{"paper":{"title":"Influence of the stiffness of the equation of state and in-medium effects on the cooling of compact stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"D. Blaschke, D. N. Voskresensky, H. Grigorian","submitted_at":"2016-03-08T19:36:45Z","abstract_excerpt":"Measurements demonstrate the existence of compact stars with masses in a broad range from 1.2 to 2 $M_\\odot$. The most massive of these objects might be hybrid stars. To fulfill the constraint $M_{\\rm max}>2~M_{\\odot}$ with a reserve we exploit the stiff DD2 hadronic equation of state (EoS) without and with excluded volume (DD2vex) correction, which produce maximum neutron star masses of $M_{\\rm max} = 2.43~M_{\\odot}$ and $2.70~M_{\\odot}$, respectively. We show that the stiffness of the EoS does not preclude an explanation of the whole set of cooling data within \"nuclear medium cooling\" scenar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.02634","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"}