The size of bodies in which this phenomenon originates must be small, because increasing mass decreases the power of it.
Near the Cauchy horizon, a Rindler observer will see an analogue to this phenomenon in the Unruh effect. Its namesake temperature is proportional to the surface gravity of its source. The size of bodies in which this phenomenon originates must be small, because increasing mass decreases the power of it. It happens when a particle resulting from pair production tunnels through the event horizon. The no-hair theorem mandates that this phenomenon be in a mixed state, even for the input of a pure quantum state, a result at odds with Liouville's theorem that results in an "information paradox." This phenomenon eventually leads to black hole evaporation. For 10 points, name this thermal radiation named for the author of A Brief History of Time.
Near the Cauchy horizon, a Rindler observer will see an analogue to this phenomenon in the Unruh effect.
Bekenstein-Hawking radiation [prompt on black-body radiation]