论文标题
密集物质对二进制中子恒星灵感和重力波的潮汐变形的影响
Effects of dense matter on the tidal deformations of binary neutron star inspirals and gravitational waves
论文作者
论文摘要
使用一组统一状态方程研究了密集物质特性在二进制中子星的潮汐变形和重力波形上的作用。基于核能密度的功能理论，这些状态方程在热力学上提供了对恒星所有区域的热力学一致处理，并使用精确的功能来计算，这些功能适合实验和理论核数据。
The role of the dense matter properties on the tidal deformability and gravitational waveforms of binary neutron stars is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equations of state provide a thermodynamically consistent treatment of all regions of the stars and were calculated using functionals that were precision fitted to experimental and theoretical nuclear data.
