{"paper":{"title":"Galactic Halos As Boson Stars","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"In-guy Koh, Jae-Weon Lee","submitted_at":"1995-07-23T05:34:58Z","abstract_excerpt":"We investigate the boson star with the self-interacting scalar field as a model of galactic halos. The model has slightly increasing rotation curves and allows wider ranges of the mass($m$) and coupling($\\lambda$) of the halo dark matter particle than the non-interacting model previously suggested(ref.\\cite{sin1}). Two quantities are related by $\\lambda^{\\frac{1}{2}} (m_p/m)^2\\st{>}{\\sim} 10^{50}$."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9507385","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":""},"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"}