摘要The displaying condition of strength, phase and polarization states of high-frequency relic gravitational waves (HFRGWs) in electromagnetic (EM) detecting systems is studied. It is shown that the displaying condition depends not only on the sensitivity of EM detecting systems and the amplitudes of HFRGWs, but also on the phase, the polarization states of HFRGWs and their matching to the EM detecting systems. In order to display simultaneously the strength, phase and polarization states of the resonant ``monochromatic component'' of HFRGWs, an important necessary condition is the utilization of two or more different EM detectors.
Abstract：The displaying condition of strength, phase and polarization states of high-frequency relic gravitational waves (HFRGWs) in electromagnetic (EM) detecting systems is studied. It is shown that the displaying condition depends not only on the sensitivity of EM detecting systems and the amplitudes of HFRGWs, but also on the phase, the polarization states of HFRGWs and their matching to the EM detecting systems. In order to display simultaneously the strength, phase and polarization states of the resonant ``monochromatic component'' of HFRGWs, an important necessary condition is the utilization of two or more different EM detectors.
(Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))
引用本文:
LI Fang-Yu;YANG Nan. Phase and Polarization State of High-Frequency Relic Gravitational Waves[J]. 中国物理快报, 2009, 26(5): 50402-050402.
LI Fang-Yu, YANG Nan. Phase and Polarization State of High-Frequency Relic Gravitational Waves. Chin. Phys. Lett., 2009, 26(5): 50402-050402.
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2009, Vol. 26 
