{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:MW7UUCLEB4EHFS2VUIEOXAH35G","short_pith_number":"pith:MW7UUCLE","schema_version":"1.0","canonical_sha256":"65bf4a09640f0872cb55a208eb80fbe9800c6ae021bcd4fff84df7ed5afbc185","source":{"kind":"arxiv","id":"1811.03771","version":2},"attestation_state":"computed","paper":{"title":"Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Hoang Nhan Luu, S. -H. Henry Tye, Tom Broadhurst","submitted_at":"2018-11-09T04:48:22Z","abstract_excerpt":"An ultralight scalar boson with mass $m_1 \\simeq 10^{-22}$ eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in String Theory, with multiple light axions predicted in this context. We examine the possibility of soliton structures over a wide range of scales, accounting for galaxy core masses and the common presence of nuclear star clusters. We present a diagnostic soliton core mass-radius plot that provides a global view, indicating the existence of an additional axio"},"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":"1811.03771","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-09T04:48:22Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"45ff8d9fdd52bf35d8c16e378109d91f59fd13b41582f84bf685dda2639679f0","abstract_canon_sha256":"7725c78166d1f402832a323b71c1ca221e5a428ad266ea85dc659d8e390ee8f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:17:06.702286Z","signature_b64":"DL36/36lsfwn38wViAYKqAdpBRVywHPMyK331Si3FQlBR2V+kYbH8yl21j2TIgpNM2cC9Y3kpzeMdaked3c1Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65bf4a09640f0872cb55a208eb80fbe9800c6ae021bcd4fff84df7ed5afbc185","last_reissued_at":"2026-07-05T02:17:06.701840Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:17:06.701840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiple Ultralight Axionic Wave Dark Matter and Astronomical Structures","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Hoang Nhan Luu, S. -H. Henry Tye, Tom Broadhurst","submitted_at":"2018-11-09T04:48:22Z","abstract_excerpt":"An ultralight scalar boson with mass $m_1 \\simeq 10^{-22}$ eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in String Theory, with multiple light axions predicted in this context. We examine the possibility of soliton structures over a wide range of scales, accounting for galaxy core masses and the common presence of nuclear star clusters. We present a diagnostic soliton core mass-radius plot that provides a global view, indicating the existence of an additional axio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.03771","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/1811.03771/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":"1811.03771","created_at":"2026-07-05T02:17:06.701904+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.03771v2","created_at":"2026-07-05T02:17:06.701904+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.03771","created_at":"2026-07-05T02:17:06.701904+00:00"},{"alias_kind":"pith_short_12","alias_value":"MW7UUCLEB4EH","created_at":"2026-07-05T02:17:06.701904+00:00"},{"alias_kind":"pith_short_16","alias_value":"MW7UUCLEB4EHFS2V","created_at":"2026-07-05T02:17:06.701904+00:00"},{"alias_kind":"pith_short_8","alias_value":"MW7UUCLE","created_at":"2026-07-05T02:17:06.701904+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.12589","citing_title":"Tunneling and tidal stripping in multifield ultralight dark matter halos","ref_index":37,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G","json":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G.json","graph_json":"https://pith.science/api/pith-number/MW7UUCLEB4EHFS2VUIEOXAH35G/graph.json","events_json":"https://pith.science/api/pith-number/MW7UUCLEB4EHFS2VUIEOXAH35G/events.json","paper":"https://pith.science/paper/MW7UUCLE"},"agent_actions":{"view_html":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G","download_json":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G.json","view_paper":"https://pith.science/paper/MW7UUCLE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.03771&json=true","fetch_graph":"https://pith.science/api/pith-number/MW7UUCLEB4EHFS2VUIEOXAH35G/graph.json","fetch_events":"https://pith.science/api/pith-number/MW7UUCLEB4EHFS2VUIEOXAH35G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G/action/storage_attestation","attest_author":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G/action/author_attestation","sign_citation":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G/action/citation_signature","submit_replication":"https://pith.science/pith/MW7UUCLEB4EHFS2VUIEOXAH35G/action/replication_record"}},"created_at":"2026-07-05T02:17:06.701904+00:00","updated_at":"2026-07-05T02:17:06.701904+00:00"}