{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:W3CNQSS2M4S2JBAQX2C56FLWO2","short_pith_number":"pith:W3CNQSS2","schema_version":"1.0","canonical_sha256":"b6c4d84a5a6725a48410be85df157676ab2c4f9431adc7082574d777b9a26701","source":{"kind":"arxiv","id":"2412.12012","version":1},"attestation_state":"computed","paper":{"title":"Fuzzy Axions and Associated Relics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Andreas Schachner, David J. E. Marsh, Elijah Sheridan, Federico Carta, Keir K. Rogers, Liam McAllister, Mudit Jain, Naomi Gendler, Nicole Righi","submitted_at":"2024-12-16T17:37:49Z","abstract_excerpt":"We study fuzzy axion dark matter in type IIB string theory, for axions descending from the Ramond-Ramond four-form in compactifications on orientifolds of Calabi-Yau hypersurfaces. Such models can be tested by cosmological measurements if a significant relic abundance of fuzzy dark matter arises, which we argue is most common in models with small numbers of axions. We construct a topologically exhaustive ensemble of more than 350,000 Calabi-Yau compactifications yielding up to seven axions, and in this setting we perform a systematic analysis of misalignment production of fuzzy dark matter. In"},"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":"2412.12012","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-12-16T17:37:49Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"aff14847bdaf5c9b66864ed93250a0b5c48cc528da71d4d8a90f9cccea1e17f7","abstract_canon_sha256":"6d1eb95ac83c85329d34380e05c4b6e74bb7105b839609f379ddf2ca3d6db901"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:49:55.505933Z","signature_b64":"exispLAkN3LaAJsHEGDs7SfNzqd1zmj0kZRo07XuizJ2k5t1QBfk/oPX85SDB7GYFutyFMBYnQJH0wh4lXCwDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b6c4d84a5a6725a48410be85df157676ab2c4f9431adc7082574d777b9a26701","last_reissued_at":"2026-07-05T09:49:55.505371Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:49:55.505371Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fuzzy Axions and Associated Relics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"hep-th","authors_text":"Andreas Schachner, David J. E. Marsh, Elijah Sheridan, Federico Carta, Keir K. Rogers, Liam McAllister, Mudit Jain, Naomi Gendler, Nicole Righi","submitted_at":"2024-12-16T17:37:49Z","abstract_excerpt":"We study fuzzy axion dark matter in type IIB string theory, for axions descending from the Ramond-Ramond four-form in compactifications on orientifolds of Calabi-Yau hypersurfaces. Such models can be tested by cosmological measurements if a significant relic abundance of fuzzy dark matter arises, which we argue is most common in models with small numbers of axions. We construct a topologically exhaustive ensemble of more than 350,000 Calabi-Yau compactifications yielding up to seven axions, and in this setting we perform a systematic analysis of misalignment production of fuzzy dark matter. In"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.12012","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2412.12012/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2412.12012","created_at":"2026-07-05T09:49:55.505435+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.12012v1","created_at":"2026-07-05T09:49:55.505435+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.12012","created_at":"2026-07-05T09:49:55.505435+00:00"},{"alias_kind":"pith_short_12","alias_value":"W3CNQSS2M4S2","created_at":"2026-07-05T09:49:55.505435+00:00"},{"alias_kind":"pith_short_16","alias_value":"W3CNQSS2M4S2JBAQ","created_at":"2026-07-05T09:49:55.505435+00:00"},{"alias_kind":"pith_short_8","alias_value":"W3CNQSS2","created_at":"2026-07-05T09:49:55.505435+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.20826","citing_title":"Counting axions with IAXO","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12549","citing_title":"Tachyonic Encore: A universal shift of inflationary observables","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2606.09982","citing_title":"Testing F-theory GUTs with the Axiverse","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06410","citing_title":"The Atacama Cosmology Telescope: Probing new signatures of ultralight axions with gravitational lensing","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2605.22912","citing_title":"Sharpening the Supersymmetric Axion Weak Gravity Conjecture","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2510.17977","citing_title":"Growth of Structure in Multi-species Wave Dark Matter","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2511.00157","citing_title":"Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09081","citing_title":"Probing High-Quality Axions with Gravitational Waves","ref_index":86,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2","json":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2.json","graph_json":"https://pith.science/api/pith-number/W3CNQSS2M4S2JBAQX2C56FLWO2/graph.json","events_json":"https://pith.science/api/pith-number/W3CNQSS2M4S2JBAQX2C56FLWO2/events.json","paper":"https://pith.science/paper/W3CNQSS2"},"agent_actions":{"view_html":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2","download_json":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2.json","view_paper":"https://pith.science/paper/W3CNQSS2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.12012&json=true","fetch_graph":"https://pith.science/api/pith-number/W3CNQSS2M4S2JBAQX2C56FLWO2/graph.json","fetch_events":"https://pith.science/api/pith-number/W3CNQSS2M4S2JBAQX2C56FLWO2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2/action/storage_attestation","attest_author":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2/action/author_attestation","sign_citation":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2/action/citation_signature","submit_replication":"https://pith.science/pith/W3CNQSS2M4S2JBAQX2C56FLWO2/action/replication_record"}},"created_at":"2026-07-05T09:49:55.505435+00:00","updated_at":"2026-07-05T09:49:55.505435+00:00"}