由引力波引起的加速和回旋辐射
Acceleration and Cyclotron Radiation, Induced by Gravitational Waves
摘要：
在广义相对论的线性近似下，导出了在磁场中运动的带电粒子对入射引力波的响应方程。我们简要地讨论了几个天体物理的应用导出的公式考虑到波和粒子的运动之间的共振发生在$ω_g=2Ω$，每当GW是平行于恒定的磁场。在GW垂直于恒定磁场的情况下，在$ω_g=Ω$和$ω_g=2Ω$处出现磁共振。这种谐振机制可以用于建立GW驱动的回旋加速器发射器的模型。
英文摘要：
The equations which determine the response of a charged particle moving in a magnetic field to an incident gravitational wave(GW) are derived in the linearized approximation to general relativity. We briefly discuss several astrophysical applications of the derived formulae taking into account the resonance between the wave and the particle's motion which occurs at $ω_g=2Ω$, whenever the GW is parallel to the constant magnetic field. In the case where the GW is perpendicular to the constant magnetic field, magnetic resonances appear at $ω_g=Ω$ and $ω_g=2Ω$. Such resonant mechanism may be useful to build models of GW driven cyclotron emitters.
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