论文标题
极端鹰辐射
Extreme Hawking Radiation
论文作者
论文摘要
通过解决渐近接近均匀加速度的轨迹的相应运动镜模型，通过求解相应的运动镜模型来建模极端的Reissner-Nordström（ERN）黑洞的崩溃，我们始终获得非零的beta系数。发射有限的能量，辐射光谱是非热的（非稳态 /非planck），软颗粒表征了蒸发的特征，并且在超长时期的颗粒产生受阻。纠缠熵在没有页面曲线转换的情况下发散，证明了非热信息损失。辐射遵守时间反转对称性。
Modeling the collapse of an extreme Reissner-Nordström (ERN) black hole by solving the corresponding moving mirror model for the trajectory that asymptotically approaches uniform acceleration, we obtain the non-zero beta coefficients for all times. Finite energy is emitted, the radiation spectra is non-thermal (non-steady / not Planck), soft particles characterize the evaporation, and particle production at ultra-late times is damped. Entanglement entropy diverges with no Page curve turn-over, demonstrating non-thermal information loss. The radiation obeys time-reversal symmetry.
