{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:SWHUPMGFGA4NUDEUVDKQCOAUIA","short_pith_number":"pith:SWHUPMGF","schema_version":"1.0","canonical_sha256":"958f47b0c53038da0c94a8d501381440348516a0cc7b9cf7c84abe53d2c150b5","source":{"kind":"arxiv","id":"1711.04807","version":2},"attestation_state":"computed","paper":{"title":"Confronting K\\\"ahler moduli inflation with CMB data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Anshuman Maharana, Koushik Dutta, Mayukh R. Gangopadhyay, Sukannya Bhattacharya","submitted_at":"2017-11-09T10:50:05Z","abstract_excerpt":"In models of inflation obtained from string compactification, moduli vacuum misalignment leads to an epoch in the post-inflationary history of the universe when the energy density is dominated by cold moduli particles. This effect leads to a modification in the number of $e$-foldings ($N_{\\rm pivot}$) between horizon exit of the CMB modes and the end of inflation. Taking K\\\"ahler moduli inflation as a prototype, the shift in $e$-foldings turns out to be a function of the model parameters which also determines the inflationary observables. We analyse this scenario numerically using publicly ava"},"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":"1711.04807","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-09T10:50:05Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"3aa6a5ce838f6a7d5e69519307a7d282886aa3c5ad051f76bf252b3c402b99a5","abstract_canon_sha256":"154867146aa6f0b3a35af98cf2f8f968f4fb5acc7661887aebd2ffa92f48d2b1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:40.069963Z","signature_b64":"nhWy4s1s0ZGsBek18JGwhUAPgmH4bCJ+lbJ27fIw6cY7NEHT+ydqYwULcVn3YMPZ51cFpFGnKH8WE+nq/B+cAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"958f47b0c53038da0c94a8d501381440348516a0cc7b9cf7c84abe53d2c150b5","last_reissued_at":"2026-05-18T00:11:40.069398Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:40.069398Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Confronting K\\\"ahler moduli inflation with CMB data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Anshuman Maharana, Koushik Dutta, Mayukh R. Gangopadhyay, Sukannya Bhattacharya","submitted_at":"2017-11-09T10:50:05Z","abstract_excerpt":"In models of inflation obtained from string compactification, moduli vacuum misalignment leads to an epoch in the post-inflationary history of the universe when the energy density is dominated by cold moduli particles. This effect leads to a modification in the number of $e$-foldings ($N_{\\rm pivot}$) between horizon exit of the CMB modes and the end of inflation. Taking K\\\"ahler moduli inflation as a prototype, the shift in $e$-foldings turns out to be a function of the model parameters which also determines the inflationary observables. We analyse this scenario numerically using publicly ava"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.04807","kind":"arxiv","version":2},"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":"1711.04807","created_at":"2026-05-18T00:11:40.069483+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.04807v2","created_at":"2026-05-18T00:11:40.069483+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.04807","created_at":"2026-05-18T00:11:40.069483+00:00"},{"alias_kind":"pith_short_12","alias_value":"SWHUPMGFGA4N","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_16","alias_value":"SWHUPMGFGA4NUDEU","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_8","alias_value":"SWHUPMGF","created_at":"2026-05-18T12:31:43.269735+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/SWHUPMGFGA4NUDEUVDKQCOAUIA","json":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA.json","graph_json":"https://pith.science/api/pith-number/SWHUPMGFGA4NUDEUVDKQCOAUIA/graph.json","events_json":"https://pith.science/api/pith-number/SWHUPMGFGA4NUDEUVDKQCOAUIA/events.json","paper":"https://pith.science/paper/SWHUPMGF"},"agent_actions":{"view_html":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA","download_json":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA.json","view_paper":"https://pith.science/paper/SWHUPMGF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.04807&json=true","fetch_graph":"https://pith.science/api/pith-number/SWHUPMGFGA4NUDEUVDKQCOAUIA/graph.json","fetch_events":"https://pith.science/api/pith-number/SWHUPMGFGA4NUDEUVDKQCOAUIA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA/action/storage_attestation","attest_author":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA/action/author_attestation","sign_citation":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA/action/citation_signature","submit_replication":"https://pith.science/pith/SWHUPMGFGA4NUDEUVDKQCOAUIA/action/replication_record"}},"created_at":"2026-05-18T00:11:40.069483+00:00","updated_at":"2026-05-18T00:11:40.069483+00:00"}