Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
复制标题
从二元螺旋到后牛顿三阶引力波通量的自旋诱发多极矩
DOI：
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发表时间：
2010
期刊：
影响因子：
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通讯作者：
I. Rothstein
中科院分区：
文献类型：
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作者：
Rafael A. Porto;A. Ross;I. Rothstein
使用有效场论技术，我们计算的源多极矩需要获得的自旋贡献的引力波辐射的功率从螺旋紧凑的二进制文件的第三后牛顿顺序（3PN）。多极子线性地和二次地依赖于自旋，并且包括自旋（1）自旋（2）和自旋（1）自旋（1）分量。本文中的结果提供了最后一个缺失的成分，需要确定的相位演变到3PN，包括所有的自旋效应，我们将在一个单独的文件中报告。
Using effective field theory techniques we calculate the source multipole moments needed to obtain the spin contributions to the power radiated in gravitational waves from inspiralling compact binaries to third Post-Newtonian order (3PN). The multipoles depend linearly and quadratically on the spins and include both spin(1)spin(2) and spin(1)spin(1) components. The results in this paper provide the last missing ingredient required to determine the phase evolution to 3PN including all spin effects which we will report in a separate paper.