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Neutron star and dense nuclear matter with phenomenological short distance repulsion.
Jesper Leong (University of Adelaide, Australia)
The nuclear equation of state is well known at the low-density from the study of finite nuclear. Conversely, perturbative QCD describes nuclear matter existing as deconfined quark-gluon plasma when the densities become extremely high. However, the intermediate range is yet to be determined. To nuclear theorist neutron stars are interesting because their core densities sit precisely in this region. Measurements …
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