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19 April 2024
 
  » arxiv » nucl-th/0411016

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Hybrid stars that masquerade as neutron stars
Mark Alford ; Matt Braby ; Mark Paris ; Sanjay Reddy ;
Date 4 Nov 2004
Journal Astrophys.J. 629 (2005) 969-978
Subject nucl-th astro-ph hep-ph
AffiliationWashington Univ, St Louis), Matt Braby (Washington Univ, St Louis), Mark Paris (Jefferson National Laboratory), Sanjay Reddy (Los Alamos National Laboratory
AbstractWe show that a hybrid (nuclear + quark matter) star can have a mass-radius relationship very similar to that predicted for a star made of purely nucleonic matter. We show this for a generic parameterization of the quark matter equation of state, and also for an MIT bag model, each including a phenomenological correction based on gluonic corrections to the equation of state. We obtain hybrid stars as heavy as 2 M_solar for reasonable values of the bag model parameters. For nuclear matter, we use the equation of state calculated by Akmal, Pandharipande, and Ravenhall using many-body techniques. Both mixed and homogeneous phases of nuclear and quark matter are considered.
Source arXiv, nucl-th/0411016
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