Quasi-equilibriums of magnetized binary neutron stars and initial data for numerical relativity simulations

导出了磁化双星中子星准平衡的计算公式及其广义热力学定律。我们开发了一个新的程序，Cocal-Compact天体计算器，用于计算准平衡中致密天体的结构，并成功地计算了例如三轴形变的快速旋转中子星。计算了双星中子星的准平衡解，并将其作为模拟双星的初始数据集。对模拟得到的重力波形进行了分析。

Formulations for computing quasi-equilibrium of magnetized binary neutron stars and their generalized thermodynamic laws are derived. We develop a new code, Cocal-Compact Object CALculator, to calculate structures of compact objects in quasi-equilibriums, and successfully compute, for example, triaxially deformed rapidly rotating neutron stars. Quasi-equilibrium solutions for binary neutron stars are also calculated, and they are provided as initial data sets for simulations of binary inspirals. Gravitational waveforms obtained the simulations are analyzed.