论文标题
辐射光谱和高维电荷保姆的有效温度黑色孔
Radiation Spectra and Effective Temperatures in Higher-Dimensional Charged-de Sitter Black Holes
论文作者
论文摘要
在这项研究中，研究了一个标量场在高维reissner-nordström-de Sitter黑洞中传播的标量场。假定标量字段与勃雷或散装标量曲率具有非最小耦合。讨论了黑洞温度的五种不同的{定义}：基于表面重力，Bousso-Hawking温度和三个有效温度的温度。在粒子和时空特性的效果下检查了棕褐色和散装上的最小和非最小耦合标量场的灰体因子。黑洞的能量发射光谱是在各种温度下针对Brane和散装通道确定的。发现Bousso-Hawking温度下的能量发射速率在其他温度下占主导地位。能量发射曲线被耦合参数的存在抑制。最后，计算了宽大的武器发射比。值得注意的是，对于宇宙常数的温度和状态的一定定义，可以进行批量优势。
In this study, a scalar field propagating in a higher-dimensional Reissner-Nordström-de Sitter black hole is investigated. Scalar fields are assumed to have non-minimal coupling to the brane or bulk scalar curvature. Five different {definitions} of black hole temperatures are discussed: temperature based on surface gravity, Bousso-Hawking temperature, and three effective temperatures. The greybody factors of minimally and non-minimally coupled scalar fields on the brane and in the bulk are examined under the effect of particle and spacetime properties. The energy emission spectra of black holes are determined at various temperatures for both the brane and bulk channels. The energy emission rates at the Bousso-Hawking temperature are found to be dominant over those at other temperatures. The energy emission curves are suppressed by the presence of coupling parameters. Finally, the bulk-over-brane emission ratios are calculated. Notably, bulk dominance becomes possible for a certain definition of the temperatures and regime of the cosmological constant.
