论文标题
回复“评论'灰体辐射和大黄蜂重力模型中类似Kerr的黑洞的准模式”
Reply to "Comment on 'Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model' "
论文作者
论文摘要
在我们最近的研究参考中。 [1]：欧洲。物理。 J. C 81，501（2021），主要目标是通过灰色体因子和准标准模式分析揭示洛伦兹对称性破坏（LSB）效应。丁等。 [2]我们论文中使用的大黄蜂重力模型的Kerr样黑洞解[1]毫无疑问，Maluf和Muniz [3]证明了这是错误的。现在，我们在[1]中执行的灰体因子和准模式分析的条件下解释了。我们根据所讨论的条件重新制定计算，并在此答复中介绍新的结果。
In our recent study Ref. [1]: Eur. Phys. J. C 81, 501 (2021) , the main goal was to reveal the Lorentz symmetry breaking (LSB) effect in the rotating black holes via the greybody factor and quasinormal mode analyzes. Ding et al. [2] Kerr-like black hole solution of the bumblebee gravity model used in our paper [1] has unquestionably proven by Maluf and Muniz [3] that it is wrong. We now explain under which condition the greybody factor and quasinormal mode analyzes performed in [1] become valid. We re-make the calculations according to the condition in question and present the new results in this reply.
