{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:E4IDMOOC4UDLNEEZZCVXSRHYLD","short_pith_number":"pith:E4IDMOOC","schema_version":"1.0","canonical_sha256":"27103639c2e506b69099c8ab7944f858dd1b2dcd16232f7b544265b76313d838","source":{"kind":"arxiv","id":"2008.12251","version":2},"attestation_state":"computed","paper":{"title":"Particle Production by a Relativistic Semi-Transparent Mirror in 1+3D Minkowski Spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Chih-En Chou, Kuan-Nan Lin, Pisin Chen","submitted_at":"2020-08-27T16:47:24Z","abstract_excerpt":"Production of scalar particles by a relativistic, semi-transparent mirror in 1+3D Minkowski spacetime based on the Barton-Calogeracos (BC) action is investigated. The corresponding Bogoliubov coefficients are derived for a mirror with arbitrary trajectory. In particular, we apply our derived formula to the gravitational collapse trajectory. In addition, we identify the relation between the particle spectrum and the particle production probability, and we demonstrate the equivalence between our approach and the existing approach in the literature, which is restricted to 1+1D. In short, our trea"},"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":"2008.12251","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-08-27T16:47:24Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"0bef7a3da53d352d0b2925cd7e85d61009b54f5302caf1c23300b65e3b9f2c18","abstract_canon_sha256":"bf489cdfa280e9ef52176d7e3fd0f405b4a80e0b1f329f1d000cfdba4731ba69"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:08:10.879524Z","signature_b64":"Yzk7P15jcrZpg8k/0xMLlnt6aRCZuUBXw5Hr0XnVPZw1+9IGcqBtYIZYOvt/MqSDKddhap4RZ+O2zHva0icMAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"27103639c2e506b69099c8ab7944f858dd1b2dcd16232f7b544265b76313d838","last_reissued_at":"2026-07-05T02:08:10.879079Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:08:10.879079Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Particle Production by a Relativistic Semi-Transparent Mirror in 1+3D Minkowski Spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Chih-En Chou, Kuan-Nan Lin, Pisin Chen","submitted_at":"2020-08-27T16:47:24Z","abstract_excerpt":"Production of scalar particles by a relativistic, semi-transparent mirror in 1+3D Minkowski spacetime based on the Barton-Calogeracos (BC) action is investigated. The corresponding Bogoliubov coefficients are derived for a mirror with arbitrary trajectory. In particular, we apply our derived formula to the gravitational collapse trajectory. In addition, we identify the relation between the particle spectrum and the particle production probability, and we demonstrate the equivalence between our approach and the existing approach in the literature, which is restricted to 1+1D. In short, our trea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.12251","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/2008.12251/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":"2008.12251","created_at":"2026-07-05T02:08:10.879151+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.12251v2","created_at":"2026-07-05T02:08:10.879151+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.12251","created_at":"2026-07-05T02:08:10.879151+00:00"},{"alias_kind":"pith_short_12","alias_value":"E4IDMOOC4UDL","created_at":"2026-07-05T02:08:10.879151+00:00"},{"alias_kind":"pith_short_16","alias_value":"E4IDMOOC4UDLNEEZ","created_at":"2026-07-05T02:08:10.879151+00:00"},{"alias_kind":"pith_short_8","alias_value":"E4IDMOOC","created_at":"2026-07-05T02:08:10.879151+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.11957","citing_title":"Squeezed quantum states and partner modes in the moving mirror model of black hole evaporation","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD","json":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD.json","graph_json":"https://pith.science/api/pith-number/E4IDMOOC4UDLNEEZZCVXSRHYLD/graph.json","events_json":"https://pith.science/api/pith-number/E4IDMOOC4UDLNEEZZCVXSRHYLD/events.json","paper":"https://pith.science/paper/E4IDMOOC"},"agent_actions":{"view_html":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD","download_json":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD.json","view_paper":"https://pith.science/paper/E4IDMOOC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.12251&json=true","fetch_graph":"https://pith.science/api/pith-number/E4IDMOOC4UDLNEEZZCVXSRHYLD/graph.json","fetch_events":"https://pith.science/api/pith-number/E4IDMOOC4UDLNEEZZCVXSRHYLD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD/action/storage_attestation","attest_author":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD/action/author_attestation","sign_citation":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD/action/citation_signature","submit_replication":"https://pith.science/pith/E4IDMOOC4UDLNEEZZCVXSRHYLD/action/replication_record"}},"created_at":"2026-07-05T02:08:10.879151+00:00","updated_at":"2026-07-05T02:08:10.879151+00:00"}