Size Gap for Zero Temperature Black Holes in Semiclassical Gravity
arXiv:gr-qc/9806069 · doi:10.1103/PhysRevD.59.044007
Abstract
We show that a gap exists in the allowed sizes of all zero temperature static spherically symmetric black holes in semiclassical gravity when only conformally invariant fields are present. The result holds for both charged and uncharged black holes. By size we mean the proper area of the event horizon. The range of sizes that do not occur depends on the numbers and types of quantized fields that are present. We also derive some general properties that both zero and nonzero temperature black holes have in all classical and semiclassical metric theories of gravity.
arXiv comment4 pages, ReVTeX, no figures
References in corpus (6)
- No hair for spherical black holes: charged and nonminimally coupled scalar field with self--interaction
- Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole
- Positivity of Entropy in the Semi-Classical Theory of Black Holes and Radiation
- Geometry of nonextreme black holes near the extreme state
- Gauge Field Back-reaction on a Black Hole
- Quantum corrections to critical phenomena in gravitational collapse
Cited by in corpus (7)
- Energy-Momentum Tensor of Particles Created in an Expanding Universe
- Do semiclassical zero temperature black holes exist?
- Black hole remnants may exist if Starobinsky inflation occurred
- Reissner-Nordström geometry counterpart in semiclassical gravity
- Truly naked spherically-symmetric and distorted black holes
- GEO600 Online Detector Characterization System
- Quantum scalar field in D-dimensional static black hole space-times