How neutron stars constrain the nuclear equation of state

Thomas Hell; Bernhard Röttgers; Wolfram Weise

doi:10.1051/epjconf/20146604011

How neutron stars constrain the nuclear equation of state

Thomas Hell
, Bernhard Röttgers
, Wolfram Weise

Department of Physics

Technical University of Munich
ECT

Research output: Contribution to journal › Conference article › peer-review

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.

Original language	English
Article number	04011
Journal	EPJ Web of Conferences
Volume	66
DOIs	https://doi.org/10.1051/epjconf/20146604011
State	Published - 2014
Event	2013 International Nuclear Physics Conference, INPC 2013 - Firenze, Italy Duration: 2 Jun 2013 → 7 Jun 2013

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title = "How neutron stars constrain the nuclear equation of state",

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.",

author = "Thomas Hell and Bernhard R{\"o}ttgers and Wolfram Weise",

year = "2014",

doi = "10.1051/epjconf/20146604011",

language = "English",

volume = "66",

journal = "EPJ Web of Conferences",

issn = "2101-6275",

publisher = "EDP Sciences",

note = "2013 International Nuclear Physics Conference, INPC 2013 ; Conference date: 02-06-2013 Through 07-06-2013",

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TY - JOUR

T1 - How neutron stars constrain the nuclear equation of state

AU - Hell, Thomas

AU - Röttgers, Bernhard

AU - Weise, Wolfram

PY - 2014

Y1 - 2014

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/84898739173

U2 - 10.1051/epjconf/20146604011

DO - 10.1051/epjconf/20146604011

M3 - Conference article

AN - SCOPUS:84898739173

SN - 2101-6275

VL - 66

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

M1 - 04011

T2 - 2013 International Nuclear Physics Conference, INPC 2013

Y2 - 2 June 2013 through 7 June 2013

ER -

How neutron stars constrain the nuclear equation of state

Abstract

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