{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:DKVYU33X5VU6FFFF5M6EGIZNVI","short_pith_number":"pith:DKVYU33X","schema_version":"1.0","canonical_sha256":"1aab8a6f77ed69e294a5eb3c43232daa3bd205d8bcaacac523920f8ea07cdd65","source":{"kind":"arxiv","id":"2010.02590","version":3},"attestation_state":"computed","paper":{"title":"Bubble wall velocity: heavy physics effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aleksandr Azatov, Miguel Vanvlasselaer","submitted_at":"2020-10-06T10:00:44Z","abstract_excerpt":"We analyse the dynamics of the relativistic bubble expansion during the first order phase transition focusing on the ultra relativistic velocities $\\gamma\\gg 1$. We show that fields much heavier than the scale of the phase transition can significantly contribute to the friction and modify the motion of the bubble wall leading to interesting phenomenological consequences. NLO effects on the friction due to the soft vector field emission are reviewed as well."},"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":"2010.02590","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-10-06T10:00:44Z","cross_cats_sorted":[],"title_canon_sha256":"9c0f9b866b217167e894f3e98fd3df930e18a4b255c8f0edde845649f5f14f2c","abstract_canon_sha256":"595ea025941770bc92e7e3ecc57793e9c641fa5201b5e38b4928f2c8e9c7ba39"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:12:06.972507Z","signature_b64":"7BB93Bi6Kz9um16QznXDu4R1Tc/I9TdK08nIp/Zj6rMx0mSWFKv1VXdySgZU32UvGTblYoxXYcQ/4PnkveCZAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1aab8a6f77ed69e294a5eb3c43232daa3bd205d8bcaacac523920f8ea07cdd65","last_reissued_at":"2026-07-05T02:12:06.972068Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:12:06.972068Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bubble wall velocity: heavy physics effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aleksandr Azatov, Miguel Vanvlasselaer","submitted_at":"2020-10-06T10:00:44Z","abstract_excerpt":"We analyse the dynamics of the relativistic bubble expansion during the first order phase transition focusing on the ultra relativistic velocities $\\gamma\\gg 1$. We show that fields much heavier than the scale of the phase transition can significantly contribute to the friction and modify the motion of the bubble wall leading to interesting phenomenological consequences. NLO effects on the friction due to the soft vector field emission are reviewed as well."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.02590","kind":"arxiv","version":3},"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/2010.02590/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":"2010.02590","created_at":"2026-07-05T02:12:06.972127+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.02590v3","created_at":"2026-07-05T02:12:06.972127+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.02590","created_at":"2026-07-05T02:12:06.972127+00:00"},{"alias_kind":"pith_short_12","alias_value":"DKVYU33X5VU6","created_at":"2026-07-05T02:12:06.972127+00:00"},{"alias_kind":"pith_short_16","alias_value":"DKVYU33X5VU6FFFF","created_at":"2026-07-05T02:12:06.972127+00:00"},{"alias_kind":"pith_short_8","alias_value":"DKVYU33X","created_at":"2026-07-05T02:12:06.972127+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30740","citing_title":"Dynamical evolution of the pressure on the bubble wall","ref_index":86,"is_internal_anchor":false},{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":178,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11203","citing_title":"Bounds from D/H on baryogenesis models","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI","json":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI.json","graph_json":"https://pith.science/api/pith-number/DKVYU33X5VU6FFFF5M6EGIZNVI/graph.json","events_json":"https://pith.science/api/pith-number/DKVYU33X5VU6FFFF5M6EGIZNVI/events.json","paper":"https://pith.science/paper/DKVYU33X"},"agent_actions":{"view_html":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI","download_json":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI.json","view_paper":"https://pith.science/paper/DKVYU33X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.02590&json=true","fetch_graph":"https://pith.science/api/pith-number/DKVYU33X5VU6FFFF5M6EGIZNVI/graph.json","fetch_events":"https://pith.science/api/pith-number/DKVYU33X5VU6FFFF5M6EGIZNVI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI/action/storage_attestation","attest_author":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI/action/author_attestation","sign_citation":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI/action/citation_signature","submit_replication":"https://pith.science/pith/DKVYU33X5VU6FFFF5M6EGIZNVI/action/replication_record"}},"created_at":"2026-07-05T02:12:06.972127+00:00","updated_at":"2026-07-05T02:12:06.972127+00:00"}