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

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

2001-08-27

arxiv.org/abs/astro-ph/0108410v1

Phys.Rev. C64 (2001) 048801

Astronomy and Astrophysics

Astrophysics

4 pages, to appear in Physical Review C

Scientific paper

10.1103/PhysRevC.64.048801

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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