The power of this phenomenon is proportional to the constant h-bar times c to the sixth over pi times G-squared times 15360, and the temperature of emission of this phenomenon is equal to 6.4 times 10 to the 6 kelvin over the mass by considering it as a blackbody phenomenon, and sets said temperature proportional to the (*) surface gravity.
An experimental analogue of this phenomenon can be created by firing short laser pulses through a medium with varying refractive index, and was done by Daniele Faccio. The power of this phenomenon is proportional to the constant h-bar times c to the sixth over pi times G-squared times 15360, and the temperature of emission of this phenomenon is equal to 6.4 times 10 to the 6 kelvin over the mass by considering it as a blackbody phenomenon, and sets said temperature proportional to the (*) surface gravity. That effective temperature is the same as that experienced by a uniformly accelerating detector in a vacuum field. A critical mass related to this phenomenon is a sensitive measure of the Hubble time. The original derivation of this phenomenon had particles that had infinite frequency and wavelength less than the Planck length. This phenomenon causes the evaporation of the entities that emit it, and is caused by pair production at the event horizon. For 10 points, name this phenomenon, a form of radiation emitted by a black hole.
An experimental analogue of this phenomenon can be created by firing short laser pulses through a medium with varying refractive index, and was done by Daniele Faccio.
Hawking radiation