Mass inflation - The semiclassical regime

Details Mass inflation - The semiclassical regime Mass inflation - The semiclassical regime

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvl..70...13b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 70, no. 1, p. 13-16.

Statistics

Computation

26

Astronomical Models, Black Holes (Astronomy), Cauchy Problem, Space-Time Functions, Computational Astrophysics, Mass Distribution, Wave Equations

Scientific paper

We examine the possible influence of semiclassical effects on the structure of spacetime in the vicinity of a black-hole Cauchy horizon. While the classical picture is that of a weak mass-inflation singularity (a null singularity characterized by the unbounded increase of the black-hole internal mass function), we suggest that quantum effects may produce either (1) a stronger, spacelike singularity, or (2) a regular spacetime, in the sense that curvature would nowhere increase beyond Planckian.

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