2001/06/08 by A. Peshier, B. Kampfer, Peshier, A. +4
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #High-Energy Particle Collisions Research #Pulsars and Gravitational Waves Research #Quantum Chromodynamics and Particle Interactions #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0106090
4 pages with figs (v2: minor grammatical changes)
openalex publication_date 2001/06/08 · arxiv created 2001/06/15 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Recent finite-temperature QCD lattice data are analyzed within a quasiparticle model, and extrapolated to nonzero chemical potential. Determined by the chiral transition temperature, the resulting equation of state of charge neutral, β-stable deconfined matter limits the mass and the size of quark stars.