量子引力中普朗克光度约束的证据

IF 3.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Wolfgang Wieland
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引用次数: 0

摘要

最近,我们引入了脉冲引力零初始数据的非摄动量子化。在本文中,我们研究该模型的直接物理含义。其中一个量子数是总光度无穷大。我们证明,当光度达到普朗克能量时,跃迁就发生了。下面,辐射功率的频谱是离散的。在普朗克功率以上,光谱是连续的。连续谱中的物理状态由运动状态的叠加组成,其中剪切从上面无界。我们认为这种状态是非物理的,因为它们包含与渐近无穷衰减条件相冲突的焦散量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evidence for Planck luminosity bound in quantum gravity
Recently, we introduced a non-perturbative quantization of impulsive gravitational null initial data. In this note, we investigate an immediate physical implication of the model. One of the quantum numbers is the total luminosity carried to infinity. We show that a transition happens when the luminosity reaches the Planck power . Below , the spectrum of the radiated power is discrete. Above the Planck power, the spectrum is continuous. A physical state that lies in the continuous spectrum consists of a superposition of kinematical states in which the shear is unbounded from above. We argue that such states are unphysical because they contain caustics that are in conflict with the falloff conditions at asymptotic infinity.
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来源期刊
Classical and Quantum Gravity
Classical and Quantum Gravity 物理-天文与天体物理
CiteScore
7.00
自引率
8.60%
发文量
301
审稿时长
2-4 weeks
期刊介绍: Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.
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