Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
1994-05-28
Phys.Lett. B338 (1994) 165-168
Physics
High Energy Physics
High Energy Physics - Theory
11, EDO-EP-1
Scientific paper
10.1016/0370-2693(94)91361-7
In this note we consider a stringy description of black hole horizon. We start with a nonlinear sigma model defined on a two dimensional Euclidean surface with background Rindler metric. By solving the field equations, we show that to the leading order the Bekenstein-Hawking formula of black hole entropy can be produced. We also point out a relation between the present formalism and the 'tHooft formalism.
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