Equilibrium of slowly rotating polytropes in modified theories of gravity
pith:V6DLI2ISopen to challenge →
classification
gr-qc
astro-ph.SR
keywords
gravitymodifiedrotatingslowlytheoriesanalyticalclassdensity
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A general formalism to find the density profile of a slowly rotating stellar object in modified gravity is presented. We derive a generic Lane-Emden equation and its analytical solution for a wide class of modified theories of gravity.
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