How neutron stars constrain the nuclear equation of state

How neutron stars constrain the nuclear equation of state

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...

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Bibliographic Details
Main Authors:	Hell Thomas, Röttgers Bernhard, Weise Wolfram
Format:	Article
Language:	English
Published:	EDP Sciences 2014-03-01
Series:	EPJ Web of Conferences
Online Access:	http://dx.doi.org/10.1051/epjconf/20146604011

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