κ-general-relativity I: a non-commutative GR theory with the κ-Minkowski spacetime as its flat limit

IF 3.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Daniel Rozental and Ofek Birnholtz
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引用次数: 0

Abstract

We employ a twist deformation of infinitesimal diffeomorphisms to construct a modification of general relativity on a non-commutative spacetime extending the local κ-Minkowski geometry. This spacetime arises in deformed special relativity (DSR) models, where a fundamental length scale is incorporated into SR as an effective description of quantum gravitational effects. To avoid the mathematical and physical inconsistencies associated with twisting the Poincaré group, we instead deform the dilatation-enlarged IGL(3,1) group, constructing a covariant and explicitly consistent gravitational theory (distinct from Weyl gravity). The relativistic consistency of the twisted κ-Minkowski spacetime is demonstrated, including deformed transformations and differential structures. A physically motivated Inönü–Wigner contraction procedure is suggested to enable a well-defined classical limit, addressing the correspondence issue. This framework provides a consistent foundation for a dynamical sector of DSR and allows, in future treatment, explicit computations that could advance phenomenological predictions.
广义相对论I:以广义-闵可夫斯基时空为平面极限的非交换广义相对论
我们利用无穷小微分同态的扭曲变形,在非交换时空上构造广义相对论的修正,扩展了局部的kb - minkowski几何。这种时空出现在变形的狭义相对论(DSR)模型中,其中基本长度尺度被纳入狭义相对论中,作为量子引力效应的有效描述。为了避免与扭曲庞卡洛群相关的数学和物理不一致,我们转而变形膨胀放大的IGL(3,1)群,构建一个协变和明确一致的引力理论(不同于Weyl引力)。证明了扭曲的κ-闵可夫斯基时空的相对论一致性,包括变形变换和微分结构。提出了一个物理驱动的Inönü-Wigner收缩过程,以实现定义良好的经典极限,解决对应问题。该框架为DSR的动态部分提供了一致的基础,并允许在未来的治疗中,可以推进现象学预测的显式计算。
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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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