A Possible Solution of the Cosmological Constant Problem Based on GW170817 and Planck Observations with Minimal Length Uncertainty

IF 1.5 4区 物理与天体物理 Q3 PHYSICS, PARTICLES & FIELDS
A. Diab, Abdel Nasser Tawfik
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引用次数: 3

Abstract

We propose generalized uncertainty principle (GUP) with an additional term of quadratic momentum motivated by string theory and black hole physics and providing a quantum mechanical framework for the minimal length uncertainty, at the Planck scale. We demonstrate that the GUP parameter, β 0 , could be best constrained by the gravitational wave observations, GW170817 event. To determine the difference between the group velocity of graviton and that of the light, we suggest another proposal based on the modified dispersion relations (MDRs). We conclude that the upper bound of β 0 reads ≃1060. Utilizing features of the UV/IR correspondence and the apparent similarities between GUP (including nongravitating and gravitating impacts on Heisenberg uncertainty principle) and the discrepancy between the theoretical and the observed cosmological constant Λ (obviously manifesting gravitational influences on the vacuum energy density), known as catastrophe of nongravitating vacuum, we suggest a possible solution for this long-standing physical problem, Λ ≃ 1 0 − 47  GeV4/ℏ3c3.
基于GW170817和最小长度不确定性普朗克观测的宇宙学常数问题的可能解
我们提出了广义不确定性原理(GUP),并在弦理论和黑洞物理的驱动下增加了二次动量项,并为普朗克尺度下的最小长度不确定性提供了量子力学框架。我们证明GUP参数β 0可以最好地由引力波观测GW170817事件约束。为了确定引力子的群速度和光的群速度之间的差异,我们提出了另一种基于修正色散关系(mdr)的方法。我们得出β 0的上限为≃1060。利用紫外/红外光谱的对应特征和GUP的明显相似性(包括非重力和重力对海森堡测不准原理的影响)以及理论和观测到的宇宙常数Λ的差异(重力对真空能量密度的明显影响),即非重力真空突变,我们提出了一个可能的解决方案Λ: 1 0−47 GeV4/ h 3c3。
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来源期刊
Advances in High Energy Physics
Advances in High Energy Physics PHYSICS, PARTICLES & FIELDS-
CiteScore
3.40
自引率
5.90%
发文量
55
审稿时长
6-12 weeks
期刊介绍: Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.
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