{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:2RVL5G6342HHBK4CZ7COLKMDFD","short_pith_number":"pith:2RVL5G63","schema_version":"1.0","canonical_sha256":"d46abe9bdbe68e70ab82cfc4e5a98328fdbc70e54ced7d70ebb183e3b7c61ea4","source":{"kind":"arxiv","id":"1609.00364","version":2},"attestation_state":"computed","paper":{"title":"Inflation from Nilpotent K\\\"ahler Corrections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Evan McDonough, Marco Scalisi","submitted_at":"2016-09-01T19:50:52Z","abstract_excerpt":"We develop a new class of supergravity cosmological models where inflation is induced by terms in the K\\\"ahler potential which mix a nilpotent superfield $S$ with a chiral sector $\\Phi$. As the new terms are non-(anti)holomorphic, and hence cannot be removed by a K\\\"ahler transformation, these models are intrinsically K\\\"ahler potential driven. Such terms could arise for example due to a backreaction of an anti-D3 brane on the string theory bulk geometry. We show that this mechanism is very general and allows for a unified description of inflation and dark energy, with controllable SUSY breaki"},"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":"1609.00364","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2016-09-01T19:50:52Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ph"],"title_canon_sha256":"dcec8069fd9fad8530d6440d692c6ec833391e05c118fc403f3771bfff74e515","abstract_canon_sha256":"16c3eccc55d5cb9efbe7dd58f4bfbe97ff30d1e26d41f449abbec06d0d4dd3c1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:58:03.828141Z","signature_b64":"B9ISLiLuc207Em49rXhwOSfsAyijylR3kBSglEzud9j8U5jUbB+uZS0jKpUuABtoO0/pKHaWAdsZ1Mnt8RvNBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d46abe9bdbe68e70ab82cfc4e5a98328fdbc70e54ced7d70ebb183e3b7c61ea4","last_reissued_at":"2026-05-18T00:58:03.827657Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:58:03.827657Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inflation from Nilpotent K\\\"ahler Corrections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Evan McDonough, Marco Scalisi","submitted_at":"2016-09-01T19:50:52Z","abstract_excerpt":"We develop a new class of supergravity cosmological models where inflation is induced by terms in the K\\\"ahler potential which mix a nilpotent superfield $S$ with a chiral sector $\\Phi$. As the new terms are non-(anti)holomorphic, and hence cannot be removed by a K\\\"ahler transformation, these models are intrinsically K\\\"ahler potential driven. Such terms could arise for example due to a backreaction of an anti-D3 brane on the string theory bulk geometry. We show that this mechanism is very general and allows for a unified description of inflation and dark energy, with controllable SUSY breaki"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.00364","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":"1609.00364","created_at":"2026-05-18T00:58:03.827735+00:00"},{"alias_kind":"arxiv_version","alias_value":"1609.00364v2","created_at":"2026-05-18T00:58:03.827735+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.00364","created_at":"2026-05-18T00:58:03.827735+00:00"},{"alias_kind":"pith_short_12","alias_value":"2RVL5G6342HH","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"2RVL5G6342HHBK4C","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"2RVL5G63","created_at":"2026-05-18T12:29:55.572404+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.02539","citing_title":"Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy","ref_index":59,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD","json":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD.json","graph_json":"https://pith.science/api/pith-number/2RVL5G6342HHBK4CZ7COLKMDFD/graph.json","events_json":"https://pith.science/api/pith-number/2RVL5G6342HHBK4CZ7COLKMDFD/events.json","paper":"https://pith.science/paper/2RVL5G63"},"agent_actions":{"view_html":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD","download_json":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD.json","view_paper":"https://pith.science/paper/2RVL5G63","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1609.00364&json=true","fetch_graph":"https://pith.science/api/pith-number/2RVL5G6342HHBK4CZ7COLKMDFD/graph.json","fetch_events":"https://pith.science/api/pith-number/2RVL5G6342HHBK4CZ7COLKMDFD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD/action/storage_attestation","attest_author":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD/action/author_attestation","sign_citation":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD/action/citation_signature","submit_replication":"https://pith.science/pith/2RVL5G6342HHBK4CZ7COLKMDFD/action/replication_record"}},"created_at":"2026-05-18T00:58:03.827735+00:00","updated_at":"2026-05-18T00:58:03.827735+00:00"}