Total spectral distributions from Hawking radiation

Abstract

Taking into account time-dependence of the Hawking temperature and finite evaporation time of the black hole, total spectral distributions of the radiant energy and of the number of particles have been explicitly calculated and compared to their temporary (initial) blackbody counterparts (spectral exitances).

8 pages, 1 figure, accepted version (equivalent to previous version, i.e. to v3, but completely re-edited)

References in corpus (1)

• Hawking radiation is corpuscular

Cited by in corpus (3)

• Unitary toy qubit transport model for black hole evaporation
• Photon intrinsic frequency and size in stringy photon model
• Unitary evolution to a state with a fixed mean number of particles