Fate of black branes in Einstein-Gauss-Bonnet gravity
Fate of black branes in Einstein-Gauss-Bonnet gravity
复制标题
爱因斯坦-高斯-博内引力中黑膜的命运
DOI：
10.1103/physrevd.79.124046
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发表时间：
2008
影响因子：
5
通讯作者：
L. Wijewardhana
中科院分区：
文献类型：
--
作者：
P. Surányi;C. Vaz;L. Wijewardhana
Black branes are studied in Einstein-Gauss-Bonnet gravity. Evaporation drives black branes toward one of two singularities depending on the sign of {alpha}, the Gauss-Bonnet coupling. For positive {alpha} and sufficiently large ratio {radical}({alpha})/L, where L/2{pi} is the radius of compactification, black branes avoid the Gregory-Laflamme (GL) instability before reaching a critical state. No black branes with the radius of horizon smaller than the critical value can exist. Approaching the critical state branes have a nonzero Hawking temperature. For negative {alpha} all black branes encounter the GL instability. No black branes may exist outside of the interval of the critical values 0{<=}{beta}<3, where {beta}=1-8{alpha}/r{sub h}{sup 2} and r{sub h} is the radius of horizon of the black brane. The first order phase transition line of GL transitions ends in a second order phase transition point at {beta}=0.
