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首页> 外文期刊>International Journal of Modern Physics, A. Particles and Fields, Gravitation, Cosmology >Asymptotic quasinormal modes of d-dimensional schwarzschild black hole with Gauss-Bonnet correction
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Asymptotic quasinormal modes of d-dimensional schwarzschild black hole with Gauss-Bonnet correction

机译:带有高斯-贝涅特校正的d维schwarzschild黑洞的渐近拟正模

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摘要

We obtain an analytic expression for the highly damped asymptotic quasinormal mode frequencies of the (d >= 5)-dimensional Schwarzschild black hole modified by the Gauss-Bonnet term, which appears in string derived models of gravity. The analytic expression is obtained under the string inspired assumption that there exists a minimum length scale in the system and in the limit when the coupling in front of the Gauss-Bonnet term in the action is small. Although there are several similarities of this geometry with that of the Schwarzschild black hole, the asymptotic quasinormal mode frequencies axe quite different. In particular, the real part of the asymptotic quasinormal frequencies for this class of single horizon black holes is not proportional to log(3).
机译:我们获得了一个高阻尼渐近准正态模态频率的解析表达式,该模态频率由高斯-邦纳特项修正,并出现在弦的引力模型中,该维斯瓦尔兹黑洞的(d> = 5)维。该解析表达式是在字符串启发的假设下获得的,即在动作中高斯-邦纳特项前面的耦合较小时,系统中存在最小长度比例,并且存在极限。尽管此几何形状与Schwarzschild黑洞有许多相似之处,但渐近准正态模频率却有很大不同。特别是,此类单水平黑洞渐近准正态频率的实部与log(3)不成比例。

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