Probing evolution of binaries influenced by the spin-orbit resonances

作者: Achamveedu Gopakumar , Anuradha Gupta

DOI: 10.1088/0264-9381/31/10/105017

关键词: Orbital angular momentum of lightGravitational waveAngular momentumAngular momentum of lightSpin–orbit interactionSpecific relative angular momentumPhysicsAngular momentum couplingTotal angular momentum quantum numberAstrophysicsQuantum mechanics

摘要: We evolve isolated comparable mass spinning compact binaries experiencing Schnittman's post-Newtonian spin-orbit resonances in an inertial frame associated with $j_0$, the initial direction of total angular momentum. argue that accurate gravitational wave (GW) measurements orientations two spins and orbital momentum from $j_0$ should allow us to distinguish between possible families resonances. Therefore, these have potential provide direct observational evidence binary formation scenarios. The above statements also apply for do not remain a resonant plane when they become detectable by GW interferometers. plane, characterized vanishing scalar triple product involving momentum, naturally appears one parameter family equilibrium solutions, discovered Schnittman. develop prescription compute time-domain inspiral templates residing configurations explore their preliminary data analysis consequences.

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