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Иш: Accurate calibration of relativistic mean-field models: Correlating observables and providing meaningful theoretical uncertainties
A two-solar-mass neutron star measured using Shapiro delay
Paul B. Demorest, Timothy T. Pennucci, S. M. Ransom +2
Мақола201013 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 иқтибосABISelf-consistent mean-field models for nuclear structure
M. Bender, P.-H. Heenen, P.‐G. Reinhard
Мақола20035 иқтибосABIA chiral effective lagrangian for nuclei
R. J. Furnstahl, Brian D. Serot, Hua-Bin Tang
Мақола19973 иқтибосABINeutron radii of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>208</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Pb</mml:mi></mml:math>and neutron stars
C. J. Horowitz, J. Piekarewicz
Мақола20012 иқтибосABI