{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:2GINWIDZP2GQJCMIQM2TBQYXY5","short_pith_number":"pith:2GINWIDZ","schema_version":"1.0","canonical_sha256":"d190db20797e8d048988833530c317c77bf76281a6bcb5ee4714273ae1a57a6e","source":{"kind":"arxiv","id":"0708.1220","version":1},"attestation_state":"computed","paper":{"title":"UV/IR Mixing and Black Hole Thermodynamics","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Behnaz Fazlpour, Kourosh Nozari","submitted_at":"2007-08-09T07:13:49Z","abstract_excerpt":"The goal of this paper is to investigate the final stage of black hole evaporation process in the framework of Lorentz violating Modified Dispersion Relations(MDRs). As a consequence of MDRs, the high energy sector of the underlying field theory does not decouple from the low energy sector, the phenomenon which is known as UV/IR mixing. In the absence of exact supersymmetry, we derive a modified dispersion relation which shows UV/IR mixing by a novel energy dependence. Then we investigate the effects of these type of MDRs on the thermodynamics of a radiating noncommutative Schwarzschild black "},"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":"0708.1220","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2007-08-09T07:13:49Z","cross_cats_sorted":[],"title_canon_sha256":"f3b4f75833ae14281111731c22332c70e8368f883a7706a070780dfcf3a15241","abstract_canon_sha256":"0354d9f6939640b7a5df6163d94491f03851d38413a4ce552c2c011b3f8ae1cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:24:34.062752Z","signature_b64":"01zKPlGDfo13v3bEBpEMOnsiRoSBSQxUiXTONFmqbuDvQBahMw37q5Exlr3ARvEEx4WZiflZn4I76+vvBpfkBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d190db20797e8d048988833530c317c77bf76281a6bcb5ee4714273ae1a57a6e","last_reissued_at":"2026-07-04T15:24:34.062285Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:24:34.062285Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"UV/IR Mixing and Black Hole Thermodynamics","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Behnaz Fazlpour, Kourosh Nozari","submitted_at":"2007-08-09T07:13:49Z","abstract_excerpt":"The goal of this paper is to investigate the final stage of black hole evaporation process in the framework of Lorentz violating Modified Dispersion Relations(MDRs). As a consequence of MDRs, the high energy sector of the underlying field theory does not decouple from the low energy sector, the phenomenon which is known as UV/IR mixing. In the absence of exact supersymmetry, we derive a modified dispersion relation which shows UV/IR mixing by a novel energy dependence. Then we investigate the effects of these type of MDRs on the thermodynamics of a radiating noncommutative Schwarzschild black "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0708.1220","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/0708.1220/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":"0708.1220","created_at":"2026-07-04T15:24:34.062343+00:00"},{"alias_kind":"arxiv_version","alias_value":"0708.1220v1","created_at":"2026-07-04T15:24:34.062343+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0708.1220","created_at":"2026-07-04T15:24:34.062343+00:00"},{"alias_kind":"pith_short_12","alias_value":"2GINWIDZP2GQ","created_at":"2026-07-04T15:24:34.062343+00:00"},{"alias_kind":"pith_short_16","alias_value":"2GINWIDZP2GQJCMI","created_at":"2026-07-04T15:24:34.062343+00:00"},{"alias_kind":"pith_short_8","alias_value":"2GINWIDZ","created_at":"2026-07-04T15:24:34.062343+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.18255","citing_title":"Perturbative black-hole and horizon solutions in gravity with explicit spacetime-symmetry breaking","ref_index":94,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5","json":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5.json","graph_json":"https://pith.science/api/pith-number/2GINWIDZP2GQJCMIQM2TBQYXY5/graph.json","events_json":"https://pith.science/api/pith-number/2GINWIDZP2GQJCMIQM2TBQYXY5/events.json","paper":"https://pith.science/paper/2GINWIDZ"},"agent_actions":{"view_html":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5","download_json":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5.json","view_paper":"https://pith.science/paper/2GINWIDZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0708.1220&json=true","fetch_graph":"https://pith.science/api/pith-number/2GINWIDZP2GQJCMIQM2TBQYXY5/graph.json","fetch_events":"https://pith.science/api/pith-number/2GINWIDZP2GQJCMIQM2TBQYXY5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5/action/storage_attestation","attest_author":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5/action/author_attestation","sign_citation":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5/action/citation_signature","submit_replication":"https://pith.science/pith/2GINWIDZP2GQJCMIQM2TBQYXY5/action/replication_record"}},"created_at":"2026-07-04T15:24:34.062343+00:00","updated_at":"2026-07-04T15:24:34.062343+00:00"}