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arXiv 2512.19087hep-th

德西特视界结构中的极点跳变

Pole-skipping in the de Sitter horizon structure

Haiming Yuan, Xian-Hui Ge, Keun-Young Kim

AI总结:

研究发现德西特时空中的不同自旋场在特定条件下表现出相同的极点跳变频率,但动量在复空间中因曲率而偏移,可通过算子维度测量。

摘要:

我们研究了在德西特(dS)时空的宇宙视界$ r = r_c $附近入射波的极点跳变结构。我们发现标量场(自旋0)、狄拉克场(自旋1/2)、麦克斯韦场(自旋1)、拉里-施温格场(自旋3/2)以及引力场(自旋2)在满足反德西特(AdS)时空相应自旋场入射波条件时,表现出相同的极点跳变点频率$ ω_\star $。然而,动量$ k_\star $在复空间中经历偏移,这种偏移源于时空曲率。在两个弯曲时空中的算子维度$ Δ $中,极点跳变点的动量偏移可通过相互复共轭的动量来测量,在dS和AdS这两种曲率相反的时空背景下。

英文摘要:

We study the pole-skipping structure of incoming waves near the cosmic horizon $r=r_c$ in de Sitter (dS) spacetime. We find that the scalar field with spin-0, the Dirac field with spin-1/2, the Maxwell field with spin-1, the Rarita-Schwinger field with spin-3/2, and the gravitational field with spin-2 exhibit the same frequencies $ω_\star$ of pole-skipping points as their corresponding spin fields satisfying the incoming wave conditions in anti-de Sitter (AdS) spacetime. However, the momenta $k_\star$ undergo a shift in complex space, which originates from the spacetime curvature. The shift in momenta at the pole-skipping points could be measured through the operator dimensions $Δ$ in two curved spacetimes, where momenta are mutually complex conjugate in dS and AdS, two opposite curvature spacetimes.

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