Speaker
Gregory Vereshchagin
(ICRANet)
Description
Cooling of newborn quark stars occurs through neutrino emission from their interiors and photon and electron-positron pairs emission from their surface. We will discuss the cooling process of bare hot quark stars with particular emphasis on luminosity and spectrum, providing input for ongoing observational programs in X-rays.
Authors
Gregory Vereshchagin
(ICRANet)
Mikalai Prakapenia