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Reconstructing the equation of state for cold nuclear matter from the relationship of any two properties of neutron stars

Tomohiro Harada
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Abstract

A direct method is developed to reconstruct the equation of state for high-density nuclear matter from the relationship between any two properties of neutron stars, such as masses, radii, moments of inertia, baryonic masses, binding energies, gravitational redshifts, and their combinations.

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Tomohiro Harada. 2001-08-27. Reconstructing the equation of state for cold nuclear matter from the relationship of any two properties of neutron stars. https://doi.org/10.1103/physrevc.64.048801

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