{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:NXQYDLRN7XWUKJXQZIOSRLII5S","short_pith_number":"pith:NXQYDLRN","schema_version":"1.0","canonical_sha256":"6de181ae2dfded4526f0ca1d28ad08ecbb593532c0cde2df6ab3de1ff8c7cec1","source":{"kind":"arxiv","id":"0812.3442","version":1},"attestation_state":"computed","paper":{"title":"Micro Black Holes and the Democratic Transition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gia Dvali, Oriol Pujolas","submitted_at":"2008-12-18T20:42:37Z","abstract_excerpt":"Unitarity implies that the evaporation of microscopic quasi-classical black holes cannot be universal in different particle species. This creates a puzzle, since it conflicts with the thermal nature of quasi-classical black holes, according to which all the species should see the same horizon and be produced with the same Hawking temperatures. We resolve this puzzle by showing that for the microscopic black holes, on top the usual quantum evaporation time, there is a new time-scale which characterizes a purely classical process during which the black hole looses the ability to differentiate am"},"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":"0812.3442","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2008-12-18T20:42:37Z","cross_cats_sorted":[],"title_canon_sha256":"14955ab5c029e40ac0290725c42329dae9a3e47016b4b51f9c93edcafab36ba9","abstract_canon_sha256":"af05dc838cfb2d2563e5cf93b4e1e7eeef2209521b6b9cf52a9760bb010dd895"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:21:47.588761Z","signature_b64":"/lvhNsu38+Ag1c3tTWC22ewi3lX3fgCdQ4e2c7TQ4Zp4L+hxoFvIZwa5/jfpjuDQtz9ZuPZvSoZZ0PiNCDEzBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6de181ae2dfded4526f0ca1d28ad08ecbb593532c0cde2df6ab3de1ff8c7cec1","last_reissued_at":"2026-07-04T16:21:47.588412Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:21:47.588412Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Micro Black Holes and the Democratic Transition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gia Dvali, Oriol Pujolas","submitted_at":"2008-12-18T20:42:37Z","abstract_excerpt":"Unitarity implies that the evaporation of microscopic quasi-classical black holes cannot be universal in different particle species. This creates a puzzle, since it conflicts with the thermal nature of quasi-classical black holes, according to which all the species should see the same horizon and be produced with the same Hawking temperatures. We resolve this puzzle by showing that for the microscopic black holes, on top the usual quantum evaporation time, there is a new time-scale which characterizes a purely classical process during which the black hole looses the ability to differentiate am"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0812.3442","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/0812.3442/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":"0812.3442","created_at":"2026-07-04T16:21:47.588475+00:00"},{"alias_kind":"arxiv_version","alias_value":"0812.3442v1","created_at":"2026-07-04T16:21:47.588475+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0812.3442","created_at":"2026-07-04T16:21:47.588475+00:00"},{"alias_kind":"pith_short_12","alias_value":"NXQYDLRN7XWU","created_at":"2026-07-04T16:21:47.588475+00:00"},{"alias_kind":"pith_short_16","alias_value":"NXQYDLRN7XWUKJXQ","created_at":"2026-07-04T16:21:47.588475+00:00"},{"alias_kind":"pith_short_8","alias_value":"NXQYDLRN","created_at":"2026-07-04T16:21:47.588475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.01227","citing_title":"Modification of the laws of gravity in the DGP model by the presence of a second DGP brane","ref_index":9,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S","json":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S.json","graph_json":"https://pith.science/api/pith-number/NXQYDLRN7XWUKJXQZIOSRLII5S/graph.json","events_json":"https://pith.science/api/pith-number/NXQYDLRN7XWUKJXQZIOSRLII5S/events.json","paper":"https://pith.science/paper/NXQYDLRN"},"agent_actions":{"view_html":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S","download_json":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S.json","view_paper":"https://pith.science/paper/NXQYDLRN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0812.3442&json=true","fetch_graph":"https://pith.science/api/pith-number/NXQYDLRN7XWUKJXQZIOSRLII5S/graph.json","fetch_events":"https://pith.science/api/pith-number/NXQYDLRN7XWUKJXQZIOSRLII5S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S/action/storage_attestation","attest_author":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S/action/author_attestation","sign_citation":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S/action/citation_signature","submit_replication":"https://pith.science/pith/NXQYDLRN7XWUKJXQZIOSRLII5S/action/replication_record"}},"created_at":"2026-07-04T16:21:47.588475+00:00","updated_at":"2026-07-04T16:21:47.588475+00:00"}