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arXiv 1406.4147hep-thgr-qc
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引力子的高能引力散射和玻色-爱因斯坦凝聚体

High-Energy Gravitational Scattering and Bose-Einstein Condensates of Gravitons

Florian Kuhnel, Bo Sundborg

摘要:

量子黑洞很难描述。我们考虑了两种看似不同的方法,高能散射和把黑洞看作引力子的玻色-爱因斯坦凝聚体的提议,并建立了它们之间的联系。在程函近似下研究了高能散射,并进一步用鞍点近似处理。对散射振幅的主要贡献来自于N个引力子交换的梯形图,引力子的数目服从泊松分布。这种近似支持引力子玻色-爱因斯坦凝聚体的图像,其范围等于史瓦西半径,它以鞍点决定的方式随N增长。该方法允许计算的1 / N修正鞍点周围的波动,我们评论这些。散射方法可能是量子黑洞的有用探测器,特别是当用凝聚体来解释时。

英文摘要:

Quantum black holes are difficult to describe. We consider two seemingly divergent approaches, high-energy scattering and the proposal to regard black holes as Bose-Einstein condensates of gravitons, and establish a connection between them. High-energy scattering is studied in the eikonal approximation, which is processed further by a saddle-point approximation. The dominant contribution to the scattering amplitude comes from a ladder diagram with the exchange of N gravitons, and the number of gravitons follows a Poisson distribution. This approximation supports the picture of a graviton Bose-Einstein condensate with an extent equal the Schwarzschild radius, which grows with N in a way determined by the saddle point. The approach permits calculations of 1 / N corrections from the fluctuations around the saddle points and we comment on these. Scattering methods might be useful probes of quantum black holes, especially when interpreted in terms of condensates.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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