{"paper":{"title":"Hawking temperature in the tunneling picture","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Douglas Singleton, Emil T. Akhmedov, Valeria Akhmedova","submitted_at":"2006-08-15T05:40:35Z","abstract_excerpt":"We examine Hawking radiation from a Schwarzschild black hole in several reference frames using the quasi-classical tunneling picture. It is shown that when one uses, $\\Gamma \\propto \\exp(Im [\\oint p dr])$, rather than, $\\Gamma \\propto \\exp(2 Im [\\int p dr])$, for the tunneling probability/decay rate one obtains twice the original Hawking temperature. The former expression for $\\Gamma$ is argued to be correct since $\\oint p dr$ is invariant under canonical transformations, while $\\int p dr$ is not. Thus, either the tunneling methods of calculating Hawking radiation are suspect or the Hawking te"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0608098","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":""},"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"}