Semiclassical zero temperature black holes in spherically reduced theories
arXiv:hep-th/0201133 · doi:10.1103/PhysRevD.66.024012
Abstract
We numerically integrate the semiclassical equations of motion for spherically symmetric Einstein-Maxwell theory with a dilaton coupled scalar field and look for zero temperature configurations. The solution we find is studied in detail close to the horizon and comparison is made with the corresponding one in the minimally coupled case.
14 pages, latex, 9 eps figures
References in corpus (5)
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- Quantum backreaction of massive fields and self-consistent semiclassical extreme black holes and acceleration horizons
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Cited by in corpus (7)
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- Fundamental Structure of Loop Quantum Gravity
- Reissner-Nordström geometry counterpart in semiclassical gravity
- Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime
- Hawking effect in an extremal Kerr black hole spacetime
- Exactly solvable models in 2D semiclassical dilaton gravity and extremal black holes
- Near-extremal and extremal quantum-corrected two-dimensional charged black holes