fQ引力中的偶极宇宙学

IF 5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Andronikos Paliathanasis
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引用次数: 0

摘要

对称远平行 f(Q)引力允许在康托夫斯基-萨克斯几何中存在具有倾斜速度的完美流体。在这个偶极模型中,我们考虑了理想气体,并研究了物理参数的演变。通过场方程的非对角方程,倾斜参数受到非线性函数 f(Q) 的约束。我们发现,动力学总是还原为 STEGR 的真空解。这包括 f(Q) 函数没有引入宇宙学项的卡斯纳宇宙,以及 fQ 扮演宇宙学常数角色的各向同性德西特宇宙。在极端倾斜极限中,宇宙始终是各向异性和加速的。然而,最终解与 STEGR 的解相吻合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dipole cosmology in fQ-gravity

Symmetric teleparallel f(Q)-gravity allows for the presence of a perfect fluid with a tilted velocity in the Kantowski–Sachs geometry. In this dipole model, we consider an ideal gas and we investigate the evolution of the physical parameters. The tilt parameter is constrained by the nonlinear function f(Q) through the non-diagonal equations of the field equations. We find that the dynamics always reduce to the vacuum solutions of STEGR. This includes the Kasner universe, when no cosmological term is introduced by the f(Q) function, and the isotropic de Sitter universe, where fQ plays the role of the cosmological constant. In the extreme tilt limit, the universe is consistently anisotropic and accelerated. However, the final solution matches that of STEGR.

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来源期刊
Physics of the Dark Universe
Physics of the Dark Universe ASTRONOMY & ASTROPHYSICS-
CiteScore
9.60
自引率
7.30%
发文量
118
审稿时长
61 days
期刊介绍: Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact. The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.
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