Detection of high-frequency gravitational waves using high-energy pulsed lasers

Detection of high-frequency gravitational waves using high-energy pulsed lasers
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使用高能脉冲激光探测高频引力波

DOI:
10.1088/1361-6382/acd517
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发表时间:
2023
影响因子:
3.5
通讯作者:
Vacalis G
Vacalis G
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Vacalis G

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提出了一种利用高能脉冲激光探测高频引力波的新方法。通过逆Gertsenshtein效应,GW和激光束之间的相互作用导致电磁信号的产生。后者可以使用单光子计数技术检测。我们计算了可检测GW的最小应变,该应变仅取决于激光参数。我们发现,共振发生在这个过程中,当GW的频率是激光频率的两倍。用这种方法,对10 13-10 19 Hz的频率范围内的应变进行了非连续的探索
We propose a new method for detecting high-frequency gravitational waves (GWs) using high-energy pulsed lasers. Through the inverse Gertsenshtein effect, the interaction between a GW and the laser beam results in the creation of an electromagnetic signal. The latter can be detected using single-photon counting techniques. We compute the minimal strain of a detectable GW which only depends on the laser parameters. We find that a resonance occurs in this process when the frequency of the GW is twice the frequency of the laser. With this method, the frequency range 10 13–10 19 Hz is explored non-continuously for strains
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