Measuring a parity-violation signature in the early universe via ground-based laser interferometers.

Measuring a parity-violation signature in the early universe via ground-based laser interferometers.
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DOI:
10.1103/physrevlett.99.121101
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发表时间:
2007-07
影响因子:
8.6
通讯作者:
N. Seto;A. Taruya
N. Seto;A. Taruya
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
N. Seto;A. Taruya

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我们表明,成对的相距甚远的干涉仪对于测量引力波随机背景的斯托克斯参数V是有利的。这个参数表征了左右手波振幅的不对称性,这种不对称性的产生与早期宇宙中的宇称破坏密切相关。有利的对包括更大尺寸的干涉仪LIGO(利文斯顿)-LCGT和AIGO-Virgo,它们对Omega(GW)(背景的简单强度)相对不敏感。使用至少三个检测器,可以分别测量强度Ω(GW)和不对称度V的信息。
We show that pairs of widely separated interferometers are advantageous for measuring the Stokes parameter V of a stochastic background of gravitational waves. This parameter characterizes asymmetry of amplitudes of right- and left-handed waves, and generation of the asymmetry is closely related to parity violation in the early universe. The advantageous pairs include the kilometer-size interferometers LIGO (Livingston)-LCGT and AIGO-Virgo, which are relatively insensitive to Omega(GW) (the simple intensity of the background). Using at least three detectors, information of the intensity Omega(GW) and the degree of asymmetry V can be separately measured.