{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RUA2L2ZQZONH7MADPYWEBRR2ZY","short_pith_number":"pith:RUA2L2ZQ","schema_version":"1.0","canonical_sha256":"8d01a5eb30cb9a7fb0037e2c40c63ace30ad229316fb1d64d87539428ef83201","source":{"kind":"arxiv","id":"2412.06996","version":2},"attestation_state":"computed","paper":{"title":"Searching for the classical version of Hawking radiation and screening of Coulomb field by the horizon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"D.S. Shatkov, S.A. Paston","submitted_at":"2024-12-09T21:05:28Z","abstract_excerpt":"We investigate the possibility of the existence of a classical version of Hawking radiation - solutions to classical field equations that consist solely of outgoing waves, in the spacetime of a collapsing black hole. The non-static nature of the corresponding metric results in the absence of energy conservation for matter, which could otherwise a priori prohibit such solutions. A specific and simple scenario is considered: a black hole formation as a result of the collapse of a thin shell, which is not necessarily dust-like. In the corresponding spacetime, we study solutions of the equations f"},"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":"2412.06996","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-12-09T21:05:28Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"d3373eb454c69b9fc98dc82f04bd36cfe3ae204039006b5f21bdd8a4ba748b07","abstract_canon_sha256":"81b25c5add22d36480b65b480293c978e0c4ed464e10802a2a58aadbb9ac0dff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:18:40.760689Z","signature_b64":"j3L/vftuKu6eWemIms0tWon2nPNeQXp544F0Q7TEss5fEBFm96M7QzefDjN2o34FM7HaMLvyCQBSbP5ou7nfCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8d01a5eb30cb9a7fb0037e2c40c63ace30ad229316fb1d64d87539428ef83201","last_reissued_at":"2026-07-05T11:18:40.760204Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:18:40.760204Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for the classical version of Hawking radiation and screening of Coulomb field by the horizon","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"D.S. Shatkov, S.A. Paston","submitted_at":"2024-12-09T21:05:28Z","abstract_excerpt":"We investigate the possibility of the existence of a classical version of Hawking radiation - solutions to classical field equations that consist solely of outgoing waves, in the spacetime of a collapsing black hole. The non-static nature of the corresponding metric results in the absence of energy conservation for matter, which could otherwise a priori prohibit such solutions. A specific and simple scenario is considered: a black hole formation as a result of the collapse of a thin shell, which is not necessarily dust-like. In the corresponding spacetime, we study solutions of the equations f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.06996","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/2412.06996/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":"2412.06996","created_at":"2026-07-05T11:18:40.760257+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.06996v2","created_at":"2026-07-05T11:18:40.760257+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.06996","created_at":"2026-07-05T11:18:40.760257+00:00"},{"alias_kind":"pith_short_12","alias_value":"RUA2L2ZQZONH","created_at":"2026-07-05T11:18:40.760257+00:00"},{"alias_kind":"pith_short_16","alias_value":"RUA2L2ZQZONH7MAD","created_at":"2026-07-05T11:18:40.760257+00:00"},{"alias_kind":"pith_short_8","alias_value":"RUA2L2ZQ","created_at":"2026-07-05T11:18:40.760257+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.17059","citing_title":"TheUse of Conditional Variational Autoencoders in Generating Stellar Spectra","ref_index":18,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY","json":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY.json","graph_json":"https://pith.science/api/pith-number/RUA2L2ZQZONH7MADPYWEBRR2ZY/graph.json","events_json":"https://pith.science/api/pith-number/RUA2L2ZQZONH7MADPYWEBRR2ZY/events.json","paper":"https://pith.science/paper/RUA2L2ZQ"},"agent_actions":{"view_html":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY","download_json":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY.json","view_paper":"https://pith.science/paper/RUA2L2ZQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.06996&json=true","fetch_graph":"https://pith.science/api/pith-number/RUA2L2ZQZONH7MADPYWEBRR2ZY/graph.json","fetch_events":"https://pith.science/api/pith-number/RUA2L2ZQZONH7MADPYWEBRR2ZY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY/action/storage_attestation","attest_author":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY/action/author_attestation","sign_citation":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY/action/citation_signature","submit_replication":"https://pith.science/pith/RUA2L2ZQZONH7MADPYWEBRR2ZY/action/replication_record"}},"created_at":"2026-07-05T11:18:40.760257+00:00","updated_at":"2026-07-05T11:18:40.760257+00:00"}