A radiating metric for evaporating black holes

Details A radiating metric for evaporating black holes A radiating metric for evaporating black holes

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ncimb..68..104b&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 68 B, Mar. 11, 1982, p. 104-110.

Astronomy and Astrophysics

Astrophysics

6

Astrophysics, Black Holes (Astronomy), Mass Transfer, Space-Time Functions, Stellar Evolution, Differential Equations, Evaporation, Schwarzschild Metric

Scientific paper

Since the black-hole (BH) evaporation process is highly dynamic with a mass loss roughly equivalent to 1/M-squared, sooner or later a point will be reached in which the mass carried away by the radiation is no longer a negligible part of the total mass. In such a case, the space-time of the evaporating BH could differ from the usual standard static or stationary one. In this paper, a time-dependent radiating metric is introduced to describe the evaporating BH, and the modifications of the standard picture that this assumption implies are examined. It is shown that the radiating metric permits a better description of the intermediate phases of the evaporation.

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