Spectral Chebyshev representations of neutron-star equations of state with strong first-order phase transitions are generally somewhat more accurate than piecewise analytic representations with the same number of parameters, and both converge roughly as 1/N.
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Representing Equations of State With Strong First-Order Phase Transitions
Spectral Chebyshev representations of neutron-star equations of state with strong first-order phase transitions are generally somewhat more accurate than piecewise analytic representations with the same number of parameters, and both converge roughly as 1/N.