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...
| Main Authors: | , , |
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| Language: | en |
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IOP PUBLISHING LTD
2016
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| Online Access: | http://hdl.handle.net/10150/622054 http://arizona.openrepository.com/arizona/handle/10150/622054 |