论文标题
Kerr-Newman黑洞的鹰辐射粒子谱
Hawking radiation particle spectrum of a Kerr-Newman black hole
论文作者
论文摘要
带电的，旋转的Kerr-Newman黑洞代表了Einstein-Maxwell的一般相对论的最渐近平坦的黑洞解决方案。在这里，我们考虑了通过利用（1+1）二维加速边界对应关系（即Minkowski SpaceTime中的平坦时空镜轨迹），用于由Kerr-Newman Black Hole产生的鹰辐射的简化模型。我们在适当的限制下得出了粒子光谱及其延迟热分布，该粒子光谱及其延迟热分布。我们还计算了极端Kerr-Newman系统的粒子光谱和发出的总能量。
Charged, rotating Kerr-Newman black holes represent the most general class of asymptotically flat black hole solutions to the Einstein-Maxwell equations of general relativity. Here, we consider a simplified model for the Hawking radiation produced by a Kerr-Newman black hole by utilising a (1+1)-dimensional accelerated boundary correspondence (i.e. a flat spacetime mirror trajectory) in Minkowski spacetime. We derive the particle spectrum and its late-time thermal distribution which reduces to the Kerr, Reissner-Nordström and Schwarzschild cases in the appropriate limits. We also compute the particle spectrum of the extremal Kerr-Newman system and the total energy emitted.
