{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:4WKDZGK4PVV4THWVMYZA2QSSI4","short_pith_number":"pith:4WKDZGK4","schema_version":"1.0","canonical_sha256":"e5943c995c7d6bc99ed566320d425247044c09b347299babf0137b884209adab","source":{"kind":"arxiv","id":"astro-ph/0105564","version":3},"attestation_state":"computed","paper":{"title":"Quintessential Haloes around Galaxies","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph","authors_text":"Alexandre Arbey, Julien Lesgourgues, Pierre Salati","submitted_at":"2001-05-31T20:20:53Z","abstract_excerpt":"The nature of the dark matter that binds galaxies remains an open question. The favored candidate has been so far the neutralino. This massive species with evanescent interactions is now in difficulty. It would actually collapse in dense clumps and would therefore play havoc with the matter it is supposed to shepherd. We focus here on a massive and non-interacting charged scalar field as an alternate option to the astronomical missing mass. We investigate the classical solutions that describe the Bose condensate of such a field in gravitational interaction with matter. This simplistic model ac"},"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":"astro-ph/0105564","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-05-31T20:20:53Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"1e45fd8be199f3da82b6c40a362657f8bcf3eaa92962206da1213634bd2de186","abstract_canon_sha256":"26f22c6dc50b4b8f9a93f0eece08eef389298ff7a02e051e5b3f6b0f7b10b390"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:23:28.587067Z","signature_b64":"CeytJYtUWVlzHu82YTJ6cm1e7WubJEasUKBzt6vyHSbZXectSHGEZ1O1CdajZvznY8xiDyiTNoSU0NveIl5cAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e5943c995c7d6bc99ed566320d425247044c09b347299babf0137b884209adab","last_reissued_at":"2026-07-04T16:23:28.586527Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:23:28.586527Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quintessential Haloes around Galaxies","license":"","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph","authors_text":"Alexandre Arbey, Julien Lesgourgues, Pierre Salati","submitted_at":"2001-05-31T20:20:53Z","abstract_excerpt":"The nature of the dark matter that binds galaxies remains an open question. The favored candidate has been so far the neutralino. This massive species with evanescent interactions is now in difficulty. It would actually collapse in dense clumps and would therefore play havoc with the matter it is supposed to shepherd. We focus here on a massive and non-interacting charged scalar field as an alternate option to the astronomical missing mass. We investigate the classical solutions that describe the Bose condensate of such a field in gravitational interaction with matter. This simplistic model ac"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0105564","kind":"arxiv","version":3},"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/astro-ph/0105564/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":"astro-ph/0105564","created_at":"2026-07-04T16:23:28.586586+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0105564v3","created_at":"2026-07-04T16:23:28.586586+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0105564","created_at":"2026-07-04T16:23:28.586586+00:00"},{"alias_kind":"pith_short_12","alias_value":"4WKDZGK4PVV4","created_at":"2026-07-04T16:23:28.586586+00:00"},{"alias_kind":"pith_short_16","alias_value":"4WKDZGK4PVV4THWV","created_at":"2026-07-04T16:23:28.586586+00:00"},{"alias_kind":"pith_short_8","alias_value":"4WKDZGK4","created_at":"2026-07-04T16:23:28.586586+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.17083","citing_title":"Dark ages bounds on non-accreting massive compact halo objects","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4","json":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4.json","graph_json":"https://pith.science/api/pith-number/4WKDZGK4PVV4THWVMYZA2QSSI4/graph.json","events_json":"https://pith.science/api/pith-number/4WKDZGK4PVV4THWVMYZA2QSSI4/events.json","paper":"https://pith.science/paper/4WKDZGK4"},"agent_actions":{"view_html":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4","download_json":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4.json","view_paper":"https://pith.science/paper/4WKDZGK4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0105564&json=true","fetch_graph":"https://pith.science/api/pith-number/4WKDZGK4PVV4THWVMYZA2QSSI4/graph.json","fetch_events":"https://pith.science/api/pith-number/4WKDZGK4PVV4THWVMYZA2QSSI4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4/action/storage_attestation","attest_author":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4/action/author_attestation","sign_citation":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4/action/citation_signature","submit_replication":"https://pith.science/pith/4WKDZGK4PVV4THWVMYZA2QSSI4/action/replication_record"}},"created_at":"2026-07-04T16:23:28.586586+00:00","updated_at":"2026-07-04T16:23:28.586586+00:00"}