2015/04/10 by A. Drago, Drago, A., Giuseppe Pagliara +2
Physics and Astronomy · #Astronomy #Astrophysics #Cosmology and Gravitation Theories #FOS: Physical sciences #Gamma-ray bursts and supernovae #Hadron #Nuclear Theory (nucl-th) #Particle physics #Physics #Pulsars and Gravitational Waves Research #Quark #Quark star #Solar and Stellar Astrophysics (astro-ph.SR) #Stars #Strange matter #astro-ph.SR #nucl-th
paper · pdf · doi:10.48550/arxiv.1504.02795
published in arXiv (Cornell University) (Cornell University) · 6 pages, 1 figure, contribution to Proceedings of the workshop "Compact Stars in the QCD phase diagram IV", Prerow, Germany, September 26 - 30, 2014
arxiv created 2015/04/10 · openalex publication_date 2015/04/10 · arxiv updated 2015/04/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We will review the approach used for studying the conversion of a hadronic star into a quark star based on the assumption of a infinitely thin combustion zone and we will discuss why, in this scheme, the combustion stops before the whole hadronic star is converted.