Thermal fluctuations, deflection angle and greybody factor of a high-dimensional Schwarzschild black hole in STVG

Qian Li, Yu Zhang, Qi-Quan Li, Qinshan Sun
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Abstract

In this work, we study the thermal fluctuations, deflection angle and greybody factor of the high-dimensional Schwarzschild black hole in scalar-tensor-vector gravity (STVG). We calculate some thermodynamic quantities related to the correction of black hole entropy caused by thermal fluctuations and discuss the effect of the correction parameters on these quantities. By analysing the changes in the corrected specific heat, we find that thermal fluctuations make the small-sized black hole more stable. It is worth noting that the STVG parameter does not affect the thermodynamic stability of this black hole. Additionally, by utilizing the Gauss-Bonnet theorem, the deflection angle is obtained in the weak field limit and the effect of two parameters on the results is visualized. Finally, we calculate the bounds on greybody factor of a massless scalar field. We observe that as the STVG parameter around black hole increases, the weak deflection angle becomes larger and the more scalar particles can reach infinity. However, the spacetime dimension has the opposite effect to the STVG parameter on the weak deflection angle and greybody factor.
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STVG中高维施瓦兹柴尔德黑洞的热波动、偏转角和灰度因子
在这项工作中,我们研究了标量-张量-矢量引力(STVG)中高维施瓦兹柴尔德黑洞的热波动、偏转角和灰度因子。我们计算了一些与热波动引起的黑洞熵修正有关的热力学量,并讨论了修正参数对这些量的影响。通过分析修正比热的变化,我们发现热波动使小尺寸黑洞更加稳定。值得注意的是,STVG 参数并不影响该黑洞的热力学稳定性。此外,利用高斯-波内特定理,我们得到了弱场极限下的偏转角,并直观地看到了两个参数对结果的影响。最后,我们计算了无质量标量场的灰体因子边界。我们观察到,随着黑洞周围 STVG 参数的增加,弱偏转角变得更大,更多的标量粒子可以达到无穷大。然而,时空维度对弱偏转角和灰度因子的影响与 STVG 参数相反。
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