{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:RNBAUZFTJI22RLMA3QMHGAEYON","short_pith_number":"pith:RNBAUZFT","schema_version":"1.0","canonical_sha256":"8b420a64b34a35a8ad80dc18730098737fc74fe75290b3f33fca71abf117dffd","source":{"kind":"arxiv","id":"gr-qc/0311040","version":1},"attestation_state":"computed","paper":{"title":"A criterion for bubble formation in de Sitter universe","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Michal Demetrian, Vladimir Balek","submitted_at":"2003-11-13T08:54:11Z","abstract_excerpt":"The influence of the shape of scalar field potential on the outcome of vacuum decay in de Sitter universe is studied. Sufficient condition for vacuum decay via bubble formation, described by Coleman - de Luccia instanton, is revisited and necessary condition is found. Both conditions require that the curvature of the potential is greater than 4 $\\times$ (Hubble constant)$^2$, but while the sufficient condition states that this inequality is to be valid at the top of the barrier, the necessary condition requires that it holds at least somewhere throughout the barrier. The conditions leave a 'gr"},"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/0311040","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2003-11-13T08:54:11Z","cross_cats_sorted":[],"title_canon_sha256":"a227ff4d5c6363ed1387663d79c36550f636a6406c3f179cef3c6499a1d3f38c","abstract_canon_sha256":"946e7772e690bc6c73fd96355fbd3e8127d64990452605736ed9d0de6eb78d8b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:40:18.719755Z","signature_b64":"qFCDIoxoj2UcaxnpFO5ldGdtzB1QyS7A2aMHhsFq9tPQRHIhTLWgF89ZJKRdNh+1vweKcQjr89o6M7MwVKcnAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b420a64b34a35a8ad80dc18730098737fc74fe75290b3f33fca71abf117dffd","last_reissued_at":"2026-07-04T16:40:18.719298Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:40:18.719298Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A criterion for bubble formation in de Sitter universe","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Michal Demetrian, Vladimir Balek","submitted_at":"2003-11-13T08:54:11Z","abstract_excerpt":"The influence of the shape of scalar field potential on the outcome of vacuum decay in de Sitter universe is studied. Sufficient condition for vacuum decay via bubble formation, described by Coleman - de Luccia instanton, is revisited and necessary condition is found. Both conditions require that the curvature of the potential is greater than 4 $\\times$ (Hubble constant)$^2$, but while the sufficient condition states that this inequality is to be valid at the top of the barrier, the necessary condition requires that it holds at least somewhere throughout the barrier. The conditions leave a 'gr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0311040","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/0311040/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/0311040","created_at":"2026-07-04T16:40:18.719407+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0311040v1","created_at":"2026-07-04T16:40:18.719407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0311040","created_at":"2026-07-04T16:40:18.719407+00:00"},{"alias_kind":"pith_short_12","alias_value":"RNBAUZFTJI22","created_at":"2026-07-04T16:40:18.719407+00:00"},{"alias_kind":"pith_short_16","alias_value":"RNBAUZFTJI22RLMA","created_at":"2026-07-04T16:40:18.719407+00:00"},{"alias_kind":"pith_short_8","alias_value":"RNBAUZFT","created_at":"2026-07-04T16:40:18.719407+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22998","citing_title":"Thermal effects and finite-temperature cosmology in perturbatively stabilized large volume scenarios","ref_index":83,"is_internal_anchor":true},{"citing_arxiv_id":"2605.03758","citing_title":"Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation","ref_index":43,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON","json":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON.json","graph_json":"https://pith.science/api/pith-number/RNBAUZFTJI22RLMA3QMHGAEYON/graph.json","events_json":"https://pith.science/api/pith-number/RNBAUZFTJI22RLMA3QMHGAEYON/events.json","paper":"https://pith.science/paper/RNBAUZFT"},"agent_actions":{"view_html":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON","download_json":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON.json","view_paper":"https://pith.science/paper/RNBAUZFT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0311040&json=true","fetch_graph":"https://pith.science/api/pith-number/RNBAUZFTJI22RLMA3QMHGAEYON/graph.json","fetch_events":"https://pith.science/api/pith-number/RNBAUZFTJI22RLMA3QMHGAEYON/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON/action/storage_attestation","attest_author":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON/action/author_attestation","sign_citation":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON/action/citation_signature","submit_replication":"https://pith.science/pith/RNBAUZFTJI22RLMA3QMHGAEYON/action/replication_record"}},"created_at":"2026-07-04T16:40:18.719407+00:00","updated_at":"2026-07-04T16:40:18.719407+00:00"}