Power series and Padé approximants yield analytic approximations for mass and radius of compact stars from the TOV equations, applicable to affine, polytropic, and piecewise equations of state.
Evidence for a hard equation of state in the cores of neutron stars
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Series solutions to the TOV equations
Power series and Padé approximants yield analytic approximations for mass and radius of compact stars from the TOV equations, applicable to affine, polytropic, and piecewise equations of state.