{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1995:BBFMFQY2VXYPWOBX76I3EC4JRI","short_pith_number":"pith:BBFMFQY2","schema_version":"1.0","canonical_sha256":"084ac2c31aadf0fb3837ff91b20b898a09d6c4f6a9d3556c40bcff7bf76914cd","source":{"kind":"arxiv","id":"hep-ph/9507381","version":1},"attestation_state":"computed","paper":{"title":"Gauge independence of the bubble nucleation rate in theories with radiative symmetry breaking","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Dimitrios Metaxas, Erick J. Weinberg (Columbia University)","submitted_at":"1995-07-21T16:11:11Z","abstract_excerpt":"In field theories where a metastable false vacuum state arises as a result of radiative corrections, the calculation of the rate of false vacuum decay by bubble nucleation depends on the effective potential and the other functions that appear in the derivative expansion of the effective action. Beginning with the Nielsen identity, we derive a series of identities that govern the gauge dependence of these functions. Using these, we show, to leading nontrivial order, that even though these functions are individually gauge-dependent, one obtains a gauge-independent result for the bubble nucleatio"},"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":"hep-ph/9507381","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1995-07-21T16:11:11Z","cross_cats_sorted":[],"title_canon_sha256":"f09e5adfe20af53416735fd87fc730b79e67f1bff36ecaf850abca46ad183ed1","abstract_canon_sha256":"82be9717f178a010a245578e070ca4cf018d9a6493b913ebe8360f14cc09414c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:59:11.186816Z","signature_b64":"dY2/d1op+K2FhMq8ZiAT5uM66HK2yKo3KJalUqqzB6gVayGH9V1LZXp52i3TcQr3NAVKmNZiFAVMM/lKJJ8KAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"084ac2c31aadf0fb3837ff91b20b898a09d6c4f6a9d3556c40bcff7bf76914cd","last_reissued_at":"2026-07-04T15:59:11.186485Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:59:11.186485Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gauge independence of the bubble nucleation rate in theories with radiative symmetry breaking","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Dimitrios Metaxas, Erick J. Weinberg (Columbia University)","submitted_at":"1995-07-21T16:11:11Z","abstract_excerpt":"In field theories where a metastable false vacuum state arises as a result of radiative corrections, the calculation of the rate of false vacuum decay by bubble nucleation depends on the effective potential and the other functions that appear in the derivative expansion of the effective action. Beginning with the Nielsen identity, we derive a series of identities that govern the gauge dependence of these functions. Using these, we show, to leading nontrivial order, that even though these functions are individually gauge-dependent, one obtains a gauge-independent result for the bubble nucleatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9507381","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/hep-ph/9507381/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":"hep-ph/9507381","created_at":"2026-07-04T15:59:11.186538+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9507381v1","created_at":"2026-07-04T15:59:11.186538+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9507381","created_at":"2026-07-04T15:59:11.186538+00:00"},{"alias_kind":"pith_short_12","alias_value":"BBFMFQY2VXYP","created_at":"2026-07-04T15:59:11.186538+00:00"},{"alias_kind":"pith_short_16","alias_value":"BBFMFQY2VXYPWOBX","created_at":"2026-07-04T15:59:11.186538+00:00"},{"alias_kind":"pith_short_8","alias_value":"BBFMFQY2","created_at":"2026-07-04T15:59:11.186538+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2607.02505","citing_title":"A critical look at low-scale cosmological phase transitions in the PTA era","ref_index":61,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26251","citing_title":"Supercool with PPO: Exploring Supercooled Phase Transitions via Reinforcement Learning","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2510.13770","citing_title":"Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe","ref_index":79,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI","json":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI.json","graph_json":"https://pith.science/api/pith-number/BBFMFQY2VXYPWOBX76I3EC4JRI/graph.json","events_json":"https://pith.science/api/pith-number/BBFMFQY2VXYPWOBX76I3EC4JRI/events.json","paper":"https://pith.science/paper/BBFMFQY2"},"agent_actions":{"view_html":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI","download_json":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI.json","view_paper":"https://pith.science/paper/BBFMFQY2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9507381&json=true","fetch_graph":"https://pith.science/api/pith-number/BBFMFQY2VXYPWOBX76I3EC4JRI/graph.json","fetch_events":"https://pith.science/api/pith-number/BBFMFQY2VXYPWOBX76I3EC4JRI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI/action/storage_attestation","attest_author":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI/action/author_attestation","sign_citation":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI/action/citation_signature","submit_replication":"https://pith.science/pith/BBFMFQY2VXYPWOBX76I3EC4JRI/action/replication_record"}},"created_at":"2026-07-04T15:59:11.186538+00:00","updated_at":"2026-07-04T15:59:11.186538+00:00"}