{"paper":{"title":"Energy release due to antineutrino untrapping from hot quark stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Blaschke, D. N. Aguilera, H. Grigorian","submitted_at":"2004-02-03T17:38:08Z","abstract_excerpt":"An equation of state for 2-flavor quark matter (QM) with diquark condensation under the conditions for compact stars -$\\beta$-equilibrium, charge and color neutrality- is presented. Trapped antineutrinos prevent the formation of the diquark condensate at moderate densities above a critical value of the antineutrino chemical potential $\\mu_{\\bar \\nu_e}^c$. The following consequences are presented: 1) The star develops a 2-phase structure ($\\mu_{\\bar \\nu_e}\\geq \\mu_{\\bar \\nu_e}^c$): a color superconducting QM core and a normal QM shell. 2)During the cooling, when the temperature is small enough "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0402073","kind":"arxiv","version":1},"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"}