Einstein-Gilbert-Straus solution of Einstein field equations: Timelike geodesic congruence with conventional and quantized fundamental metric tensor

IF 2.8 3区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS Nuclear Physics B Pub Date : 2025-05-01 Epub Date: 2025-03-13 DOI:10.1016/j.nuclphysb.2025.116866
Abdel Nasser Tawfik , Tahia F. Dabash , Tarek S. Amer , Mohamed O. Shaker
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Abstract

In a cosmic background characterized by inhomogeneity, anisotropy, and spherical symmetry, a nonsingular solution to the Einstein field equations is established through the application of both conventional and quantized fundamental metric tensor. The Swiss cheese model describes the complex configuration of the Einstein–Gilbert–Straus (EGS) metric, particularly emphasizing the presently undefined correlation between the radial distance r and cosmic time t. This complexity necessitates two key approaches: first, to model the cosmic substance inside the inhomogeneously interspersed spherical holes, and second, to analytically derive and numerically estimate the timelike geodesic congruence via the chain rule. In this analysis, the derivative dr/dt is calculated at the proper horizon, incorporating the proper-time derivative as proposed by Misner and Sharp. The Raychaudhuri equation serves as a crucial lemma in the context of the Hawking–Penrose singularity theorems. It provides significant insights into the dynamics of various kinematic quantities, including the expansion (volume scalar), shearing (anisotropy), rotation (vorticity), and the Ricci identity (local gravitational field). The Raychaudhuri equation describes how these quantities correlate and contribute to the characteristics and onset of space and initial singularities. To conclude, we find that a) a singularity-free solution is achieved in both space and time using either the conventional or quantized fundamental metric tensor, and b) the quantized fundamental metric tensor, which provides a significant extension of general relativity into relativistic and quantum regimes, naturally leads to the quantization of the Raychaudhuri equation, thereby greatly enhancing the strength of such a solution. The EGS metric exhibits significant differences from both the Schwarzschild and FLRW metrics, suggesting that the conclusion regarding the nonsingularity of the EGS is likely independent of the specific model employed. Additionally, the Ricci and Kretschmann scalars seem to provide evidence that the proposed geometric quantization reveals nonsingularity which is fundamentally real, intrinsic, and essential rather than an artifact arising from a specific choice of coordinates.
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爱因斯坦场方程的爱因斯坦-吉尔伯特-斯特劳斯解:与常规和量子化基本度量张量的类时测地线同余
在具有非均匀性、各向异性和球对称特征的宇宙背景下,通过应用常规和量子化基本度量张量,建立了爱因斯坦场方程的非奇异解。瑞士奶酪模型描述了爱因斯坦-吉尔伯特-斯特劳斯(EGS)度规的复杂构型,特别强调了目前未定义的径向距离r与宇宙时间t之间的相关性。这种复杂性需要两个关键方法:首先,对不均匀散布的球形孔内的宇宙物质进行建模,其次,通过链式法则解析推导并数值估计类时测地线同余。在这个分析中,导数dr/dt是在适当的视界上计算的,并结合Misner和Sharp提出的固有时导数。Raychaudhuri方程在霍金-彭罗斯奇点定理中是一个至关重要的引理。它提供了对各种运动量的动力学的重要见解,包括膨胀(体积标量)、剪切(各向异性)、旋转(涡度)和里奇恒等式(局部引力场)。Raychaudhuri方程描述了这些量如何相互关联,并对空间和初始奇点的特征和开始做出贡献。综上所述,我们发现a)使用常规或量子化的基本度量张量可以在空间和时间上获得无奇点解;b)量子化的基本度量张量将广义相对论显著扩展到相对论和量子体系,自然导致Raychaudhuri方程的量子化,从而大大增强了该解的强度。EGS指标与史瓦西和FLRW指标都有显著差异,这表明关于EGS非奇异性的结论可能与所采用的特定模型无关。此外,Ricci和Kretschmann标量似乎提供了证据,表明所提出的几何量子化揭示了非奇点,这是非奇点本质上是真实的、内在的和必要的,而不是由特定坐标选择产生的人工产物。
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来源期刊
Nuclear Physics B
Nuclear Physics B 物理-物理:粒子与场物理
CiteScore
5.50
自引率
7.10%
发文量
302
审稿时长
1 months
期刊介绍: Nuclear Physics B focuses on the domain of high energy physics, quantum field theory, statistical systems, and mathematical physics, and includes four main sections: high energy physics - phenomenology, high energy physics - theory, high energy physics - experiment, and quantum field theory, statistical systems, and mathematical physics. The emphasis is on original research papers (Frontiers Articles or Full Length Articles), but Review Articles are also welcome.
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