scholarly journals Shell-model studies of the astrophysical rp -process reactions S34(p,γ)Cl35 and Cl34g,m(p,γ)Ar35

2020 ◽  
Vol 102 (2) ◽  
Author(s):  
W. A. Richter ◽  
B. A. Brown ◽  
R. Longland ◽  
C. Wrede ◽  
P. Denissenkov ◽  
...  
Keyword(s):  
2020 ◽  
Vol 1643 ◽  
pp. 012064
Author(s):  
W. A. Richter ◽  
B. Alex Brown ◽  
R. Longland ◽  
C. Wrede ◽  
C. Fry ◽  
...  
Keyword(s):  

2013 ◽  
Vol 25 (13) ◽  
pp. 135404 ◽  
Author(s):  
R A Casali ◽  
J Lasave ◽  
M A Caravaca ◽  
S Koval ◽  
C A Ponce ◽  
...  

2017 ◽  
Vol 92 (6) ◽  
pp. 063001 ◽  
Author(s):  
Noritaka Shimizu ◽  
Takashi Abe ◽  
Michio Honma ◽  
Takaharu Otsuka ◽  
Tomoaki Togashi ◽  
...  

2011 ◽  
Vol 66 (2) ◽  
pp. 283-286 ◽  
Author(s):  
W.A. Richter ◽  
B. Alex Brown ◽  
A. Signoracci ◽  
M. Wiescher
Keyword(s):  

2001 ◽  
Vol 79 (2) ◽  
pp. 241-292 ◽  
Author(s):  
J.L. FISKER ◽  
V. BARNARD ◽  
J. GÖRRES ◽  
K. LANGANKE ◽  
G. MARTÍNEZ-PINEDO ◽  
...  

2015 ◽  
Vol 91 (2) ◽  
Author(s):  
Andrei Neacsu ◽  
Mihai Horoi
Keyword(s):  

1973 ◽  
Vol 51 (7) ◽  
pp. 737-742 ◽  
Author(s):  
G. Do Dang ◽  
J. A. Rabbat

The structure of the low-lying states of 56Ni is studied in the frameworks of the Hartree–Fock theory and the shell model. Attention is focused on the choice of the single particle energies and the effect of highly excited states. It is found that the low-lying states can reasonably be described by the shell model with 1p–1h and 2p–2h excitations from the 1f7/2 level. A critical discussion of the contradictory results of previous works is made and their connection with the present work is pointed out.


2001 ◽  
Author(s):  
C. VOLPE ◽  
N. AUERBACH ◽  
G. COLÒ ◽  
T. SUZUKI ◽  
N. VAN GIAI
Keyword(s):  

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