论文标题
palatini $ f（r）$重力的白矮星的冷却过程
Cooling Process of White Dwarf Stars in Palatini $f(R)$ Gravity
论文作者
论文摘要
白色矮星的简单冷却模型在Palatini $ f（r）$ gravity中重新分析。修饰的重力会影响白矮结构，因此会影响其年龄。我们发现，与牛顿型模型相比，所得的超级chandrasekhar白矮人需要更多的时间来冷却。
A simple cooling model of white dwarf stars is re-analyzed in Palatini $f(R)$ gravity. Modified gravity affects the white dwarf structures and consequently their ages. We find that the resulting super-Chandrasekhar white dwarfs need more time to cool down than sub-Chandrasekhar ones, or when compared to the Newtonian models.
