质子中子星结构性质的最低阶约束变分计算
Lowest Order Constrained Variational Calculation of Structure Properties of Protoneutron Star
摘要：
利用最低阶约束变分方法计算了质子中子星的状态方程、最大质量、半径和温度分布等结构性质。结果表明，质子中子星的质量和半径随着熵和温度的降低而减小。对于质子中子星，它表明，温度几乎是恒定的核心和地壳附近迅速下降。
英文摘要：
We calculate the structure properties of protoneutron star such as equation of state, maximum mass, radius and temperature profile using the lowest order constrained variational method. We show that the mass and radius of protoneutron star decrease by decreasing both entropy and temperature. For the protoneutron star, it is shown that the temperature is nearly constant in the core and drops rapidly near the crust.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
