Cargando…
Surface energy of very neutron rich nuclei
For a microscopic model calculation of the nuclear surface-energy coefficient sigma the surface energy is defined as the energy loss of an uncharged, semiinfinite (inhomogeneous) two-component system compared to an infinite (homogeneous) system with the same particle asymmetry delta . Using the Thom...
Autor principal: | Von Groote, H |
---|---|
Lenguaje: | eng |
Publicado: |
CERN
1976
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.5170/CERN-1976-013.595 http://cds.cern.ch/record/873895 |
Ejemplares similares
-
Exotic decays in very light neutron-rich nuclei
por: García-Borge, M J, et al.
Publicado: (1993) -
In-beam gamma-ray spectroscopy with RIB on very neutron-rich nuclei
por: Ishihara, M
Publicado: (2000) -
Astrophysics with neutron-rich nuclei
por: Sorlin, O
Publicado: (1996) -
Structure of very neutron-rich nuclei: following the N=21 line
por: Nummela, S, et al.
Publicado: (2000) -
One-neutron knockout from light neutron-rich nuclei at relativistic energies
por: Rodriguez-Tajes, C, et al.
Publicado: (2010)