On stability of a neutron star system in Palatini gravity
Abstract We formulate the generalized Tolman–Oppenheimer–Volkoff equations for the $$f(\hat{R})$$ f(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 $$f(\hat{R})$$ f(R^) ....
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| Format: | Article |
| Language: | English |
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SpringerOpen
2018-05-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-5900-3 |