Rapidly rotating compact stars in Rastall's gravity
arXiv:2010.00086 · doi:10.1088/1361-6382/ac129d
Abstract
In this work we study rapidly rotating stars by considering the Rastall theory of gravity. We obtain and solve the equations by numerical methods for two usual parametrization of polytropic stars. Then the mass-radius relations, moments of inertia and other results of interest are obtained and compared with the ones for non-rotating stars.
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Cited by in corpus (4)
- Rapidly rotating neutron stars in gravity
- Compact stars in Rastall gravity: hydrostatic equilibrium and radial pulsations
- Quadratic Rastall Gravity: from low-mass HESS J1731-347 to high-mass PSR J0952-0607 pulsars
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