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Иш: Neutron-proton mass difference in finite nuclei and the Nolen-Schiffer anomaly
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 иқтибосABIElectromagnetic form factors of bound nucleons revisited
U.T. Yakhshiev, U.-G. Meißner, A. Wirzba
Мақола20037 иқтибосABIAsymmetric nuclear matter: The role of the isovector scalar channel
Benye Liu, Vincenzo Greco, V. Baran +2
Мақола20026 иқтибосABIQCD sum rules in medium and the Okamoto-Nolen-Schiffer anomaly
Tetsuo Hatsuda, H. Högaasen, M. Prakash
Мақола19915 иқтибосABIIsospin Physics in Heavy-Ion Collisions at Intermediate Energies
Bao-An Li, Che Ming Ko, W. Bauer
Мақола19985 иқтибосABICharge symmetry breaking and the neutron-proton mass difference
Thomas Schäfer, Volker Koch, Gerald E. Brown
Мақола19935 иқтибосABI