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The Reissner-Nordstr"om black hole - moving mirror correspondence is solved. The beta coefficients reveal that charge makes a black hole radiate fewer particles (neutral massless scalars) per frequency. An old Reissner-Nordstr"om black hole emits particles in an explicit Planck distribution with temperature corresponding to the surface gravity of its outer horizon.

生成讲解博客的中文版本

生成AI智能校验的中文版本