← Ishga qaytish
Ushbu ish iqtibos qilgan ishlar
47 ta ish
Ish: Pure Neutron Matter Constraints and Nuclear Symmetry Energy
A Skyrme parametrization from subnuclear to neutron star densities
E. Chabanat, P. Bonche, P. Haensel +2
Maqola199710 iqtibosABIIsospin asymmetry in nuclei and neutron stars
A.W. Steiner, M. Prakash, J.M. Lattimer +1
Maqola200510 iqtibosABIEquation of state of nucleon matter and neutron star structure
A. Akmal, V. R. Pandharipande, D. G. Ravenhall
Maqola19989 iqtibosABIDetermination of the Equation of State of Dense Matter
Paweł Danielewicz, R. Lacey, W. G. Lynch
Maqola20028 iqtibosABINeutron 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
Maqola20015 iqtibosABI