Gravitomagnetic resonance in the field of a gravitational wave

M. Ruggiero, A. Ortolan
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引用次数: 10

Abstract

Using the construction of the Fermi frame, the field of a gravitational wave can be described in terms of gravito-electromagnetic fields that are transverse to the propagation direction and orthogonal to each other. In particular, the gravito-magnetic field acts on spinning particles and we show that, due to the action of the gravitational wave field, a new phenomenon, that we call gravito-magnetic resonance, may appear. We give both a classical and a quantum description of this phenomenon and suggest that it can be used as the basis for a new type of gravitational wave detectors. Our results highlight the effectiveness of collective spin excitations, e.g. spin waves in magnetized materials, in detecting high frequency gravitational waves. Here we suggest that, when gravitational waves induce a precession of the electron spin, power is released in the ferromagnetic resonant mode endowed with quadrupole symmetry of a magnetized sphere. This offers a possible path to the detection of the gravito-magnetic effects of a gravitational wave.
引力波场中的重力磁共振
利用费米框架的结构,引力波的场可以用与传播方向横向且彼此正交的引力电磁场来描述。特别是,重力磁场作用于自旋粒子,我们表明,由于引力波场的作用,可能会出现一种新的现象,我们称之为重力磁共振。我们给出了这一现象的经典和量子描述,并认为它可以作为一种新型引力波探测器的基础。我们的研究结果强调了集体自旋激发在探测高频引力波方面的有效性,例如磁化材料中的自旋波。本文提出,当引力波诱导电子自旋进动时,能量以具有磁化球四极对称的铁磁共振模式释放。这为探测引力波的引力磁效应提供了一条可能的途径。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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