Neutron Star Properties from an NJL Model Modified to Simulate Confinement

Details Neutron Star Properties from an NJL Model Modified to Simulate Confinement Neutron Star Properties from an NJL Model Modified to Simulate Confinement

2004-09-30

arxiv.org/abs/nucl-th/0409073v1

Nucl.Phys.Proc.Suppl.141:29-33,2005

Physics

Nuclear Physics

Nuclear Theory

5 pages, 6 figures, to be published in the proceedings for QCD Down Under Workshop, Adelaide, March 10-19, 2004

Scientific paper

10.1016/j.nuclphysbps.2004.12.00

The NJL model has recently been extended with a method to simulate
confinement. This leads in mean field approximation to a natural mechanism for
the saturation of nuclear matter. We use the model to investigate the equation
of state of asymmetric nuclear matter and then use it to compute the properties
of neutron stars.

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