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Иш: Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars
A two-solar-mass neutron star measured using Shapiro delay
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Мақола201013 иқтибосABIA Skyrme parametrization from subnuclear to neutron star densities
E. Chabanat, P. Bonche, P. Haensel +2
Мақола199710 иқтибосABIIsospin asymmetry in nuclei and neutron stars
A.W. Steiner, M. Prakash, J.M. Lattimer +1
Мақола200510 иқтибосABIDetermination of the Equation of State of Dense Matter
Paweł Danielewicz, R. Lacey, W. G. Lynch
Мақола20028 иқтибосABIAsymmetric nuclear matter: The role of the isovector scalar channel
Benye Liu, Vincenzo Greco, V. Baran +2
Мақола20026 иқтибосABINeutron Star Structure and the Neutron Radius of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>P</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>208</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mi>b</mml:mi></mml:math>
C. J. Horowitz, J. Piekarewicz
Мақола20015 иқтибосABI