论文标题
爱因斯坦阳米尔米尔斯重力的黑洞的标量准模式
Scalar quasinormal modes of black holes in Einstein-Yang-Mills gravity
论文作者
论文摘要
在爱因斯坦 - 阳米尔斯黑洞的背景时期，研究了标量场扰动的准模式。五维爱因斯坦 - 阳米尔斯黑洞的度量函数中的对数项消除了鹰温度的差异，但保持了准模式的电荷依赖性行为。准模式频率的真实和虚构部分在不同维度上具有相同的电荷依赖性行为。与高维施瓦茨柴尔德黑洞的情况相似，紧凑的大约关系，$ω_ {\ rm rm rm rm} \ sim d/r _ {+} $也存在于quasinormal模式频率的实际部分$ω_ {\ rm rm r} $ ymight $ n dimens $ dimens $ dimens $ dimens in night ymimens $ nimens in nigh night y dimens in nimens in in nigh-dimens in。孔。
Quasinormal modes of a scalar field perturbation are investigated in the background spacetime of Einstein-Yang-Mills black holes. The logarithmic term in the metric function of the five-dimensional Einstein-Yang-Mills black hole eliminates the divergence of the Hawking temperature but maintains the charge-dependent behavior of the quasinormal modes. The real and imaginary parts of quasinormal mode frequencies have the same charge-dependent behavior in different dimensions. Similar to the case of high dimensional Schwarzschild black holes, a compact approximate relation, $ω_{\rm R}\sim D/r_{+}$, also exists between the real part of the quasinormal mode frequencies $ω_{\rm R}$ and the number of dimensions $D$ in the higher than five dimensional Einstein-Yang-Mills black holes.
