FROM NEUTRON STAR OBSERVABLES TO THE EQUATION OF STATE. I. AN OPTIMAL PARAMETRIZATION

FROM NEUTRON STAR OBSERVABLES TO THE EQUATION OF STATE. I. AN OPTIMAL PARAMETRIZATION

The increasing number and precision of measurements of neutron star masses, radii, and, in the near future, moments of inertia offer the possibility of precisely determining the neutron star equation of state (EOS). One way to facilitate the mapping of observables to the EOS is through a parametriza...

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Bibliographic Details
Main Authors:	Raithel, Carolyn A., Özel, Feryal, Psaltis, Dimitrios
Other Authors:	Univ Arizona, Dept Astron
Language:	en
Published:	IOP PUBLISHING LTD 2016
Subjects:	equation of state stars: interiors stars: neutron
Online Access:	http://hdl.handle.net/10150/622054 http://arizona.openrepository.com/arizona/handle/10150/622054

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