{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:BINS6XNPD74BJE44DAA5WCFTCM","short_pith_number":"pith:BINS6XNP","schema_version":"1.0","canonical_sha256":"0a1b2f5daf1ff814939c1801db08b31339b3580c88252a67a2678bd1510db305","source":{"kind":"arxiv","id":"1903.00043","version":7},"attestation_state":"computed","paper":{"title":"Experimental Observation of Acceleration-Induced Thermality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Eliahu Cohen, Ido Kaminer, Morgan H. Lynch, Yaron Hadad","submitted_at":"2019-02-28T19:39:53Z","abstract_excerpt":"We examine the radiation emitted by high energy positrons channeled into silicon crystal samples. The positrons are modeled as semiclassical vector currents coupled to an Unruh-DeWitt detector to incorporate any local change in the energy of the positron. In the subsequent accelerated QED analysis, we discover a Larmor formula and power spectrum that are both thermalized by the acceleration. Thus, these systems explicitly exhibit thermalization of the detector energy gap at the celebrated Fulling-Davies-Unruh (FDU) temperature. Our derived power spectrum, with a nonzero energy gap, is then sho"},"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":"1903.00043","kind":"arxiv","version":7},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-02-28T19:39:53Z","cross_cats_sorted":["hep-ph","hep-th"],"title_canon_sha256":"fa3b3455c210f45d7d4bfb44a9a91fc20da4b5bcbbd6cc638475d7a416740cdf","abstract_canon_sha256":"6b5f4fd4a9304901d936aabb3984fcf980b99cfb2628607468cd876b3837e164"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:01:08.117109Z","signature_b64":"A6yg+5H2Ie178uP8IR3Vf3Rq9rJV7t5iNse8/Jjb+gnzQZnuoJQnOZbXqXKdlA7pLabkcs6+oXJsgAKLiGTZDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0a1b2f5daf1ff814939c1801db08b31339b3580c88252a67a2678bd1510db305","last_reissued_at":"2026-07-05T03:01:08.116741Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:01:08.116741Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Experimental Observation of Acceleration-Induced Thermality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Eliahu Cohen, Ido Kaminer, Morgan H. Lynch, Yaron Hadad","submitted_at":"2019-02-28T19:39:53Z","abstract_excerpt":"We examine the radiation emitted by high energy positrons channeled into silicon crystal samples. The positrons are modeled as semiclassical vector currents coupled to an Unruh-DeWitt detector to incorporate any local change in the energy of the positron. In the subsequent accelerated QED analysis, we discover a Larmor formula and power spectrum that are both thermalized by the acceleration. Thus, these systems explicitly exhibit thermalization of the detector energy gap at the celebrated Fulling-Davies-Unruh (FDU) temperature. Our derived power spectrum, with a nonzero energy gap, is then sho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.00043","kind":"arxiv","version":7},"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/1903.00043/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":"1903.00043","created_at":"2026-07-05T03:01:08.116804+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.00043v7","created_at":"2026-07-05T03:01:08.116804+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.00043","created_at":"2026-07-05T03:01:08.116804+00:00"},{"alias_kind":"pith_short_12","alias_value":"BINS6XNPD74B","created_at":"2026-07-05T03:01:08.116804+00:00"},{"alias_kind":"pith_short_16","alias_value":"BINS6XNPD74BJE44","created_at":"2026-07-05T03:01:08.116804+00:00"},{"alias_kind":"pith_short_8","alias_value":"BINS6XNP","created_at":"2026-07-05T03:01:08.116804+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.20314","citing_title":"Macroscopic Black-Hole Remnants in a Nonlocal Field Theory: Towards Hawking Radiation in SFT","ref_index":62,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM","json":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM.json","graph_json":"https://pith.science/api/pith-number/BINS6XNPD74BJE44DAA5WCFTCM/graph.json","events_json":"https://pith.science/api/pith-number/BINS6XNPD74BJE44DAA5WCFTCM/events.json","paper":"https://pith.science/paper/BINS6XNP"},"agent_actions":{"view_html":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM","download_json":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM.json","view_paper":"https://pith.science/paper/BINS6XNP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.00043&json=true","fetch_graph":"https://pith.science/api/pith-number/BINS6XNPD74BJE44DAA5WCFTCM/graph.json","fetch_events":"https://pith.science/api/pith-number/BINS6XNPD74BJE44DAA5WCFTCM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM/action/storage_attestation","attest_author":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM/action/author_attestation","sign_citation":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM/action/citation_signature","submit_replication":"https://pith.science/pith/BINS6XNPD74BJE44DAA5WCFTCM/action/replication_record"}},"created_at":"2026-07-05T03:01:08.116804+00:00","updated_at":"2026-07-05T03:01:08.116804+00:00"}