Improved Spectral Representations of Neutron-Star Equations of State

Abstract

Spectral representations have been shown to provide an efficient way to represent the poorly understood high-density portion of the neutron-star equation of state. This paper shows how the efficiency and accuracy of those representations can be improved by a very simple change.

5 pages, 6 figures

References in corpus (2)

• PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
• Spectral Representations of Neutron-Star Equations of State

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