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Signatures of QCD Phase Transition in a Newborn Compact Star

K. -W. Wong·M. -C. Chu
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Abstract

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 $10^{53}$ erg. We also propose that a second neutrino burst will be emitted at the completion of this phase transition.

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BibTeXRIS

K. -W. Wong, M. -C. Chu. 2004-04-19. Signatures of QCD Phase Transition in a Newborn Compact Star. https://doi.org/10.1111/j.1365-2966.2004.07849.x

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