{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:ILVJI2YLVLMW6K56QHZZIGIRML","short_pith_number":"pith:ILVJI2YL","schema_version":"1.0","canonical_sha256":"42ea946b0baad96f2bbe81f394191162c2e979dd8f0e94291d02765f2e0aad9a","source":{"kind":"arxiv","id":"2111.15148","version":1},"attestation_state":"computed","paper":{"title":"Quantum power: a Lorentz invariant approach to Hawking radiation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th","quant-ph"],"primary_cat":"gr-qc","authors_text":"Eric V. Linder, Michael R.R. Good","submitted_at":"2021-11-30T06:13:34Z","abstract_excerpt":"Particle radiation from black holes has an observed emission power depending on the surface gravity $\\kappa = c^4/(4GM)$ as \\begin{equation}\\nonumber P_{\\textrm{black hole}} \\sim \\frac{\\hbar \\kappa^2}{6\\pi c^2} = \\frac{\\hbar c^6}{96\\pi G^2 M^2}\\,,\\end{equation} while both the radiation from accelerating particles and moving mirrors (accelerating boundaries) obey similar relativistic Larmor powers, \\begin{equation}\\nonumber P_{\\textrm{electron}}= \\frac{q^2\\alpha^2}{6\\pi \\epsilon_0 c^3}\\,, \\quad P_{\\textrm{mirror}} =\\frac{\\hbar \\alpha^2}{6\\pi c^2}\\,, \\end{equation} where $\\alpha$ is the Lorentz "},"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":"2111.15148","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2021-11-30T06:13:34Z","cross_cats_sorted":["hep-th","quant-ph"],"title_canon_sha256":"5162c4f5dd75342466d045af9b2d3c799ca0bc676fc79653fecb1556f2a2c4d6","abstract_canon_sha256":"f5b2c2d411997a50b440c006aa4e848853264d7dac5106a2ee31ca46730f2056"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:02:40.429124Z","signature_b64":"h4Qy8kcta0OlerCLaubCyk2j/4OZzUaCdgJ4brl7BOHykDQU8OohOoLQ8zi5f4v9zEiRhMiXV/lW4pEf6+eoBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"42ea946b0baad96f2bbe81f394191162c2e979dd8f0e94291d02765f2e0aad9a","last_reissued_at":"2026-07-05T04:02:40.428499Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:02:40.428499Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum power: a Lorentz invariant approach to Hawking radiation","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th","quant-ph"],"primary_cat":"gr-qc","authors_text":"Eric V. Linder, Michael R.R. Good","submitted_at":"2021-11-30T06:13:34Z","abstract_excerpt":"Particle radiation from black holes has an observed emission power depending on the surface gravity $\\kappa = c^4/(4GM)$ as \\begin{equation}\\nonumber P_{\\textrm{black hole}} \\sim \\frac{\\hbar \\kappa^2}{6\\pi c^2} = \\frac{\\hbar c^6}{96\\pi G^2 M^2}\\,,\\end{equation} while both the radiation from accelerating particles and moving mirrors (accelerating boundaries) obey similar relativistic Larmor powers, \\begin{equation}\\nonumber P_{\\textrm{electron}}= \\frac{q^2\\alpha^2}{6\\pi \\epsilon_0 c^3}\\,, \\quad P_{\\textrm{mirror}} =\\frac{\\hbar \\alpha^2}{6\\pi c^2}\\,, \\end{equation} where $\\alpha$ is the Lorentz "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.15148","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/2111.15148/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":"2111.15148","created_at":"2026-07-05T04:02:40.428565+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.15148v1","created_at":"2026-07-05T04:02:40.428565+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.15148","created_at":"2026-07-05T04:02:40.428565+00:00"},{"alias_kind":"pith_short_12","alias_value":"ILVJI2YLVLMW","created_at":"2026-07-05T04:02:40.428565+00:00"},{"alias_kind":"pith_short_16","alias_value":"ILVJI2YLVLMW6K56","created_at":"2026-07-05T04:02:40.428565+00:00"},{"alias_kind":"pith_short_8","alias_value":"ILVJI2YL","created_at":"2026-07-05T04:02:40.428565+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":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML","json":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML.json","graph_json":"https://pith.science/api/pith-number/ILVJI2YLVLMW6K56QHZZIGIRML/graph.json","events_json":"https://pith.science/api/pith-number/ILVJI2YLVLMW6K56QHZZIGIRML/events.json","paper":"https://pith.science/paper/ILVJI2YL"},"agent_actions":{"view_html":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML","download_json":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML.json","view_paper":"https://pith.science/paper/ILVJI2YL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.15148&json=true","fetch_graph":"https://pith.science/api/pith-number/ILVJI2YLVLMW6K56QHZZIGIRML/graph.json","fetch_events":"https://pith.science/api/pith-number/ILVJI2YLVLMW6K56QHZZIGIRML/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML/action/storage_attestation","attest_author":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML/action/author_attestation","sign_citation":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML/action/citation_signature","submit_replication":"https://pith.science/pith/ILVJI2YLVLMW6K56QHZZIGIRML/action/replication_record"}},"created_at":"2026-07-05T04:02:40.428565+00:00","updated_at":"2026-07-05T04:02:40.428565+00:00"}