Microscopic nuclear structure and nuclear reactions at intermediate energies

1995 ◽  
Vol 45 (4-5) ◽  
pp. 395-438 ◽  
Author(s):  
Peter U. Sauer ◽  
Guido Thamm
2005 ◽  
Vol 93 (9-10) ◽  
Author(s):  
Hiroshi Matsumura ◽  
Toshiya Sanami ◽  
Kazuyoshi Masumoto ◽  
Noriaki Nakao ◽  
Akihiro Toyoda ◽  
...  

SummaryThe yields of


2005 ◽  
Vol 14 (01) ◽  
pp. 85-93 ◽  
Author(s):  
PETR NAVRÁTIL

There has been significant progress in the ab initio approaches to the structure of light nuclei. One such method is the ab initio no-core shell model (NCSM). Starting from the realistic two- and three-nucleon interactions, this method can predict the low-lying levels in p-shell nuclei. It is a challenging task to extend the ab initio methods to describe nuclear reactions. In this contribution, we present a brief overview of the NCSM with examples of recent applications as well as the first steps taken toward nuclear reaction applications.


2020 ◽  
Vol 31 (1) ◽  
Author(s):  
Huan Nhut Phan

Nuclear reactions of proton by light nuclei at low energies play a key role in the study ofnucleosynthesis which is of interest in nuclear astrophysics. The most fundamental process whichis very necessary is the elastic scattering. In this work, we construct a microscopic proton-nucleuspotential in order to describe the differential cross-sections over scattering angles of the protonelastic scattering by 12C and 13C in the range of available energies 14 - 22 MeV. The microscopicoptical potential is based on the folding model using the effective nucleon-nucleon interactionCDM3Yn. The results show the promising use of the CDM3Yn interactions at low and very lowenergies, which were originally used for nuclear reactions at intermediate energies. This could bethe premise for the study of nuclear reactions using CDM3Yn interaction in astrophysics at lowenergies.


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