论文标题
用微观方程式冷却混合中性星星
Cooling of hybrid neutron stars with microscopic equations of state
论文作者
论文摘要
我们对混合中性恒星的冷却建模，结合了与不同夸克模型的Brueckner-Hartree-fock方法中的微观核方程式。然后，我们分析了由不同模型预测的中子星冷却曲线，并挑出了首选。我们发现，在我们的情况下可以排除中子P波配对的可能性。
We model the cooling of hybrid neutron stars combining a microscopic nuclear equation of state in the Brueckner-Hartree-Fock approach with different quark models. We then analyze the neutron star cooling curves predicted by the different models and single out the preferred ones. We find that the possibility of neutron p-wave pairing can be excluded in our scenario.
