Anisotropic fluid spheres admitting Karmarkar condition in f (G, T) gravity
This study deals with the construction of compact stars in f (G, T) gravity, where T and G
represent the trace of energy momentum tensor and Gauss-Bonnet term respectively. We
consider spherically symmetric space-time with anisotropic fluid distribution. In particular, the
Karmarkar condition to embed the spherically symmetric space-time into class-1 metric is
used to explore the compact stars solutions. Further, we choose two specific sets of
observational data, like LMC X-4 (mass= 1.29M/M⊙ & radii= 9.711 km), and EXO 1785-248 …
represent the trace of energy momentum tensor and Gauss-Bonnet term respectively. We
consider spherically symmetric space-time with anisotropic fluid distribution. In particular, the
Karmarkar condition to embed the spherically symmetric space-time into class-1 metric is
used to explore the compact stars solutions. Further, we choose two specific sets of
observational data, like LMC X-4 (mass= 1.29M/M⊙ & radii= 9.711 km), and EXO 1785-248 …
以上显示的是最相近的搜索结果。 查看全部搜索结果