Angular-momentum loss in evaporating black holes

Details Angular-momentum loss in evaporating black holes Angular-momentum loss in evaporating black holes

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nciml..30...13b&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 30, Jan. 3, 1981, p. 13, 14.

Mathematics

Probability

1

Angular Momentum, Black Holes (Astronomy), Evaporation, Mass Transfer, Decay Rates, Gravitation Theory, Probability Theory, Quantum Theory, Rotary Stability, Singularity (Mathematics), Space-Time Functions

Scientific paper

Consideration is given to the evolution of the angular momentum of an evaporating black hole. The conclusions of Carter (1974), that the mass and angular momentum losses of a black hole in the initial stages of evaporation are comparable, and of Page (1976), that the angular momentum loss is sufficiently great to reduce the residual angular momentum to zero, are examined. It is pointed out that the limitation of Page that the axial quantum number of particles emitted be greater than zero is too restrictive. With this restriction relaxed, there would then be a nonnegligible residual angular momentum, and the possibility of the formation of Kerr naked singularity as a final state arises.

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