论文标题
连续重力波检测以了解快速无线电爆发的发电机理
Continuous gravitational wave detection to understand the generation mechanism of fast radio bursts
论文作者
论文摘要
由于意外发现快速无线电爆发（FRB），研究人员提出了各种理论和模型来解释这些现象。最近开发的一种这样的模型结合了所谓的Gertsenshtein-Zel'dovich（Gz）效应，该效应指出，当引力波穿越脉冲星磁层时，重力辐射的一部分被转化为电磁（EM）辐射。观察到的FRB的特性与该EM辐射的特性一致，这一点明显地表明，Gz效应可以解释重复和不重复的FRB。如果该模型正确，则PULSAR的性质不应随着时间的流逝而变化，并且会在很长一段时间内继续发射EM偶极子和重力四极杆辐射。本文针对脉冲星机制产生的重力辐射，并表明几个提出的引力波检测器可以检测到这些引力波。如果将来从FRB的位置进行此类检测，它可能会验证FRB生产的GZ过程，并有可能排除其他FRB生成的其他几种理论。
Since the unexpected discovery of fast radio bursts (FRBs), researchers have proposed varied theories and models to explain these phenomena. One such model that has recently been developed incorporates the so-called Gertsenshtein-Zel'dovich (GZ) effect, which states that when gravitational waves traverse a pulsar magnetosphere, a portion of the gravitational radiation is transformed into electromagnetic (EM) radiation. The observed properties of FRBs are consistent with the properties of this EM radiation, implying, remarkably, that the GZ effect can account for both repeating and non-repeating FRBs. If this model is correct, the pulsar's properties should not change over time, and it would continue to emit both EM dipole and gravitational quadrupole radiation for a long period of time. This article targets the gravitational radiation produced by the pulsar mechanism and shows that several proposed gravitational wave detectors can detect these gravitational waves. If such detections are performed in the future from the location of FRBs, it might validate the GZ process for FRB production and potentially rule out several other theories of FRB generation.
