Gravitational collapse in f(R) gravity for a spherically symmetric spacetime admitting a homothetic Killing vector

The gravitational collapse of a spherical distribution, in a class of f® theories of gravity, where f® is power function of R, is discussed. The spacetime is assumed to admit a homothetic Killing vector. In the collapsing modes, some of the situations indeed hit a singularity, but they are all covered with an apparent horizon. Some peculiar cases are observed where the collapsing body settles to a constant radius at a given value of the radial coordinate.