Reissner-Nordstrom Black Holes and Strings with Rescaled Tension
arXiv:hep-th/9610068 · doi:10.1142/S0217751X99001780
Abstract
We show that extreme and nonextreme Reissner--Nordstrom black holes in five dimensions can be described by closed fundamental strings with two charges in a magnetic five brane. Due to the five brane background the string oscillator number and tension are rescaled whereas the mass remains fixed. The black hole mass is given by the sum of the five brane and string masses. Its entropy however is given by only that of the string with the tension rescaling taken into account. We also show that the emission of a low energy scalar from the slightly nonextreme string matches the Hawking radiation expected from the black hole.
20 pages in phyzzx
References in corpus (1)
Cited by in corpus (19)
- General Rotating Black Holes in String Theory: Greybody Factors and Event Horizons
- Black Holes and Solitons in String Theory
- Strings and the Holographic Description of Asymptotically de Sitter Spaces
- Black Holes as Fundamental Strings: Comparing the Absorption of Scalars
- Black Holes as Conformal Field Theories on Horizons
- On the Cardy-Verlinde Formula and the de Sitter/CFT Correspondence
- Horizon Conformal Field Theories from Black Holes
- Rindler Energy is Wald Entropy
- On the Holographic Nature Of Rindler Energy
- Liouville Theory on Horizons: Towards a Quantum Theory of Black Holes
- Black Hole Entropy and Superconformal Field Theories on Brane-Antibrane Systems
- Statistical entropy of near-extremal and fundamental black p-branes
- Extremal Black Hole Entropy from Horizon Conformal Field Theories
- The Holographic Entanglement Entropy of Schwarzschild Black Holes
- Dynamics of D-brane Black Holes
- Schwarzschild Black Holes and Asymptotic
- Black Hole Entropy and the Pseudo Goldstone Bosons of Conformal Symmetry
- Bekenstein Entropy is String Entropy
- Entropic Gravity in Rindler Space