{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:NLHWRDCE3WENIFCXTKMNTDBTGQ","short_pith_number":"pith:NLHWRDCE","schema_version":"1.0","canonical_sha256":"6acf688c44dd88d414579a98d98c333400dbebd6cd056d1b236bf9c68e46503d","source":{"kind":"arxiv","id":"1512.04224","version":2},"attestation_state":"computed","paper":{"title":"Vacuum Selection on Axionic Landscapes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Gaoyuan Wang, Thorsten Battefeld","submitted_at":"2015-12-14T09:21:46Z","abstract_excerpt":"We compute the distribution of minima that are reached dynamically on multi-field axionic landscapes, both numerically and analytically. Such landscapes are well suited for inflationary model building due to the presence of shift symmetries and possible alignment effects (the KNP mechanism). The resulting distribution of dynamically reached minima differs considerably from the naive expectation based on counting all vacua. These differences are more pronounced in the presence of many fields due to dynamical selection effects: while low lying minima are preferred as fields roll down the potenti"},"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":"1512.04224","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-12-14T09:21:46Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"c9bb2a001dd4a3d49232b7c807ed0c0b6f4d861761cd0c5c8b231d90493b4798","abstract_canon_sha256":"c4ad2c81d5021953daf79ac5e08544d14401ec4641baa3ef37b2c71c72972747"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:59.880188Z","signature_b64":"EfnIZr809kRZm9tQHZDFeU8pC0kPiDQnGup/eeU4pFuKCYhuwFqUElYlilcEKXaHa+CzX1WcVKgR9GUkVbX5AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6acf688c44dd88d414579a98d98c333400dbebd6cd056d1b236bf9c68e46503d","last_reissued_at":"2026-05-18T01:16:59.879458Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:59.879458Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vacuum Selection on Axionic Landscapes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-th","authors_text":"Gaoyuan Wang, Thorsten Battefeld","submitted_at":"2015-12-14T09:21:46Z","abstract_excerpt":"We compute the distribution of minima that are reached dynamically on multi-field axionic landscapes, both numerically and analytically. Such landscapes are well suited for inflationary model building due to the presence of shift symmetries and possible alignment effects (the KNP mechanism). The resulting distribution of dynamically reached minima differs considerably from the naive expectation based on counting all vacua. These differences are more pronounced in the presence of many fields due to dynamical selection effects: while low lying minima are preferred as fields roll down the potenti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.04224","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":"1512.04224","created_at":"2026-05-18T01:16:59.879586+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.04224v2","created_at":"2026-05-18T01:16:59.879586+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.04224","created_at":"2026-05-18T01:16:59.879586+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLHWRDCE3WEN","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLHWRDCE3WENIFCX","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLHWRDCE","created_at":"2026-05-18T12:29:32.376354+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.30259","citing_title":"Late-time Quantum Vacuum Decay and its Cosmological Implications","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ","json":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ.json","graph_json":"https://pith.science/api/pith-number/NLHWRDCE3WENIFCXTKMNTDBTGQ/graph.json","events_json":"https://pith.science/api/pith-number/NLHWRDCE3WENIFCXTKMNTDBTGQ/events.json","paper":"https://pith.science/paper/NLHWRDCE"},"agent_actions":{"view_html":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ","download_json":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ.json","view_paper":"https://pith.science/paper/NLHWRDCE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.04224&json=true","fetch_graph":"https://pith.science/api/pith-number/NLHWRDCE3WENIFCXTKMNTDBTGQ/graph.json","fetch_events":"https://pith.science/api/pith-number/NLHWRDCE3WENIFCXTKMNTDBTGQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ/action/storage_attestation","attest_author":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ/action/author_attestation","sign_citation":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ/action/citation_signature","submit_replication":"https://pith.science/pith/NLHWRDCE3WENIFCXTKMNTDBTGQ/action/replication_record"}},"created_at":"2026-05-18T01:16:59.879586+00:00","updated_at":"2026-05-18T01:16:59.879586+00:00"}