Pole skipping and zero temperature

Pole skipping and zero temperature
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DOI:
10.1103/physrevd.103.066017
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发表时间:
2020-11
期刊:
影响因子:
5
通讯作者:
Makoto Natsuume;T. Okamura
Makoto Natsuume;T. Okamura
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Makoto Natsuume;T. Okamura

文献摘要

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研究了旋转BTZ黑洞背景中标量延迟格林函数的跳极现象。在静态情况下,跳极点通常位于具有适当复波数$q$的负虚Matsubara频率$\omega=-(2\pi T)ni$处。但是,在$(1+1)$维CFT中,可以独立地引入左移动扇区和右移动扇区的温度。因此,跳极点$\omega$取决于旋转背景中的左右温度。在极限情况下,一般不会发生跳杆现象。但在一种特殊情况下,即使在极限情况下也会发生极点跳跃,并且跳极点由右松原频率给出。
We study the pole-skipping phenomenon of the scalar retarded Green's function in the rotating BTZ black hole background. In the static case, the pole-skipping points are typically located at negative imaginary Matsubara frequencies $\omega=-(2\pi T)ni$ with appropriate values of complex wave number $q$. But, in a $(1+1)$-dimensional CFT, one can introduce temperatures for left-moving and right-moving sectors independently. As a result, the pole-skipping points $\omega$ depend both on left and right temperatures in the rotating background. In the extreme limit, the pole-skipping does not occur in general. But in a special case, the pole-skipping does occur even in the extreme limit, and the pole-skipping points are given by right Matsubara frequencies.