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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… Click to show full 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.
Keywords:
stars rastall;
rotating compact;
compact stars;
gravity rapidly;
gravity;
rapidly rotating
Journal Title: Classical and Quantum Gravity
Year Published: 2021
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Journal Title: Classical and Quantum Gravity
Year Published: 2021
Link to full text (if available)
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recommendations!