We present holographic arguments to predict properties of strongly coupled gravitational systems in terms of weakly coupled gauge theories. In particular we relate the latest computed value for the Choptuik critical exponent in black hole formation in five dimensions, gamma(5D) = 0.412 +/- 1%, to the saturation exponent of four-dimensional Yang-Mills theory in the Regge limit, gamma(BFKL) similar or equal to 0.410. (c) 2007 Elsevier B.V. All rights reserved.
机构:
CEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, FranceCEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, France
Munier, S
Peschanski, R
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机构:CEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, France
机构:
CEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, FranceCEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, France
Munier, S
Peschanski, R
论文数: 0引用数: 0
h-index: 0
机构:CEA Saclay, Serv Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, France