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Quantum Corrections and Entropy Spectrum in Different Gravity

机译:不同引力的量子校正和熵谱

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Black hole spectroscopy has been successfully reproduced in the tunneling picture [1,2]. As a result, the derived entropy spectrum of black hole in different gravity (including Einstein's gravity, Einstein-Gauss-Bonnet gravity and Horava-Lifshitz gravity) are all evenly spaced, sharing the same forms as S_n = n, where physical process is only confined in the semiclassical framework. However, the real physical picture should go beyond the semiclassical approximation. In this case, the physical quantities would undergo higher-order quantum corrections, whose effect on different gravity shares in different forms. Motivated by these facts, in this chapter we aim to observe how quantum corrections affect black hole spectroscopy in different gravity. The result shows that, in the presence of higher-order quantum corrections, black hole spectroscopy in different gravity still shares the same form as S_n = n,further confirming the entropy quantum is universal in the sense that it is not only independent of black hole parameters, but also independent of higher-order quantum corrections. This is a desiring.result for the forthcoming quantum gravity theory.
机译:黑洞光谱学已成功地复制到隧道照片中[1,2]。结果,在不同引力(包括爱因斯坦引力,爱因斯坦-高斯-邦尼特引力和霍拉瓦-利夫希茨引力)下得出的黑洞熵谱都均匀分布,共享与S_n = n相同的形式,其中物理过程仅局限于半经典框架。但是,真实的物理图像应该超出半经典近似。在这种情况下,物理量将经历高阶量子校正,其对不同重力份额的影响形式不同。基于这些事实,在本章中,我们旨在观察量子校正如何在不同重力下影响黑洞光谱。结果表明,在存在高阶量子校正的情况下,不同引力下的黑洞光谱仍具有与S_n = n相同的形式,进一步证实了熵量子是普遍的,因为它不仅独立于黑洞参数,但也独立于高阶量子校正。这是即将出现的量子引力理论的理想结果。

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