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Brane-world black holes with post-Newtonian parameter: astrophysical signatures

机译:Brane-World Black洞与牛顿参数:天体物理签名

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The existence of the many unanswered questions in fundamental physics, in particular, in astrophysics allows for a great variety of theories to remain viable candidates for becoming the correct theory at energies not accessible in current experiments. One special class of these type of theories is the class of extra-dimensional brane-world models. Besides answering many fundamental problems, for instance, the hierarchy problem, they may produce testable predictions. In this work, we find and investigate brane-world induced black string horizon corrections, when the black hole solution has a post-Newtonian parameter. For suitable choices of such a parameter, the Hawking radiation on the brane is precluded, and the Hawking radiation in the bulk causes the black hole to slightly recoil into the bulk, which modifies the black hole apparent horizon. It has an impact on quasars luminosity and, therefore, might be detected and measured.
机译:特别是在天体物理学中存在许多未答复的问题,特别是在天体物理学中允许各种理论,以保持可行的候选人,以便在当前实验中无法获得的能量处于正确的理论。这些理论的一个特殊类别是跨度尺寸的锋利世界模型。除了回答许多基本问题之外,例如,层次问题,它们可能会产生可测试的预测。在这项工作中,当黑洞解决方案具有后牛顿参数时,我们发现并调查了Brane-World诱导的黑色弦校正。对于这样一个参数的合适选择,燃烧的尖端辐射被排除,并且散装中的霍克宁辐射使黑洞略微反冲到散装中,这改变了黑洞表观视野。它对Quasars亮度产生影响,因此可能会检测和测量。

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