We formulate the generalized Tolman-Oppenheimer-Volkoff equations for the f(R^) Palatini gravity in the case of static and spherical symmetric geometry. We also show that a neutron star is a stable system independently of the form of the functional f(R^)
@article{arxiv.1712.01943,
title = {On stability of a neutron star system in Palatini gravity},
author = {Aneta Wojnar},
journal= {arXiv preprint arXiv:1712.01943},
year = {2018}
}