Its Planck spectrum with temperature T is given by Boltzmann's constant, h-bar, the Schwarzchild radius, and the mass of the object that produces this phenomenon.
Its Planck spectrum with temperature T is given by Boltzmann's constant, h-bar, the Schwarzchild radius, and the mass of the object that produces this phenomenon. Its luminosity is given by the standard Stefan-Boltzmann blackbody formula, though if the temperature exceeds the rest mass energy of a particle type, then particles and antiparticles are radiated in addition to photons, which cause the apparent luminosity outside of a black hole. FTP, identify this type of radiation that black holes emit, named after the current holder of the Lucasian Professorship of Mathematics.
Its Planck spectrum with temperature T is given by Boltzmann's constant, h-bar, the Schwarzchild radius, and the mass of the object that produces this phenomenon.
{Hawking} radiation