{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:MQ4RSNRMRLJBIFGEBFS7QUQ2OE","short_pith_number":"pith:MQ4RSNRM","schema_version":"1.0","canonical_sha256":"643919362c8ad21414c40965f8521a71313cb434d530b6fe237754395957df2d","source":{"kind":"arxiv","id":"hep-ph/9812483","version":1},"attestation_state":"computed","paper":{"title":"Brane Inflation","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Gia Dvali, S.-H. Henry Tye","submitted_at":"1998-12-22T21:04:15Z","abstract_excerpt":"We present a novel inflationary scenario in theories with low scale (TeV) quantum gravity, in which the standard model particles are localized on the branes whereas gravity propagates in the bulk of large extra dimensions. This inflationary scenario is natural in the brane world picture. In the lowest energy state, a number of branes sit on top of each other (or at an orientifold plane), so the vacuum energy cancels out. In the cosmological setting, some of the branes \"start out\" relatively displaced in the extra dimensions and the resulting vacuum energy triggers the exponential growth of the"},"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":"hep-ph/9812483","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1998-12-22T21:04:15Z","cross_cats_sorted":[],"title_canon_sha256":"27bee2a777aafcaf7d7610518b1696719cca566b9013dfff95ed5c4a8a41e7c7","abstract_canon_sha256":"8474f8e14370fbd136b3aa8e6ed335f3fd14c88917d2500c97ddc06e6c472ebb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:09:38.923173Z","signature_b64":"l32clmTMRjFyfeBhtlWDZ5USgN//t80ROX7vjevAKVOWaYiXc6dBDosTLcmgT8Zn8O6Vdj6E1moc1X5R5weSBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"643919362c8ad21414c40965f8521a71313cb434d530b6fe237754395957df2d","last_reissued_at":"2026-07-04T16:09:38.922819Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:09:38.922819Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Brane Inflation","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Gia Dvali, S.-H. Henry Tye","submitted_at":"1998-12-22T21:04:15Z","abstract_excerpt":"We present a novel inflationary scenario in theories with low scale (TeV) quantum gravity, in which the standard model particles are localized on the branes whereas gravity propagates in the bulk of large extra dimensions. This inflationary scenario is natural in the brane world picture. In the lowest energy state, a number of branes sit on top of each other (or at an orientifold plane), so the vacuum energy cancels out. In the cosmological setting, some of the branes \"start out\" relatively displaced in the extra dimensions and the resulting vacuum energy triggers the exponential growth of the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9812483","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/hep-ph/9812483/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":"hep-ph/9812483","created_at":"2026-07-04T16:09:38.922882+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9812483v1","created_at":"2026-07-04T16:09:38.922882+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9812483","created_at":"2026-07-04T16:09:38.922882+00:00"},{"alias_kind":"pith_short_12","alias_value":"MQ4RSNRMRLJB","created_at":"2026-07-04T16:09:38.922882+00:00"},{"alias_kind":"pith_short_16","alias_value":"MQ4RSNRMRLJBIFGE","created_at":"2026-07-04T16:09:38.922882+00:00"},{"alias_kind":"pith_short_8","alias_value":"MQ4RSNRM","created_at":"2026-07-04T16:09:38.922882+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2607.07684","citing_title":"Unification of polynomial and exponential cosmological attractors","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20486","citing_title":"Cosmological history after higher dimensional inflation","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2511.06453","citing_title":"Inflationary models in a minimally coupled $f(R,T)$ gravity: Constraints from $Planck$, BICEP/$Keck$, and ACT","ref_index":67,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE","json":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE.json","graph_json":"https://pith.science/api/pith-number/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/graph.json","events_json":"https://pith.science/api/pith-number/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/events.json","paper":"https://pith.science/paper/MQ4RSNRM"},"agent_actions":{"view_html":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE","download_json":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE.json","view_paper":"https://pith.science/paper/MQ4RSNRM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9812483&json=true","fetch_graph":"https://pith.science/api/pith-number/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/graph.json","fetch_events":"https://pith.science/api/pith-number/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/action/storage_attestation","attest_author":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/action/author_attestation","sign_citation":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/action/citation_signature","submit_replication":"https://pith.science/pith/MQ4RSNRMRLJBIFGEBFS7QUQ2OE/action/replication_record"}},"created_at":"2026-07-04T16:09:38.922882+00:00","updated_at":"2026-07-04T16:09:38.922882+00:00"}