Classical Black Hole Evaporation in Randall-Sundrum Infinite Braneworld
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概要
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After the gravity induced on the brane in the Randall-Sundrum (RS) infinite braneworld is briefly reviewed, we discuss the possibility that black holes evaporate as a result of classical evolution in this model based on the AdS/CFT correspondence. If this possibility is really the case, the existence of long-lived solar mass black holes will give the strongest constraint on the bulk curvature radius. At the same time, we can propose a new method to simulate the evaporation of a 4D black hole due to the Hawking radiation as a 5D process.
- 一般社団法人日本物理学会の論文
- 2003-03-28
著者
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Tanaka T
Department Of Physics Graduate School Of Science Kyoto University
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Tanaka Takahiro
Yukawa Institute For Theoretical Physics Kyoto University
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