The Black Hole Entropy Can Be Smaller than A/4
arXiv:hep-th/9503202 · doi:10.1016/0370-2693(96)00027-5
Abstract
The coupling of a Nambu-Goto string to gravity allows for Schwarzschild black holes whose entropy to area relation is , where is the string tension.
LaTeX, 9 pages, final version to appear in Phys.Lett. B
References in corpus (7)
- Black Hole Entropy in Canonical Quantum Gravity and Superstring Theory
- The Gravitational Hamiltonian, Action, Entropy, and Surface Terms
- Black Hole Entropy and the Dimensional Continuation of the Gauss-Bonnet Theorem
- Quantum Hair on Black Holes
- Action and Entropy of Extreme and Non-Extreme Black Holes
- The Off-Shell Black Hole
- Euclidean Black Hole Vortices
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- Topological black holes dressed with a conformally coupled scalar field and electric charge
- Rotating Black Branes in Brans-Dicke-Born-Infeld Theory
- Thermodynamics of charged rotating black branes in Brans-Dicke theory with quadratic scalar field potential
- Coloured Black Holes in Higher Curvature String Gravity
- Bubbles of Nothing and Supersymmetric Compactifications
- Modification of black-hole entropy by strings
- The Number of Particles Released in Gauge Cosmic String Formation
- Thermal Action and Specific Heat of the Five-Dimensional Non-Extremal Black Hole
- 2+1 Black Hole with a Dynamical Conical Singularity