On stability of a neutron star system in Palatini gravity
classification
🌀 gr-qc
hep-th
keywords
gravityneutronpalatinistarsystemcaseequationsform
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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 is a stable system independently of the form of the functional $f(\hat{R})$
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