论文标题
Kuchowicz公制功能对F（R，T）理论中的静电杆的影响
Impact of Kuchowicz Metric Function on Gravastars in f(R,T) Theory
论文作者
论文摘要
本文讨论了重力真空恒星或Gravastar的构型，并在$ f（r，t）$重力中存在几何和物质耦合的影响。 GRAVASTAR还概念化为黑洞的替代品，该黑洞由三种几何形状（1）内部几何形状，（2）中间薄壳和（3）外部几何形状说明。对于特定的$ f（r，t）$模型，我们分析了与kuchowicz公制功能相对应的这些几何形状。我们评估了内部结构域以及两个域非单一的中间壳的另一个度量电位。采用Schwarzschild指标来证明Grastar的外部几何形状，而未知常数的数值是通过边界条件计算的。最后，我们讨论了急性区域的不同特征，例如适当的长度，能量，表面红移以及状态参数方程。我们得出的结论是，在这种重力的背景下，Grastar模型可以被视为成功替换黑洞。
This paper discusses the configuration of gravitational vacuum star or gravastar with the impact of geometry and matter coupling present in $f(R,T)$ gravity. The gravastar is also conceptualized as a substitute for a black hole which is illustrated by three geometries known as (1) the interior geometry, (2) the intermediate thin-shell and (3) the exterior geometry. For a particular $f(R,T)$ model, we analyze these geometries corresponding to Kuchowicz metric function. We evaluate another metric potential for the interior domain as well as the intermediate shell which is non-singular for both domains. The Schwarzschild metric is adopted to demonstrate the exterior geometry of gravastar, while the numerical values of unknown constants are calculated through boundary conditions. Finally, we discuss different features of gravastar regions like proper length, energy, surface redshift as well as equation of state parameter. We conclude that the gravastar model can be regarded as a successful replacement of the black hole in the context of this gravity.
