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Иш: Pure Neutron Matter Constraints and Nuclear Symmetry Energy
A 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 иқтибосABIEquation of state of nucleon matter and neutron star structure
A. Akmal, V. R. Pandharipande, D. G. Ravenhall
Мақола19989 иқтибосABIDetermination of the Equation of State of Dense Matter
Paweł Danielewicz, R. Lacey, W. G. Lynch
Мақола20028 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