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51 ta ish
Ish: 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
Maqola199710 iqtibosABIIsospin asymmetry in nuclei and neutron stars
A.W. Steiner, M. Prakash, J.M. Lattimer +1
Maqola200510 iqtibosABIMedium modification of nucleon properties in the Skyrme model
A. M. Rakhimov, M. M. Musakhanov, F. C. Khanna +1
Maqola199810 iqtibosABIElectromagnetic form factors of bound nucleons revisited
U.T. Yakhshiev, U.-G. Meißner, A. Wirzba
Maqola20037 iqtibosABIAsymmetric nuclear matter: The role of the isovector scalar channel
Benye Liu, Vincenzo Greco, V. Baran +2
Maqola20026 iqtibosABIQCD sum rules in medium and the Okamoto-Nolen-Schiffer anomaly
Tetsuo Hatsuda, H. Högaasen, M. Prakash
Maqola19915 iqtibosABIIsospin Physics in Heavy-Ion Collisions at Intermediate Energies
Bao-An Li, Che Ming Ko, W. Bauer
Maqola19985 iqtibosABICharge symmetry breaking and the neutron-proton mass difference
Thomas Schäfer, Volker Koch, Gerald E. Brown
Maqola19935 iqtibosABI