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astro-ph.HE2026
Emission and cooling of a newborn quark star
Mikalai Prakapenia, Gregory Vereshchagin
It has long been believed that newborn quark stars are inefficient emitters because the quark plasma frequency is so high that it suppresses electromagnetic radiation across the en…
astro-ph.HE2026
Pair luminosity and cooling of newborn strange star: Color-flavor-locked and two-flavor color superconducting quarks
Mikalai Prakapenia, Cheng-Jun Xia, Gregory Vereshchagin
Following the previous wor k[1] here we consider early thermal evolution of hot strange stars made of color superconducting quarks in two different pairing states: two-flavor color…