scholarly journals Primary γ -ray intensities and γ -strength functions from discrete two-step γ -ray cascades in radiative proton-capture experiments

2020 ◽  
Vol 101 (4) ◽  
Author(s):  
P. Scholz ◽  
M. Guttormsen ◽  
F. Heim ◽  
A. C. Larsen ◽  
J. Mayer ◽  
...  
2021 ◽  
Vol 104 (1) ◽  
Author(s):  
M. Wiedeking ◽  
M. Guttormsen ◽  
A. C. Larsen ◽  
F. Zeiser ◽  
A. Görgen ◽  
...  
Keyword(s):  
Γ Ray ◽  

2019 ◽  
Vol 99 (5) ◽  
Author(s):  
C. P. Brits ◽  
K. L. Malatji ◽  
M. Wiedeking ◽  
B. V. Kheswa ◽  
S. Goriely ◽  
...  

2017 ◽  
Vol 146 ◽  
pp. 01010 ◽  
Author(s):  
K.L. Malatji ◽  
B.V. Kheswa ◽  
M. Wiedeking ◽  
F.L. Bello Garrote ◽  
C.P. Brits ◽  
...  

1991 ◽  
Vol 69 (6) ◽  
pp. 658-664 ◽  
Author(s):  
M. A. Islam ◽  
T. J. Kennett ◽  
W. V. Prestwich

The thermal neutron capture γ rays from natural molybdenum and ruthenium have been studied using a pair spectrometer and the tangential facility at the McMaster University Nuclear Reactor. Precise transition, level, and neutron separation energies of different isotopes are inferred. The separation energies are: Sn(93Mo) = 8069.76 ± 0.09, Sn(95Mo) = 7369.10 ± 0.10, Sn(96Mo) = 9154.31 ± 0.05, Sn(97Mo) = 6821.15 ± 0.25, Sn(98Mo) = 8642.55 ± 0.07, Sn(99Mo) = 5925.42 ± 0.15, Sn(100Ru) = 9673.48 ± 0.05, and Sn(102Ru) = 9219.64 ± 0.05 keV. The M1 strength functions of 100Ru,102Ru, 96Mo, and 98Mo are (34 ± 15) × 10−9, (82 ± 41) × 10−9, (22 ± 7) × 10−9, and (25 ± 8) × 10−9 MeV−3, respectively. All values but that for 102Ru agree with the global average of (20 ± 6) × 10−9 MeV−3. The average [Formula: see text] of 96Mo observed is 247 ± 175 e2 fm4 MeV−1.


1974 ◽  
Vol 52 (2) ◽  
pp. 131-139 ◽  
Author(s):  
R. L. Schulte ◽  
J. D. King ◽  
H. W. Taylor

A total of 22 resonances has been observed in the 44Ca(p,γ)45Sc reaction within the incident proton energy range of 600 to 930 keV. Gamma-ray singles spectra and γ-ray angular distribution data were accumulated for resonances at Ep = 856 and 906 keV. Both of these resonant states have been found to have spin 3/2. The measured angular distributions of primary γ rays from the resonant states have given spin information on the intermediate bound states of 45Sc with excitation energies above 2 MeV. A γ-ray decay scheme has been derived from the γ-ray spectra. The data indicate new levels at 2151.0, 3525.2, 3548.5, 3584.0, and 3714.3 keV.


2008 ◽  
Author(s):  
A. C. Larsen ◽  
M. Guttormsen ◽  
R. Chankova ◽  
F. Ingebretsen ◽  
T. Lönnroth ◽  
...  

2008 ◽  
Author(s):  
A. C. Larsen ◽  
M. Guttormsen ◽  
R. Chankova ◽  
F. Ingebretsen ◽  
T. Lönnroth ◽  
...  
Keyword(s):  
Γ Ray ◽  

2010 ◽  
Vol 81 (2) ◽  
Author(s):  
A. Voinov ◽  
S. M. Grimes ◽  
C. R. Brune ◽  
M. Guttormsen ◽  
A. C. Larsen ◽  
...  

2015 ◽  
Vol 24 (03) ◽  
pp. 1550018
Author(s):  
Bora Canbula ◽  
Sibel Erşan ◽  
Halil Babacan

γ-ray strength function is the key input for the photonuclear reactions, which have a special astrophysical importance, and should be renormalized by using the nuclear level density for calculating the theoretical average radiative capture width, but performing such renormalization is challenging for light nuclei. With this motivation, recently introduced level density parameter formula including collective effects is used to calculate the average radiative capture width of light nuclei, and therefore to renormalize their γ-ray strength functions. Obtained normalization factors are tested in (n, γ) reactions for the necessity of renormalization for light nuclei.


2007 ◽  
Vol 76 (4) ◽  
Author(s):  
A. C. Larsen ◽  
M. Guttormsen ◽  
R. Chankova ◽  
F. Ingebretsen ◽  
T. Lönnroth ◽  
...  

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