Models of non-static and inhomogeneous gravitating source in Rastall gravity
Abstract
In this paper, we have explored the non-static anisotropic gravitational collapse and expansion solutions in Rastall theory of gravity. The field equations have been formulated for the non-static and inhomogeneous gravitating source. The Misner–Sharp mass function, auxiliary solution and trapped condition have been used to obtained a trapped surface. The auxiliary solutions have been used to obtain the expansion and collapse solutions; these solutions depend on and parameter (which appears due to parametric form of metric components); also the range of parameter has been examined. The expansion scalar depends on parameter , in the case of expansion for , while for collapse with . Also, the dynamics of the gravitating spherical source has been discussed graphically with the effects of Rastall parameter . For the physically reasonable fluid, the validity of energy conditions has been discussed for expansion and collapse solutions with the various values of .