QCD phase transition and explosive phenomena in the universe

在致密恒星冷却曲线的研究中，我们考虑了夸克星和/或奇异星的形成。然后我们研究了中微子特殊的发射过程对超新星爆炸的影响。此外，在这10年中，我们将我们的公式应用于超新星遗迹CaA中的一颗致密恒星。因此，我们可以通过考虑相变到超流体状态时伴随的中微子发射来解释冷却曲线。

In the study of cooling curves of compact stars, we have considered the cases of the formation of quark stars and/or strange stars. Then we investigate the effects of particular emission processes of neutrinos on the supernova explosions. Furthermore, we applied our formulations to a compact star in the supernova remnant Cas A in these 10 years. As a consequence, we can explain the cooling curve by including the neutrino emission accompanied to the phase transition to super fluid state.