scholarly journals Stellar reaction rate forMg22+p→Al23from the asymptotic normalization coefficient in the mirror nuclear systemNe22+n→Ne23

2010 ◽  
Vol 81 (3) ◽  
Author(s):  
T. Al-Abdullah ◽  
F. Carstoiu ◽  
X. Chen ◽  
H. L. Clark ◽  
C. Fu ◽  
...  
Keyword(s):  
Reaction Rate ◽  
Asymptotic Normalization ◽  
Asymptotic Normalization Coefficient ◽  
Stellar Reaction Rate

scholarly journals Total Cross Section of the n+11B Reaction

2020 ◽  
Vol 4 ◽  
pp. 13
Author(s):  
G. Galios ◽  
G. Doukelis ◽  
S. Kossionides ◽  
T. Paradellis
Keyword(s):  
Total Cross Section ◽  
Cross Section ◽  
Reaction Rate ◽  
Neutron Cross Section ◽  
Total Neutron ◽  
Cross Section Data ◽  
Total Neutron Cross Section ◽  
Section Data ◽  
Upper Limit ◽  
Stellar Reaction Rate

The total neutron cross section of 11Β has been measured from 7.2 to 8.4 MeV. The analysis of all data from the 8Li(α,n0)11Β reaction in combination with the total cross section data can determine an upper limit on the stellar reaction rate of the 8Li(a,n)11Β reaction.

INVESTIGATIONS ON THE NUCLEAR HALO STRUCTURES

2008 ◽  
Vol 17 (09) ◽  
pp. 1729-1738
Author(s):  
YU-JIE LIANG ◽  
ZU-HUA LIU ◽  
HONG-YU ZHOU
Keyword(s):  
Mean Field ◽  
Light Nuclei ◽  
Halo Nuclei ◽  
Asymptotic Normalization ◽  
Relativistic Mean Field ◽  
Asymptotic Normalization Coefficient ◽  
Nuclear Halo ◽  
Coulomb Effects ◽  
Qualitative Analyses

The halo structures in some light nuclei are investigated systemically with the nuclear asymptotic normalization coefficient (ANC) method and the relativistic mean-field (RMF) theory. Some important results about the halo structures in mirror nuclei are obtained, and some qualitative analyses are made to explore the role of Coulomb effects on the formation of proton halo nuclei.

Stellar Reaction Rate of 14N(p,γ)15O+

1986 ◽  
pp. 431-434 ◽  
Author(s):  
U. Schröder ◽  
H. W. Becker ◽  
J. Görres ◽  
C. Rolfs ◽  
H. P. Trautvetter ◽  
...  
Keyword(s):  
Reaction Rate ◽  
Stellar Reaction Rate

scholarly journals Asymptotic normalization coefficient for α+d →6Li from the peripheral direct capture d(α,γ)6 reaction and the astrophysical S factor at Big Bang energies

2020 ◽  
Vol 227 ◽  
pp. 02016
Author(s):  
K.I. Tursunmakhatov ◽  
R. Yarmukhamedov ◽  
S.B. Igamov
Keyword(s):  
Big Bang ◽  
Asymptotic Normalization ◽  
Direct Capture ◽  
Asymptotic Normalization Coefficient ◽  
S Factor ◽  
Low Energies

The results of the analysis of the new experimental astrophysical S factors Sexp24(E) [D. Trezzi, et al., Astropart. Phys. 89, 57 (2017)] and those measured earlier [R. G. Robertson, et al., Phys. Rev. Lett. 47, 1867 (1981)] for the nuclear-astrophysical d(α,γ)6Li reaction directly measured at extremely low energies E, are presented. New estimates and their uncertainties have been obtained for values of the asymptotic normalization coefficient for α + γ → 6Li and for the direct astrophysical S factors at Big Bang energies.

scholarly journals Asymptotic normalization coefficient method for two-proton radiative capture

2020 ◽  
Vol 811 ◽  
pp. 135852
Author(s):  
L.V. Grigorenko ◽  
Yu.L. Parfenova ◽  
N.B. Shulgina ◽  
M.V. Zhukov
Keyword(s):  
Radiative Capture ◽  
Asymptotic Normalization ◽  
Asymptotic Normalization Coefficient ◽  
Coefficient Method
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