{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:QB5ZN6BEAMNBYBHCRKZBX6QTXM","short_pith_number":"pith:QB5ZN6BE","schema_version":"1.0","canonical_sha256":"807b96f824031a1c04e28ab21bfa13bb106f134acfdea3ad181221270aaa5f84","source":{"kind":"arxiv","id":"2405.19389","version":2},"attestation_state":"computed","paper":{"title":"More Axion Stars from Strings","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Edward Hardy, Giovanni Villadoro, Marco Gorghetto","submitted_at":"2024-05-29T18:00:00Z","abstract_excerpt":"We show that if dark matter consists of QCD axions in the post-inflationary scenario more than ten percent of it efficiently collapses into Bose stars at matter-radiation equality. Such a result is mostly independent of the present uncertainties on the axion mass. This large population of solitons, with asteroid masses and Earth-Moon distance sizes, might plausibly survive until today, with potentially interesting implications for phenomenology and experimental searches."},"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":"2405.19389","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-05-29T18:00:00Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"61483c0394b669109984826c3019f8e3b77d4a440a19f753b91e894e4c93eba0","abstract_canon_sha256":"bf815309d09bca34df4369bd4d10a89e5fa1339aa8849452d97bccff52cb89ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:57:23.497741Z","signature_b64":"sPbBZ8t8ANFRGVUjD8HlicRVoJyOwSZCVkH+s/C2PqfDuuz2MZz6w84jLHalvMWxpw3EJSU/y7nXmR9f+cLRBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"807b96f824031a1c04e28ab21bfa13bb106f134acfdea3ad181221270aaa5f84","last_reissued_at":"2026-07-05T08:57:23.497399Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:57:23.497399Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"More Axion Stars from Strings","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Edward Hardy, Giovanni Villadoro, Marco Gorghetto","submitted_at":"2024-05-29T18:00:00Z","abstract_excerpt":"We show that if dark matter consists of QCD axions in the post-inflationary scenario more than ten percent of it efficiently collapses into Bose stars at matter-radiation equality. Such a result is mostly independent of the present uncertainties on the axion mass. This large population of solitons, with asteroid masses and Earth-Moon distance sizes, might plausibly survive until today, with potentially interesting implications for phenomenology and experimental searches."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.19389","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/2405.19389/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":"2405.19389","created_at":"2026-07-05T08:57:23.497456+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.19389v2","created_at":"2026-07-05T08:57:23.497456+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.19389","created_at":"2026-07-05T08:57:23.497456+00:00"},{"alias_kind":"pith_short_12","alias_value":"QB5ZN6BEAMNB","created_at":"2026-07-05T08:57:23.497456+00:00"},{"alias_kind":"pith_short_16","alias_value":"QB5ZN6BEAMNBYBHC","created_at":"2026-07-05T08:57:23.497456+00:00"},{"alias_kind":"pith_short_8","alias_value":"QB5ZN6BE","created_at":"2026-07-05T08:57:23.497456+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19439","citing_title":"From Rags to Jeans: Axion Miniclusters from Early matter domination","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2510.15046","citing_title":"Multi-species Dark Matter with Warmth and Randomness","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2510.17977","citing_title":"Growth of Structure in Multi-species Wave Dark Matter","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2506.12131","citing_title":"Early Growth of Structure in Warm Wave Dark Matter","ref_index":86,"is_internal_anchor":false},{"citing_arxiv_id":"2509.17059","citing_title":"Axions as Dark Matter, Dark Energy, and Dark Radiation","ref_index":118,"is_internal_anchor":false},{"citing_arxiv_id":"2601.00955","citing_title":"Is the Conventional Picture of Coherence Time Complete? Dark Matter Recoherence","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00103","citing_title":"Pre-inflationary QCD axion stars after moduli domination","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM","json":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM.json","graph_json":"https://pith.science/api/pith-number/QB5ZN6BEAMNBYBHCRKZBX6QTXM/graph.json","events_json":"https://pith.science/api/pith-number/QB5ZN6BEAMNBYBHCRKZBX6QTXM/events.json","paper":"https://pith.science/paper/QB5ZN6BE"},"agent_actions":{"view_html":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM","download_json":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM.json","view_paper":"https://pith.science/paper/QB5ZN6BE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.19389&json=true","fetch_graph":"https://pith.science/api/pith-number/QB5ZN6BEAMNBYBHCRKZBX6QTXM/graph.json","fetch_events":"https://pith.science/api/pith-number/QB5ZN6BEAMNBYBHCRKZBX6QTXM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM/action/storage_attestation","attest_author":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM/action/author_attestation","sign_citation":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM/action/citation_signature","submit_replication":"https://pith.science/pith/QB5ZN6BEAMNBYBHCRKZBX6QTXM/action/replication_record"}},"created_at":"2026-07-05T08:57:23.497456+00:00","updated_at":"2026-07-05T08:57:23.497456+00:00"}