Gravitational collapse for anisotropic radiating star with Karmarkar condition in f (R, T) gravity
In this study, we are interested to investigate the dissipative gravitational collapse of
anisotropic spherically symmetric radiating star, which satisfies the initially static Karmarkar
condition in f (R, T) gravity. Moreover, we have chosen a linear model f (R, T)= f (R)+ f (T),
where R is Ricci scalar, T is trace of energy-momentum tensor and λ is dimensionless
coupling parameter. The terms f (R)= R and f (T)= 2 λ T describe the geometry and matter of
the radiating star, respectively. The complete set of the field equations for the radiating star …
anisotropic spherically symmetric radiating star, which satisfies the initially static Karmarkar
condition in f (R, T) gravity. Moreover, we have chosen a linear model f (R, T)= f (R)+ f (T),
where R is Ricci scalar, T is trace of energy-momentum tensor and λ is dimensionless
coupling parameter. The terms f (R)= R and f (T)= 2 λ T describe the geometry and matter of
the radiating star, respectively. The complete set of the field equations for the radiating star …
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