{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:PEJUATCNDGF7RG6WBXOSNXMJBK","short_pith_number":"pith:PEJUATCN","schema_version":"1.0","canonical_sha256":"7913404c4d198bf89bd60ddd26dd890a87039485b7c6077a896abcb6ebf6cd4f","source":{"kind":"arxiv","id":"1005.1232","version":5},"attestation_state":"computed","paper":{"title":"Stochastic emergence of inflaton fluctuations in a SdS primordial universe with large-scale repulsive gravity from a 5D vacuum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"CONICET), Jose Edgar Madriz Aguilar (Guanajuato University), Luz Marina Reyes, Mauricio Bellini (Mar del Plata University & IFM","submitted_at":"2010-05-07T15:30:37Z","abstract_excerpt":"We develop a stochastic approach to study scalar field fluctuations of the inflaton field in an early inflationary universe with a black-hole (BH), which is described by an effective 4D SdS metric. Considering a 5D Ricci-flat SdS static metric, we implement a planar coordinate transformation, in order to obtain a 5D cosmological metric, from which the effective 4D SdS metric can be induced on a 4D hypersurface. We found that at the end of inflation, the squared fluctuations of the inflaton field are not exactly scale independent and becomes sensitive with the mass of the BH."},"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":"1005.1232","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-05-07T15:30:37Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"170b8718a94776e7c05aea8301aedfec1dd70b628b71ce1c04f4814307449db3","abstract_canon_sha256":"565ae2333575b48974f0ec8fb7873dfa09dac2fdc8b3e7fc1e0eb7c9de123eed"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:20:05.029281Z","signature_b64":"55zhsKupkYEV25DzVeHHFcB50Bi+wzxxzG9ms2zAHyZ1MlAyENhq/+9fuVwySe2JDrfivI1P/0gYezAr/iS0AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7913404c4d198bf89bd60ddd26dd890a87039485b7c6077a896abcb6ebf6cd4f","last_reissued_at":"2026-05-18T04:20:05.028837Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:20:05.028837Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stochastic emergence of inflaton fluctuations in a SdS primordial universe with large-scale repulsive gravity from a 5D vacuum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"CONICET), Jose Edgar Madriz Aguilar (Guanajuato University), Luz Marina Reyes, Mauricio Bellini (Mar del Plata University & IFM","submitted_at":"2010-05-07T15:30:37Z","abstract_excerpt":"We develop a stochastic approach to study scalar field fluctuations of the inflaton field in an early inflationary universe with a black-hole (BH), which is described by an effective 4D SdS metric. Considering a 5D Ricci-flat SdS static metric, we implement a planar coordinate transformation, in order to obtain a 5D cosmological metric, from which the effective 4D SdS metric can be induced on a 4D hypersurface. We found that at the end of inflation, the squared fluctuations of the inflaton field are not exactly scale independent and becomes sensitive with the mass of the BH."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1232","kind":"arxiv","version":5},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1005.1232","created_at":"2026-05-18T04:20:05.028898+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1232v5","created_at":"2026-05-18T04:20:05.028898+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1232","created_at":"2026-05-18T04:20:05.028898+00:00"},{"alias_kind":"pith_short_12","alias_value":"PEJUATCNDGF7","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"PEJUATCNDGF7RG6W","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"PEJUATCN","created_at":"2026-05-18T12:26:12.377268+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK","json":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK.json","graph_json":"https://pith.science/api/pith-number/PEJUATCNDGF7RG6WBXOSNXMJBK/graph.json","events_json":"https://pith.science/api/pith-number/PEJUATCNDGF7RG6WBXOSNXMJBK/events.json","paper":"https://pith.science/paper/PEJUATCN"},"agent_actions":{"view_html":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK","download_json":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK.json","view_paper":"https://pith.science/paper/PEJUATCN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1232&json=true","fetch_graph":"https://pith.science/api/pith-number/PEJUATCNDGF7RG6WBXOSNXMJBK/graph.json","fetch_events":"https://pith.science/api/pith-number/PEJUATCNDGF7RG6WBXOSNXMJBK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK/action/storage_attestation","attest_author":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK/action/author_attestation","sign_citation":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK/action/citation_signature","submit_replication":"https://pith.science/pith/PEJUATCNDGF7RG6WBXOSNXMJBK/action/replication_record"}},"created_at":"2026-05-18T04:20:05.028898+00:00","updated_at":"2026-05-18T04:20:05.028898+00:00"}