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Black holes in presence of cosmological constant: second order in 1 D $$ rac{1}{D} $$

机译:在宇宙学常量存在下的黑洞: < MFRAC> 1 D $$ FRAC {1} {D} $$

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A bstract We have extended the results of [1] upto second subleading order in an expansion around large dimension D . Unlike the previous case, there are non-trivial metric corrections at this order. Due to our ‘background-covariant’ formalism, the dependence on Ricci and the Riemann curvature tensor of the background is manifest here. The gravity system is dual to a dynamical membrane coupled with a velocity field. The dual membrane is embedded in some smooth background geometry that also satisfies the Einstein equation in presence of cosmological constant. We explicitly computed the corrections to the equation governing the membrane-dynamics. Our results match with earlier derivations in appropriate limits. We calculated the spectrum of QNM from our membrane equations and matched them against similar results derived from gravity.
机译:Bstract我们已经将[1]的结果扩展到最高尺寸D的扩展中的第二个外侧顺序。 与前一个情况不同,此顺序存在非普通的度量校正。 由于我们的“背景协助的”形式主义,对RICCI的依赖和背景的RIEMANN曲率张量在这里表现出来。 重力系统是与速度场耦合的动态膜的双重。 双膜嵌入在一些平滑的背景几何形状中,该几何形状也满足宇宙恒定存在的爱因斯坦方程。 我们明确计算了管理膜动力学的等式的校正。 我们的结果与早期的推导符合适当的限制。 我们计算了来自膜方程的Qnm的光谱,并将它们与重力衍生的类似结果匹配。

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