量子引力最小长度尺度下的修正换向子与修正算子

Joey Contreras, Douglas Singleton, Michael Bishop, Jaeyeong Lee
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引用次数: 2

摘要

量子引力的一般理论通常假设在某些高能量/动量尺度上会有一个固定的最小长度。这样的最小长度可以通过修改标准海森堡不确定性关系在现象学上进行研究。这在实践中通常是通过修改位置和动量算符之间的换向子来实现的,这反过来意味着修改这些算符。然而,这种不确定关系变化的修正会导致与观测数据(伽马射线暴)的冲突。这以预测的最小长度能量尺度的形式出现,它高于普朗克能量,而不是低于它。因此,似乎有一种暗示,即在这些一般理论中没有最小长度尺度。同时,修改运算符,使标准不确定关系保持相同的形式,则不会与观测数据产生冲突。我们证明了位置和动量算符的这种修改是最小长度尺度存在与否的关键决定因素。通过主要关注这些算子的作用,我们还表明,人们可以避免来自短伽马射线暴观测的限制,在某些情况下,短伽马射线暴似乎将最小长度尺度推到了普朗克尺度之上。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Modified Commutators vs Modified Operators in a Quantum Gravity minimal length scale
: Generic theories of quantum gravity often postulate that at some high energy/momentum scale there will be a fixed, minimal length. Such a minimal length can be phenomenologically investigated by modifying the standard Heisenberg Uncertainty relationship. This is generally done in practice by modifying the commutator between position and momentum operators, which in turn means modifying these operators. However, modifications such that the uncertainty relation changes lead to conflicts with observational data (gamma ray bursts). This arises in the form of a predicted minimal length energy scale that is above the Planck energy rather than below it. As a result there seems to be an implication that there is no minimal length scale in these generic theories. Meanwhile, modifying the operators such that the standard uncertainty relation retains the same form, leads to no such conflict with observational data. We show that it is this modification of the position and momentum operators that is the key determining factor in the existence (or not) of a minimal length scale. By focusing primarily on the role of these operators we also show that one can avoid the constraints from the observations of short gamma ray bursts, which in certain cases seem to push the minimal length scale above the Planck scale.
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