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 inne...

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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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spelling doaj-e176e2c918424f229c1f929f4e3715202021-08-02T16:04:07ZengEDP SciencesEPJ Web of Conferences2100-014X2014-03-01660401110.1051/epjconf/20146604011epjconf_inpc2013_04011How neutron stars constrain the nuclear equation of stateHell ThomasRöttgers Bernhard0Weise WolframPhysik Department, Technische Universität München 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. http://dx.doi.org/10.1051/epjconf/20146604011
collection DOAJ
language English
format Article
sources DOAJ
author Hell Thomas
Röttgers Bernhard
Weise Wolfram
spellingShingle Hell Thomas
Röttgers Bernhard
Weise Wolfram
How neutron stars constrain the nuclear equation of state
EPJ Web of Conferences
author_facet Hell Thomas
Röttgers Bernhard
Weise Wolfram
author_sort Hell Thomas
title How neutron stars constrain the nuclear equation of state
title_short How neutron stars constrain the nuclear equation of state
title_full How neutron stars constrain the nuclear equation of state
title_fullStr How neutron stars constrain the nuclear equation of state
title_full_unstemmed How neutron stars constrain the nuclear equation of state
title_sort how neutron stars constrain the nuclear equation of state
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2014-03-01
description 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.
url http://dx.doi.org/10.1051/epjconf/20146604011
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AT rottgersbernhard howneutronstarsconstrainthenuclearequationofstate
AT weisewolfram howneutronstarsconstrainthenuclearequationofstate
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