Signatures of QCD Phase Transition in a Newborn Compact Star
Wong, K. -W. · Chu, M. -C.
Original · EN
We study the scenario that a new born strange quark star cools to the Quantum ChromoDynamics (QCD) phase transition temperature and converts to a neutron star, and we calculate the evolution of temperature and luminosity of the compact star. We argue that the conversion energy released can be of the order 10⁵³ erg. We also propose that a second neutrino burst will be emitted at the completion of this phase transition.
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