Neutron Stars in Palatini and Theories
arXiv:2102.05722 · doi:10.1140/epjc/s10052-021-09662-z
Abstract
We study solutions of the stellar structure equations for spherically symmetric objects in Palatini and in the mass-radius region associated to neutron stars. We illustrate the potential impact of the and terms by studying a range of viable values of and . Similarly, we use different equations of state (SLy, FPS, HS(DD2) and HS(TMA)) as a simple way to account for the equation of state uncertainty. Our results show that for certain combinations of the and parameters and equation of state, the effect of modifications of general relativity on the properties of stars is sizeable. Therefore, with increasing accuracy in the determination of the equation of state for neutron stars, astrophysical observations may serve as discriminators of modifications of General Relativity.
arXiv comment13 pages, 18 figures. References added. Discussion around Fig. 18 extended. Agrees with published version
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