论文标题
电荷对$ f（r，\ textbf {t}^{2}）$ fragity中静态球的复杂性的影响
Impact of Charge on the Complexity of Static Sphere in $f(R,\textbf{T}^{2})$ Gravity
论文作者
论文摘要
本文调查了在能量摩托明平方重力背景下充满各向异性物质的带电静态球的复杂性。为此，我们评估了修改的场和保护方程式以确定天体系统的结构。质量函数是通过misner-sharp以及Tolman质量定义计算的。自我塑造系统的复杂性取决于不同因素，例如各向异性压力，电磁场，能量密度不均匀性等。我们通过riemann张量的正交分解来制定结构标量，以开发包含Stellar结构所有重要特征的复杂性因子。通过设置等于零的复杂性因子来实现消失的复杂性条件。最后，我们通过利用Gokhroo-Mehra溶液的能量密度以及状态的多极热方程以及零复杂性条件来构建两种静态溶液。发现电磁场降低了恒星结构的复杂性。
This paper investigates the complexity of a charged static sphere filled with anisotropic matter in the background of energy-momentum squared gravity. For this purpose, we evaluate the modified field and conservation equations to determine the structure of celestial system. The mass function is calculated through Misner-Sharp as well as Tolman mass definitions. The complexity of a self-gravitating system depends on different factors such as anisotropic pressure, electromagnetic field, energy density inhomogeneity, etc. We formulate the structure scalars by the orthogonal decomposition of the Riemann tensor to develop a complexity factor containing all vital features of the stellar structure. The vanishing complexity condition is achieved by setting the complexity factor equal to zero. Finally, we construct two static solutions by utilizing the energy density of Gokhroo-Mehra solution as well as the polytropic equation of state along with the zero complexity condition. It is found that electromagnetic field decreases the complexity of stellar structure.
