论文标题
加速器的边界类似物的黑洞
Accelerating boundary analog of a Kerr black hole
论文作者
论文摘要
加速的边界对应关系（即，平坦的时空加速镜轨迹）是针对Kerr时空得出的，其通用公式的范围从Schwarzschild极限（零角动量）到极端的最大旋转情况（产生渐近均匀的均匀加速）。 Beta Bogoliubov系数显示，由于角动量的“春季常数”类似物，粒子光谱是晚期的粒子分布，温度比Schwarzschild Black Hole的温度更低。量子应力张量表明在晚期与永恒热平衡一致的能量通量恒定发射。
An accelerated boundary correspondence (i.e. a flat spacetime accelerating mirror trajectory) is derived for the Kerr spacetime, with a general formula that ranges from the Schwarzschild limit (zero angular momentum) to the extreme maximal spin case (yielding asymptotic uniform acceleration). The beta Bogoliubov coefficients reveal the particle spectrum is a Planck distribution at late times with temperature cooler than a Schwarzschild black hole, due to the "spring constant" analog of angular momentum. The quantum stress tensor indicates a constant emission of energy flux at late times consistent with eternal thermal equilibrium.
