Erratum: Shell-model studies of the astrophysical rapid-proton-capture reactionP30(p,γ)S31[Phys. Rev. C89, 062801(R) (2014)]

2015 ◽  
Vol 92 (6) ◽  
Author(s):  
B. Alex Brown ◽  
W. A. Richter ◽  
C. Wrede
2013 ◽  
Vol 25 (13) ◽  
pp. 135404 ◽  
Author(s):  
R A Casali ◽  
J Lasave ◽  
M A Caravaca ◽  
S Koval ◽  
C A Ponce ◽  
...  

2012 ◽  
Vol 21 (08) ◽  
pp. 1250074 ◽  
Author(s):  
CHIRASHREE LAHIRI ◽  
G. GANGOPADHYAY

Densities from relativistic mean field calculations are applied to construct the optical potential and, hence calculate the endpoint of the rapid proton capture (rp) process. Mass values are taken from a new phenomenological mass formula. Endpoints are calculated for different temperature-density profiles of various X-ray bursters. We find that the rp process can produce significant quantities of nuclei upto around mass 95. Our results differ from existing works to some extent.


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

2016 ◽  
Vol 58 (1) ◽  
Author(s):  
D. Hove ◽  
E. Garrido ◽  
A. S. Jensen ◽  
H. O. U. Fynbo ◽  
D. V. Fedorov ◽  
...  
Keyword(s):  

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

1995 ◽  
Vol 74 (23) ◽  
pp. 4611-4614 ◽  
Author(s):  
B. Blank ◽  
S. Andriamonje ◽  
S. Czajkowski ◽  
F. Davi ◽  
R. Del Moral ◽  
...  

2011 ◽  
Vol 106 (25) ◽  
Author(s):  
A. M. Rogers ◽  
M. A. Famiano ◽  
W. G. Lynch ◽  
M. S. Wallace ◽  
F. Amorini ◽  
...  

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.


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