On stability of a neutron star system in Palatini gravity

The European Physical Journal C, May 2018

We formulate the generalized Tolman–Oppenheimer–Volkoff equations for the $$f(\hat{R})$$ Palatini gravity in the case of static and spherical symmetric geometry. We also show that a neutron star can be a stable system independently of the form of the functional $$f(\hat{R})$$.

This is a preview of a remote PDF: https://link.springer.com/content/pdf/10.1140%2Fepjc%2Fs10052-018-5900-3.pdf

Aneta Wojnar. On stability of a neutron star system in Palatini gravity, The European Physical Journal C, 2018, 421, DOI: 10.1140/epjc/s10052-018-5900-3