Hybrid Stars that Masquerade as Neutron Stars

, , , and

© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Mark Alford et al 2005 ApJ 629 969 DOI 10.1086/430902

0004-637X/629/2/969

Abstract

We 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 for reasonable values of the bag model parameters. For nuclear matter, we use the equation of state calculated by Akmal and coworkers using many-body techniques. Both mixed and homogeneous phases of nuclear and quark matter are considered.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/430902