{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:EPG2HMJODP2JBIHRFQC5SOM4IV","short_pith_number":"pith:EPG2HMJO","schema_version":"1.0","canonical_sha256":"23cda3b12e1bf490a0f12c05d9399c454321300d7e73d4fea07d8c6ee6c307d3","source":{"kind":"arxiv","id":"2403.17697","version":2},"attestation_state":"computed","paper":{"title":"Cosmology of axion dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Ciaran A. J. O'Hare","submitted_at":"2024-03-26T13:37:47Z","abstract_excerpt":"I present an introduction and topical review on axions as a dark matter candidate. Emphasis is placed on issues surrounding the cosmology of axion dark matter that are relevant for present-day searches, including: early-Universe production mechanisms, predictions of the axion mass, bounds on axion properties derived from cosmological data, as well as the direct and indirect detection of relic axion populations."},"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":"2403.17697","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-03-26T13:37:47Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"bb6a9c82e70d9de020b532fdf8aac48ad1ff415fccedd05d1c873f100c68c928","abstract_canon_sha256":"3a343e9c1e1cb2bb590573ca14e68f42096be22e72930b8ee0e32c3ea2a894ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:23:20.393826Z","signature_b64":"UZC8Y2LTRbrguz04Il2G4is2uMBawiQG2Lt+avYdM/H+dRgqdFBpRv7S3pRxfygGGBkHNnVBAr08hQUwVaWJBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23cda3b12e1bf490a0f12c05d9399c454321300d7e73d4fea07d8c6ee6c307d3","last_reissued_at":"2026-07-05T08:23:20.393365Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:23:20.393365Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmology of axion dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Ciaran A. J. O'Hare","submitted_at":"2024-03-26T13:37:47Z","abstract_excerpt":"I present an introduction and topical review on axions as a dark matter candidate. Emphasis is placed on issues surrounding the cosmology of axion dark matter that are relevant for present-day searches, including: early-Universe production mechanisms, predictions of the axion mass, bounds on axion properties derived from cosmological data, as well as the direct and indirect detection of relic axion populations."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.17697","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.17697/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":"2403.17697","created_at":"2026-07-05T08:23:20.393421+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.17697v2","created_at":"2026-07-05T08:23:20.393421+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.17697","created_at":"2026-07-05T08:23:20.393421+00:00"},{"alias_kind":"pith_short_12","alias_value":"EPG2HMJODP2J","created_at":"2026-07-05T08:23:20.393421+00:00"},{"alias_kind":"pith_short_16","alias_value":"EPG2HMJODP2JBIHR","created_at":"2026-07-05T08:23:20.393421+00:00"},{"alias_kind":"pith_short_8","alias_value":"EPG2HMJO","created_at":"2026-07-05T08:23:20.393421+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":30,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07158","citing_title":"Weakly supervised machine learning for model-agnostic searches of new phenomena in the $\\gamma$-ray sky","ref_index":39,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20524","citing_title":"String Axiverse Enhancement of Superradiant Dark Matter Production","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2606.17176","citing_title":"Tracing Ultra Light Axions in Post-reionization, Lyman-$\\alpha$ and CMB Missions","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2606.07749","citing_title":"Flavor phenomenology of light dark particles","ref_index":199,"is_internal_anchor":false},{"citing_arxiv_id":"2607.00072","citing_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06484","citing_title":"Phenomenology of Inflaton-Driven Early QCD Confinement and Solution to Axion Isocurvature Problem","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02706","citing_title":"Majoron Dark Matter, High-Scale Seesaw, and Leptogenesis","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28488","citing_title":"Dark energy from neutrino interactions in Unimodular Gravity","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15192","citing_title":"Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2606.31476","citing_title":"Landau-Zener formula and resonant axion conversion in neutron star magnetospheres","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30739","citing_title":"Fuzzy Dark Matter Halo Mass Functions at Cosmic Dawn","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2510.22592","citing_title":"Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2510.17977","citing_title":"Growth of Structure in Multi-species Wave Dark Matter","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15192","citing_title":"Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21092","citing_title":"Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17178","citing_title":"An EFT Map of Axion Dark Radiation from Reheating","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17211","citing_title":"Constraints on Self-Interacting Fuzzy Dark Matter from the Stellar Kinematics of the Dwarf Galaxy Leo II","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15261","citing_title":"Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2506.12131","citing_title":"Early Growth of Structure in Warm Wave Dark Matter","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2508.12722","citing_title":"Completing Axion Double Level Crossings","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2510.10708","citing_title":"Multimodal axion emissions from Abelian-Higgs cosmic strings","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2511.10617","citing_title":"Dark Matter from Holography","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2511.13815","citing_title":"Stripped-Envelope Supernovae for QCD Axion Detection","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2603.10189","citing_title":"Searching for axions with time resolved pulsar polarimetry","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15192","citing_title":"Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus","ref_index":6,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV","json":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV.json","graph_json":"https://pith.science/api/pith-number/EPG2HMJODP2JBIHRFQC5SOM4IV/graph.json","events_json":"https://pith.science/api/pith-number/EPG2HMJODP2JBIHRFQC5SOM4IV/events.json","paper":"https://pith.science/paper/EPG2HMJO"},"agent_actions":{"view_html":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV","download_json":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV.json","view_paper":"https://pith.science/paper/EPG2HMJO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.17697&json=true","fetch_graph":"https://pith.science/api/pith-number/EPG2HMJODP2JBIHRFQC5SOM4IV/graph.json","fetch_events":"https://pith.science/api/pith-number/EPG2HMJODP2JBIHRFQC5SOM4IV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV/action/storage_attestation","attest_author":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV/action/author_attestation","sign_citation":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV/action/citation_signature","submit_replication":"https://pith.science/pith/EPG2HMJODP2JBIHRFQC5SOM4IV/action/replication_record"}},"created_at":"2026-07-05T08:23:20.393421+00:00","updated_at":"2026-07-05T08:23:20.393421+00:00"}