Hybrid Stars that Masquerade as Neutron Stars
Author(s) -
Mark Alford,
Matt Braby,
Mark Paris,
Sanjay Reddy
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/430902
Subject(s) - physics , strange matter , equation of state , nuclear matter , quark star , neutron star , stars , solar mass , radius , particle physics , nuclear physics , quark , exotic star , star (game theory) , astrophysics , nucleon , quantum mechanics , computer security , computer science
We show that a hybrid (nuclear + quark matter) star can have a mass-radiusrelationship very similar to that predicted for a star made of purely nucleonicmatter. We show this for a generic parameterization of the quark matterequation of state, and also for an MIT bag model, each including aphenomenological correction based on gluonic corrections to the equation ofstate. We obtain hybrid stars as heavy as 2 M_solar for reasonable values ofthe bag model parameters. For nuclear matter, we use the equation of statecalculated by Akmal, Pandharipande, and Ravenhall using many-body techniques.Both mixed and homogeneous phases of nuclear and quark matter are considered.Comment: 22 pages, LaTeX. Extra figure and explanation adde
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