{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:IVUUAZAGIXQ4ERRKRRDKDX43W5","short_pith_number":"pith:IVUUAZAG","schema_version":"1.0","canonical_sha256":"456940640645e1c2462a8c46a1df9bb760ea2640431858cd0674e5c58cb3f523","source":{"kind":"arxiv","id":"1410.1298","version":1},"attestation_state":"computed","paper":{"title":"Non-Linear Trans-Planckian Corrections of Spectra due to the Non-trivial Initial States","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"E. Yusofi, M. Mohsenzadeh","submitted_at":"2014-10-06T09:25:44Z","abstract_excerpt":"Recent Planck results motivated us to use non-Bunch-Davies vacuum. In this paper, we use the excited-de Sitter mode as non-linear initial states during inflation to calculate the corrected spectra of the initial fluctuations of the scalar field. First, we consider the field in de Sitter space-time as background field and for the non-Bunch-Davies mode, we use the perturbation theory to the second order approximation. Also, unlike conventional renormalization method, we offer de Sitter space-time as the background instead Minkowski space-time. This approach preserve the symmetry of curved space-"},"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":"1410.1298","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2014-10-06T09:25:44Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"1fe40e21641dddd025a09bda136ab754339f49740c402a04a783de08a42c39b1","abstract_canon_sha256":"73d6934e1d5e301f9108e831715c15c77b2c7714bf69616f03634ff1558973f6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:41:02.361035Z","signature_b64":"8M4Zq4vw79PjuXjAgT18fI4A74tyolKlfgpbMTacUAJCPNdqoD9AhgkYxldQlwaYKCl3yI98Q/WKOBnlPOopBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"456940640645e1c2462a8c46a1df9bb760ea2640431858cd0674e5c58cb3f523","last_reissued_at":"2026-05-18T02:41:02.360600Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:41:02.360600Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Linear Trans-Planckian Corrections of Spectra due to the Non-trivial Initial States","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"E. Yusofi, M. Mohsenzadeh","submitted_at":"2014-10-06T09:25:44Z","abstract_excerpt":"Recent Planck results motivated us to use non-Bunch-Davies vacuum. In this paper, we use the excited-de Sitter mode as non-linear initial states during inflation to calculate the corrected spectra of the initial fluctuations of the scalar field. First, we consider the field in de Sitter space-time as background field and for the non-Bunch-Davies mode, we use the perturbation theory to the second order approximation. Also, unlike conventional renormalization method, we offer de Sitter space-time as the background instead Minkowski space-time. This approach preserve the symmetry of curved space-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.1298","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":""},"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":"1410.1298","created_at":"2026-05-18T02:41:02.360655+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.1298v1","created_at":"2026-05-18T02:41:02.360655+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.1298","created_at":"2026-05-18T02:41:02.360655+00:00"},{"alias_kind":"pith_short_12","alias_value":"IVUUAZAGIXQ4","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_16","alias_value":"IVUUAZAGIXQ4ERRK","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_8","alias_value":"IVUUAZAG","created_at":"2026-05-18T12:28:33.132498+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/IVUUAZAGIXQ4ERRKRRDKDX43W5","json":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5.json","graph_json":"https://pith.science/api/pith-number/IVUUAZAGIXQ4ERRKRRDKDX43W5/graph.json","events_json":"https://pith.science/api/pith-number/IVUUAZAGIXQ4ERRKRRDKDX43W5/events.json","paper":"https://pith.science/paper/IVUUAZAG"},"agent_actions":{"view_html":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5","download_json":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5.json","view_paper":"https://pith.science/paper/IVUUAZAG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.1298&json=true","fetch_graph":"https://pith.science/api/pith-number/IVUUAZAGIXQ4ERRKRRDKDX43W5/graph.json","fetch_events":"https://pith.science/api/pith-number/IVUUAZAGIXQ4ERRKRRDKDX43W5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5/action/storage_attestation","attest_author":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5/action/author_attestation","sign_citation":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5/action/citation_signature","submit_replication":"https://pith.science/pith/IVUUAZAGIXQ4ERRKRRDKDX43W5/action/replication_record"}},"created_at":"2026-05-18T02:41:02.360655+00:00","updated_at":"2026-05-18T02:41:02.360655+00:00"}