at":"2026-05-18T03:34:26.332576+00:00"}