'Evaporation' of black holes and the fundamental length

Details 'Evaporation' of black holes and the fundamental length 'Evaporation' of black holes and the fundamental length

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975zhpmr..22..514g&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 22, Nov. 20, 1975, p. 514, 515.) JETP Letters, vol. 22, Nov. 20, 1975, p. 251. Translation.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Gravitational Effects, Particle Emission, Relativistic Theory, Stellar Evolution, Emission Spectra, Stellar Temperature

Scientific paper

The effect of a fundamental length on the duration of black hole evaporation through particle emission is considered. It is suggested that the existence of a fundamental length (which would be much greater than the gravitational length of 10 to the -33rd power cm) can radically influence the behavior of black holes during the last stages of their evaporation and would have a marked effect on the high-energy region of a hole's emission spectrum. In particular, it is shown that if the presence of a fundamental length is assumed to limit the density of matter to some fundamental minimum, the evaporation of black holes having an admissible mass would, in general, be unobservable once the fundamental length is attained.

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