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Constraints to Universal Energy Density Functionals by Giant Resonances. H. Sagawa, University of Aizu. Correlations between neutron matter EPS and neutron skin thickness. Importance to determine neutron skin thickness. RMF. SHF. Model independent observation of neutron skin.
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Constraints to Universal Energy Density Functionals by Giant Resonances H. Sagawa, University of Aizu
Correlations between neutron matter EPS and neutron skin thickness Importance to determine neutron skin thickness RMF SHF
Model independent observation of neutron skin Sum Rule of Charge Exchange Spin Dipole Excitations by (p,n) and (n,p) on 90Zr Observed sum rule value ⇒ e scattering & proton form factor