Thursday, July 18, 2013

1307.4582 (Hell Thomas et al.)

How neutron stars constrain the nuclear equation of state    [PDF]

Hell Thomas, Bernhard Roettgers, Wolfram Weise
Recent 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.
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