How neutron stars constrain the nuclear equation of state [PDF]
Hell Thomas, Bernhard Roettgers, Wolfram WeiseRecent neutron star observations set new constraints for the equation of state of baryonic matter. A chiral effective field theory approach is used for the description of neutron-dominated nuclear matter present in the outer core of neutron stars. Possible hybrid stars with quark matter in the inner core are discussed using a three-flavor Nambu--Jona-Lasinio model.View original: http://arxiv.org/abs/1307.4582
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