{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:W7P7AGU7ZL2YBH74IRPYLAFQ3X","short_pith_number":"pith:W7P7AGU7","schema_version":"1.0","canonical_sha256":"b7dff01a9fcaf5809ffc445f8580b0dde47e0776df07a53eb1c08bee5a0f19ea","source":{"kind":"arxiv","id":"1309.3122","version":2},"attestation_state":"computed","paper":{"title":"No-scale D-term inflation with stabilized moduli","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Clemens Wieck, Valerie Domcke, Wilfried Buchmuller","submitted_at":"2013-09-12T11:39:17Z","abstract_excerpt":"We study the consistency of hybrid inflation and moduli stabilization, using the Kallosh--Linde model as an example for the latter. We find that F-term hybrid inflation is not viable since inflationary trajectories are destabilized by tachyonic modes. On the other hand, D-term hybrid inflation is naturally compatible with moduli stabilization due to the absence of a large superpotential term during the inflationary phase. Our model turns out to be equivalent to superconformal D-term inflation and it therefore successfully accounts for the CMB data in the large-field regime. Supersymmetry break"},"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":"1309.3122","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-09-12T11:39:17Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"f0e4a44746095b37279bcfb3d19fe19df92912a4a4861b6183383fc3a94d7e86","abstract_canon_sha256":"9371cef82da795806ff9f076a78a24b727574146fa1e0e197385bfa274201ec6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:42.749520Z","signature_b64":"zEGdHZ9U02nucT7q294BZawljPG2TxUYztccxm2z+kQ0MPKdqszYWTsHuBAqW0oEDjpbVlMWcgqKAkUOK4tIBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b7dff01a9fcaf5809ffc445f8580b0dde47e0776df07a53eb1c08bee5a0f19ea","last_reissued_at":"2026-05-18T01:47:42.748904Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:42.748904Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"No-scale D-term inflation with stabilized moduli","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Clemens Wieck, Valerie Domcke, Wilfried Buchmuller","submitted_at":"2013-09-12T11:39:17Z","abstract_excerpt":"We study the consistency of hybrid inflation and moduli stabilization, using the Kallosh--Linde model as an example for the latter. We find that F-term hybrid inflation is not viable since inflationary trajectories are destabilized by tachyonic modes. On the other hand, D-term hybrid inflation is naturally compatible with moduli stabilization due to the absence of a large superpotential term during the inflationary phase. Our model turns out to be equivalent to superconformal D-term inflation and it therefore successfully accounts for the CMB data in the large-field regime. Supersymmetry break"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.3122","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":"1309.3122","created_at":"2026-05-18T01:47:42.748992+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.3122v2","created_at":"2026-05-18T01:47:42.748992+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.3122","created_at":"2026-05-18T01:47:42.748992+00:00"},{"alias_kind":"pith_short_12","alias_value":"W7P7AGU7ZL2Y","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_16","alias_value":"W7P7AGU7ZL2YBH74","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_8","alias_value":"W7P7AGU7","created_at":"2026-05-18T12:28:04.890932+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/W7P7AGU7ZL2YBH74IRPYLAFQ3X","json":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X.json","graph_json":"https://pith.science/api/pith-number/W7P7AGU7ZL2YBH74IRPYLAFQ3X/graph.json","events_json":"https://pith.science/api/pith-number/W7P7AGU7ZL2YBH74IRPYLAFQ3X/events.json","paper":"https://pith.science/paper/W7P7AGU7"},"agent_actions":{"view_html":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X","download_json":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X.json","view_paper":"https://pith.science/paper/W7P7AGU7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.3122&json=true","fetch_graph":"https://pith.science/api/pith-number/W7P7AGU7ZL2YBH74IRPYLAFQ3X/graph.json","fetch_events":"https://pith.science/api/pith-number/W7P7AGU7ZL2YBH74IRPYLAFQ3X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X/action/storage_attestation","attest_author":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X/action/author_attestation","sign_citation":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X/action/citation_signature","submit_replication":"https://pith.science/pith/W7P7AGU7ZL2YBH74IRPYLAFQ3X/action/replication_record"}},"created_at":"2026-05-18T01:47:42.748992+00:00","updated_at":"2026-05-18T01:47:42.748992+00:00"}