Spherically symmetric solutions in gravity and gravitational repulsion

Spherically symmetric solutions in F ( R ) theories in astronomical systems with rising energy density are studied. The range of parameters is established for which the flat space–time approximation for the background metric is valid. For the solutions in which the curvature scalar oscillates with large amplitude and high frequency, found in our previous papers, it is shown that the analysis of the Jeans instability is strongly modified. It is discovered that for large astronomical objects modified gravity can be repulsive, so such objects would shrink forming relatively thin shells instead of quasi uniform bodies.