1 / 3

Constraints to Universal Energy Density Functionals by Giant Resonances

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.

leroy
Download Presentation

Constraints to Universal Energy Density Functionals by Giant Resonances

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Constraints to Universal Energy Density Functionals by Giant Resonances H. Sagawa, University of Aizu

  2. Correlations between neutron matter EPS and neutron skin thickness Importance to determine neutron skin thickness RMF SHF

  3. 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

More Related