{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:KGXQL36UJ4K27USFJT7FSXT4W7","short_pith_number":"pith:KGXQL36U","schema_version":"1.0","canonical_sha256":"51af05efd44f15afd2454cfe595e7cb7c2d6ab0cdfb0e20231519802eb64c122","source":{"kind":"arxiv","id":"hep-th/0509128","version":2},"attestation_state":"computed","paper":{"title":"Exact Results for Evaporating Black Holes in Curvature-Squared Lovelock Gravity: Gauss-Bonnet Greybody Factors","license":"","headline":"","cross_cats":["astro-ph","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"A. Barrau, J. Grain, P. Kanti","submitted_at":"2005-09-16T10:24:42Z","abstract_excerpt":"Lovelock gravity is an important extension of General Relativity that provides a promising framework to study curvature corrections to the Einstein action, while avoiding ghosts and keeping second order field equations. This paper derives the greybody factors for D-dimensional black holes arising in a theory with a Gauss-Bonnet curvature-squared term. These factors describe the non-trivial coupling between black holes and quantum fields during the evaporation process: they can be used both from a theoretical viewpoint to investigate the intricate spacetime structure around such a black hole, a"},"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-th/0509128","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2005-09-16T10:24:42Z","cross_cats_sorted":["astro-ph","gr-qc","hep-ph"],"title_canon_sha256":"fe2ce6f6c0439fcd0d9bca848e7b609c2e811aafb243b70c1e765287f8646973","abstract_canon_sha256":"9ee90e6625c971ca2afd003479fdf2cc2a215634f68feeddbf9b17d5fd416f1c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:28:52.261856Z","signature_b64":"P2z96JKlH5Ms3VwnQdYpv4B7bzCSuQrJ5UGVscR7qVhY9yyNNk/tC6WMoRTXyxnB8fFsTnpwT4vE+f4tcn1CAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"51af05efd44f15afd2454cfe595e7cb7c2d6ab0cdfb0e20231519802eb64c122","last_reissued_at":"2026-07-04T15:28:52.261422Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:28:52.261422Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exact Results for Evaporating Black Holes in Curvature-Squared Lovelock Gravity: Gauss-Bonnet Greybody Factors","license":"","headline":"","cross_cats":["astro-ph","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"A. Barrau, J. Grain, P. Kanti","submitted_at":"2005-09-16T10:24:42Z","abstract_excerpt":"Lovelock gravity is an important extension of General Relativity that provides a promising framework to study curvature corrections to the Einstein action, while avoiding ghosts and keeping second order field equations. This paper derives the greybody factors for D-dimensional black holes arising in a theory with a Gauss-Bonnet curvature-squared term. These factors describe the non-trivial coupling between black holes and quantum fields during the evaporation process: they can be used both from a theoretical viewpoint to investigate the intricate spacetime structure around such a black hole, a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0509128","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/hep-th/0509128/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-th/0509128","created_at":"2026-07-04T15:28:52.261482+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0509128v2","created_at":"2026-07-04T15:28:52.261482+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0509128","created_at":"2026-07-04T15:28:52.261482+00:00"},{"alias_kind":"pith_short_12","alias_value":"KGXQL36UJ4K2","created_at":"2026-07-04T15:28:52.261482+00:00"},{"alias_kind":"pith_short_16","alias_value":"KGXQL36UJ4K27USF","created_at":"2026-07-04T15:28:52.261482+00:00"},{"alias_kind":"pith_short_8","alias_value":"KGXQL36U","created_at":"2026-07-04T15:28:52.261482+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.14510","citing_title":"Anisotropic Neutrino Emission from Spinning, Moving, and Charged Primordial Black Holes","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7","json":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7.json","graph_json":"https://pith.science/api/pith-number/KGXQL36UJ4K27USFJT7FSXT4W7/graph.json","events_json":"https://pith.science/api/pith-number/KGXQL36UJ4K27USFJT7FSXT4W7/events.json","paper":"https://pith.science/paper/KGXQL36U"},"agent_actions":{"view_html":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7","download_json":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7.json","view_paper":"https://pith.science/paper/KGXQL36U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0509128&json=true","fetch_graph":"https://pith.science/api/pith-number/KGXQL36UJ4K27USFJT7FSXT4W7/graph.json","fetch_events":"https://pith.science/api/pith-number/KGXQL36UJ4K27USFJT7FSXT4W7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7/action/storage_attestation","attest_author":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7/action/author_attestation","sign_citation":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7/action/citation_signature","submit_replication":"https://pith.science/pith/KGXQL36UJ4K27USFJT7FSXT4W7/action/replication_record"}},"created_at":"2026-07-04T15:28:52.261482+00:00","updated_at":"2026-07-04T15:28:52.261482+00:00"}