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|Title:||Neutron star properties from an NJL model modified to simulate confinement|
|Citation:||QCD Down Under: Proceedings of the Workshop on Quantum Chromodynamics, Adelaide, Australia, 10–19 March 2004 / Ayşe Kızılersű, Anthony W. Thomas and Anthony G. Williams (eds.), pp. 29-33|
|Conference Name:||Workshop on Quantum Chromodynamics (2004 : Adelaide, Australia)|
|S. Lawley, W. Bentz and A. W. Thomas|
|Abstract:||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.|
|Description:||Also cited as: Nuclear Physics B: Proceedings Supplements, 2005; 141: 29-33|
|Rights:||© 2004 Elsevier B.V.|
|Appears in Collections:||Chemistry and Physics publications|
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