标题： 黑洞的霍金辐射功率方程 显示英文标题

标题： Hawking Radiation Power Equations for Black Holes

摘要： 我们推导了渐近平坦、渐近反德西特（AdS）和渐近德西特（dS）黑洞的霍金辐射功率方程，这是通过使用这些黑洞的灰体因子来实现的。 我们观察到，对应于低频灰体因子的渐近平坦黑洞的辐射功率方程，既依赖于霍金温度也依赖于视界半径。 然而，对于渐近频率的灰体因子，它仅依赖于霍金温度。 我们还得到了低于和高于临界频率的渐近AdS黑洞的功率方程。 在渐近频率下，施瓦茨希尔德AdS和雷斯纳-诺德斯特伦AdS解的辐射功率方程是相同的，并且仅依赖于霍金温度。 我们还讨论了低频下渐近dS黑洞的功率方程，适用于偶数维和奇数维。 显示英文摘要

摘要： We derive the Hawking radiation power equations for black holes in asymptotically flat, asymptotically Anti-de Sitter (AdS) and asymptotically de Sitter (dS) black holes, This is done by using the greybody factor for these black holes. We observe that the radiation power equation for asymptotically flat black holes, corresponding to greybody factor at low frequency, depends on both the Hawking temperature and the horizon radius. However, for the greybody factors at asymptotic frequency, it only depends on the Hawking temperature. We also obtain the power equation for asymptotically AdS black holes both below and above the critical frequency. The radiation power equation for at asymptotic frequency is same for both Schwarzschild AdS and Reissner-Nordstr\"om AdS solutions and only depends on the Hawking temperature. We also discuss the power equation for asymptotically dS black holes at low frequency, for both even or odd dimensions.