{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:TJHQE47NNBDX4FTKSGWE6PFQEP","short_pith_number":"pith:TJHQE47N","schema_version":"1.0","canonical_sha256":"9a4f0273ed68477e166a91ac4f3cb023c32a6c69628bcab0a35201db75f5add2","source":{"kind":"arxiv","id":"0806.3801","version":1},"attestation_state":"computed","paper":{"title":"Nature of Microscopic Black Holes and Gravity in Theories with Particle Species","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gia Dvali","submitted_at":"2008-06-24T02:57:47Z","abstract_excerpt":"Relying solely on unitarity and the consistency with large-distance black hole physics, we derive model-independent properties of the microscopic black holes and of short-distance gravity in theories with N particle species. In this class of theories black holes can be as light as M_{Planck}/\\sqrt{N} and be produced in particle collisions above this energy. We show, that the micro black holes must come in the same variety as the species do, although their label is not associated with any conserved charge measurable at large distances. In contrast with big Schwarzschildian ones, the evaporation"},"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":"0806.3801","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2008-06-24T02:57:47Z","cross_cats_sorted":[],"title_canon_sha256":"56874b9a376ddecb78fc2fa9601f477e35f3499fe0b965f9c6b8f72091a5c8cc","abstract_canon_sha256":"79776ce901048255eaf429b37f398a4edb356a9869e5f41ee7e11611c033a8c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:21:44.014395Z","signature_b64":"XtPjsHMiy7TqLV5ElsUOt07YMmhYEYWZB5HbgtdgaYqAlYbk5MdQs2Ds5Zj8rwb+r4PnArrjWrFUrYsjRfZGAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a4f0273ed68477e166a91ac4f3cb023c32a6c69628bcab0a35201db75f5add2","last_reissued_at":"2026-07-04T17:21:44.013969Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:21:44.013969Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nature of Microscopic Black Holes and Gravity in Theories with Particle Species","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gia Dvali","submitted_at":"2008-06-24T02:57:47Z","abstract_excerpt":"Relying solely on unitarity and the consistency with large-distance black hole physics, we derive model-independent properties of the microscopic black holes and of short-distance gravity in theories with N particle species. In this class of theories black holes can be as light as M_{Planck}/\\sqrt{N} and be produced in particle collisions above this energy. We show, that the micro black holes must come in the same variety as the species do, although their label is not associated with any conserved charge measurable at large distances. In contrast with big Schwarzschildian ones, the evaporation"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0806.3801","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/0806.3801/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":"0806.3801","created_at":"2026-07-04T17:21:44.014032+00:00"},{"alias_kind":"arxiv_version","alias_value":"0806.3801v1","created_at":"2026-07-04T17:21:44.014032+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0806.3801","created_at":"2026-07-04T17:21:44.014032+00:00"},{"alias_kind":"pith_short_12","alias_value":"TJHQE47NNBDX","created_at":"2026-07-04T17:21:44.014032+00:00"},{"alias_kind":"pith_short_16","alias_value":"TJHQE47NNBDX4FTK","created_at":"2026-07-04T17:21:44.014032+00:00"},{"alias_kind":"pith_short_8","alias_value":"TJHQE47N","created_at":"2026-07-04T17:21:44.014032+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":10,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP","json":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP.json","graph_json":"https://pith.science/api/pith-number/TJHQE47NNBDX4FTKSGWE6PFQEP/graph.json","events_json":"https://pith.science/api/pith-number/TJHQE47NNBDX4FTKSGWE6PFQEP/events.json","paper":"https://pith.science/paper/TJHQE47N"},"agent_actions":{"view_html":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP","download_json":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP.json","view_paper":"https://pith.science/paper/TJHQE47N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0806.3801&json=true","fetch_graph":"https://pith.science/api/pith-number/TJHQE47NNBDX4FTKSGWE6PFQEP/graph.json","fetch_events":"https://pith.science/api/pith-number/TJHQE47NNBDX4FTKSGWE6PFQEP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP/action/storage_attestation","attest_author":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP/action/author_attestation","sign_citation":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP/action/citation_signature","submit_replication":"https://pith.science/pith/TJHQE47NNBDX4FTKSGWE6PFQEP/action/replication_record"}},"created_at":"2026-07-04T17:21:44.014032+00:00","updated_at":"2026-07-04T17:21:44.014032+00:00"}