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Aligned spins: Orbital elements, decaying orbits, and last stable circular orbit to high post-Newtonian orders

机译:对齐的自旋:轨道元素,衰减轨道和最后稳定的圆形轨道,直至牛顿阶高

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摘要

In this paper, the quasi-Keplerian parameterization for the case that spins and orbital angular momentum in a compact binary system are aligned or anti-aligned with the orbital angular momentum vector is extended to 3PN point-mass, next-to-next-to-leading order spin-orbit, next-to-next-to-leading order spin(1)-spin(2) and next-to-leading order spin-squared dynamics in the conservative regime. In a further step, we use the expressions for the radiative multipole moments with spin to leading order linear and quadratic in both spins to compute radiation losses of the orbital binding energy and angular momentum. Orbital averaged expressions for the decay of energy and eccentricity are provided. An expression for the last stable circular orbit is given in terms of the angular velocity-type variable x.
机译:在本文中,将紧凑二元系统中的自旋和轨道角动量与轨道角动量矢量对准或反对准的情况的拟Keplerian参数化扩展到3PN点质量,次于下一个保守状态下,先导自旋轨道,先导自旋(1)-自旋(2)和先导自旋平方动力学。在进一步的步骤中,我们使用自旋在两个自旋中都具有自旋至超前级线性和二次方的辐射多极矩的表达式来计算轨道结合能和角动量的辐射损耗。提供了关于能量和离心率衰减的轨道平均表达式。根据角速度类型变量x给出最后一个稳定的圆形轨道的表达式。

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