论文标题
静态圆柱系统的复杂性因子在能量摩孔平方重力中
Complexity Factor for Static Cylindrical System in Energy-momentum Squared Gravity
论文作者
论文摘要
本文研究了一些物理特征，这些特征在自磨的静态圆柱结构中引起了复杂性，并在能量摩托明平方重力中的各向异性分布结合。为此，我们制定了修改的场方程并探索天文体的结构。还计算了C-能量和Tolman质量以讨论问题分布。然后，我们通过riemann张量的正交分裂获得一些结构标量。由于，考虑的结构的复杂性受到多种变量的影响，包括各向异性压力和不均匀的能量密度等。因此，我们采用因子$ \ Mathcal {y} _ {tf} $作为复杂性因子。此外，采用无复杂性条件以及Gokhroo-Mehra模型和状态的多面化方程来生成其相应的溶液。我们推断出包含此修改理论的其他术语会导致更复杂的系统。
This paper investigates some physical features that give rise to complexity within the self-gravitating static cylindrical structure coupled with anisotropic distribution in the energy-momentum squared gravity. To accomplish this, we formulate the modified field equations and explore the structure of the astronomical body. The C-energy and Tolman mass are also calculated to discuss the matter distribution. We then obtain some structure scalars via orthogonal splitting of the Riemann tensor. Since, the complexity of the considered structure is influenced by a variety of variables, including anisotropic pressure and inhomogeneous energy density, etc. thus, we adopt the factor $\mathcal{Y}_{TF}$ as the complexity factor. Further, the complexity-free condition along with the Gokhroo-Mehra model and polytropic equation of state are taken to generate their corresponding solutions. We deduce that the inclusion of additional terms of this modified theory leads to a more complicated system.
