Abstract:
Relativistic stars’ equilibrium and stability evolved as an exciting aspect in both modified
theories of gravity and GR. When these systems reflect movements and make an effort
to maintain stability, they attract a lot of attention. The dynamical analysis of gravitating
systems plays key role in structure formation that is why astrophysicists and cosmologists
pay great attention in the discussion of stability range of gravitating sources.Here, we shall
analyze the stability of NSs by analyzing the evolution of hydrostatic equilibrium configu-
ration for the choice of EoS p =ω(ρ4B), with ω = 1
3 and B represents Bag constant. In this
scheme we pick the minimally coupled F(R, T ) gravity of the form F(R, T ) = R+2λT ,
λ stands as the coupling parameter. We will compare our results with recent observational
data
