Holographic quantization of gravity in a black hole background

Holographic quantization of gravity in a black hole background
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黑洞背景下重力的全息量子化

DOI:
10.1063/1.4942101
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发表时间:
2015
影响因子:
1.3
通讯作者:
I. Park
I. Park
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
I. Park

文献摘要

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它最近被观察到在公园[Eur. Phys. J. C(未出版);电子版arXiv:1404.5066 [hep-th]]认为引力的全息性质可能是引力量子化的关键。所谓的“全息量子化”已经在Park [J. High Energy Phys. 1504,053(2015); e-print arXiv:1412.1528 [hep-th]; e-print arXiv:1506.08383 [hep-th]]中针对平坦背景中的爱因斯坦引力进行。将该过程推广到弯曲背景是本工作的主要目标。特别是,我们认为爱因斯坦的行动扩大周围的史瓦西背景。
It was recently observed in Park [Eur. Phys. J. C (unpublished); e-print arXiv:1404.5066 [hep-th]] that the holographic nature of gravity may hold a key to quantization of gravity. The so-called “holographic quantization” has been carried out in Park [J. High Energy Phys. 1504, 053 (2015); e-print arXiv:1412.1528 [hep-th]; e-print arXiv:1506.08383 [hep-th]] for Einstein gravity in a flat background. Generalizing the procedure to a curved background is the main goal of the present work. In particular, we consider the Einstein action expanded around a Schwarzschild background.