Cfl-Quark Star in the Density-Dependent Quark Mass Model

Details Cfl-Quark Star in the Density-Dependent Quark Mass Model Cfl-Quark Star in the Density-Dependent Quark Mass Model

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ara..conf..129o&link_type=abstract

ASTRONOMY AND RELATIVISTIC ASTROPHYSICS New Phenomena and New States of Matter in the Universe. Proceedings of the Third Worksho

Astronomy and Astrophysics

Astrophysics

Quark Star, Superconducting Color-Flavour Locked Phase, Strange Quark Matter

Scientific paper

The static spherically symmetric quark star structure is calculated by using an equation of state which takes into account the superconducting Color-Flavor Locked (CFL) phase of the strange quark matter. Some fundamental aspects of QCD (asymptotic freedom and confinement) are considered by using the phenomenological density-dependent quark mass model. We discuss the influence of model parameters on the conventional mass-radius relationship of a quark star structure. Massive quark stars are found due to the stiffness of the equation of state at low densities.

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