Speaker
Prof.
Hans Feldmeier
(GSI)
Description
Light nuclei are studied within the Fermionic Molecular Dynamics model.
An effective interaction based on the Argonne V18 interaction is used
for all nuclei. Short-range central and tensor correlations are treated
explicitly using a unitary correlation operator. The evolution of
cluster structures and halos with increasing neutron or proton number
or excitation energy is discussed. The astrophysical S-factor is
calculated for 3He(alpha,gamma)7Be radiative capture reaction in a
fully microscopic fashion. Other applications are the Hoyle type states
in 12C above the 3 alpha threshold or the two proton halo state in 17Ne.
Primary author
Prof.
Hans Feldmeier
(GSI)
Co-author
Dr
Thomas Neff
(GSI Darmstadt)
