How neutron stars constrain the nuclear equation of state
Hell Thomas, Röttgers Bernhard, Weise Wolfram
EPJ Web of Conferences · 2014
doi:10.1051/epjconf/20146604011 (opens in a new tab)
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Abstract
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.
Abstract licence: CC BY
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