Improved Spectral Representations of Neutron-Star Equations of State
arXiv:2202.12285 · doi:10.1103/PhysRevD.105.063031
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.
arXiv comment5 pages, 6 figures
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