普朗克尺度下理想气体的热力学与强量子引力测量

Latévi M. Lawson
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引用次数: 1

摘要

最近在[J]。理论物理。答:数学。理论。53,115303(2020)],我们引入了一组描述普朗克尺度下时空的非交换代数。我们发现了一个有趣的有意义的结果,即广义不确定性原理导出的量子引力的最大长度与广义不确定性原理导出的最小长度具有不同的物理含义。在这个理论中,最大长度的出现揭示了在这个尺度上强大的量子引力效应,并预测了低能引力粒子的探测。为了证明这些预测,我们在一维空间中研究了一个被限制在无限平方阱势中的自由粒子的动力学。由于量子引力的影响在这个空间很强,我们证明了这个系统的能谱与不受引力理论影响的量子力学的普通能谱成弱比例。这种粒子的状态表现出类似于标准相干态的特性,这是在这个尺度上量子涨落的结果。然后,利用该系统的谱,我们在普朗克尺度上分析了由N个不可区分粒子组成的理想气体的正则系综和微正则系综的热力学量。结果表明两种统计描述完全一致。此外,与最小长度情景和黑洞理论的结果比较表明,该理论中的最大长度引起变形参数的对数修正,这是强量子引力效应的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thermodynamics of Ideal Gas at Planck Scale with Strong Quantum Gravity Measurement
More recently in [J. Phys. A: Math. Theor. 53, 115303 (2020)], we have introduced a set of noncommutative algebra that describes the space-time at the Planck scale. The interesting significant result we found is that the generalized uncertainty principle induced a maximal length of quantum gravity which has different physical implications to the one of generalized uncertainty principle with minimal length. The emergence of a maximal length in this theory revealed strong quantum gravitational effects at this scale and predicted the detection of gravity particles with low energies. To make evidence of these predictions, we study the dynamics of a free particle confined in an infinite square well potential in one dimension of this space. Since the effects of quantum gravity are strong in this space, we show that the energy spectrum of this system is weakly proportional to the ordinary one of quantum mechanics free of the theory of gravity. The states of this particle exhibit proprieties similar to the standard coherent states which are consequences of quantum fluctuation at this scale. Then, with the spectrum of this system at hand, we analyze the thermodynamic quantities within the canonical and microcanonical ensembles of an ideal gas made up of $N$ indistinguishable particles at the Planck scale. The results show a complete consistency between both statistical descriptions. Furthermore, a comparison with the results obtained in the context of minimal length scenarios and black hole theories indicates that the maximal length in this theory induces logarithmic corrections of deformed parameters which are consequences of a strong quantum gravitational effect.
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