γ-ray strength function forSn116,117with the pygmy dipole resonance balanced in the photoneutron and neutron capture channels

2009 ◽  
Vol 80 (5) ◽  
Author(s):  
H. Utsunomiya ◽  
S. Goriely ◽  
M. Kamata ◽  
T. Kondo ◽  
O. Itoh ◽  
...  
JETP Letters ◽  
2016 ◽  
Vol 104 (6) ◽  
pp. 374-379 ◽  
Author(s):  
O. I. Achakovskiy ◽  
S. P. Kamerdzhiev ◽  
V. I. Tselyaev

2010 ◽  
Author(s):  
M. Kamata ◽  
H. Utsunomiya ◽  
H. Akimune ◽  
T. Yamagata ◽  
O. Itoh ◽  
...  

1974 ◽  
Vol 52 (11) ◽  
pp. 989-998 ◽  
Author(s):  
E. D. Earle ◽  
M. A. Lone ◽  
G. A. Bartholomew ◽  
W. J. McDonald ◽  
K. H. Bray ◽  
...  

Gamma ray spectra following the capture of 0.7, 1.7, and 2.6 MeV neutrons in Tl and Hg, of 0.7 and 2.6 MeV neutrons in Ta, and of 2.6 MeV neutrons in Au were measured with a NaI detector. The spectral distributions were obtained by unfolding the detector response function, and γ-ray strength functions were deduced for Tl, Au, and Ta by a spectrum fitting method. The strength functions in Tl and Au, when compared with the Lorentzian predictions, show a strong decrease below ~5 MeV and in Tl there is a resonance-like structure at ~5.5 MeV. No such structure is found in the strength function for Ta. This behavior is qualitatively interpreted in terms of recent particle–hole calculations.


1990 ◽  
Vol 68 (11) ◽  
pp. 1237-1242 ◽  
Author(s):  
M. A. Islam ◽  
T. J. Kennett ◽  
W. V. Prestwich

The thermal neutron capture gamma rays from the reaction 139La(n, γ)140La were investigated using a pair spectrometer and the tangential facility at the McMaster University Nuclear Reactor. A large number of previously unreported transitions have been observed from which details of the 140La structure are inferred. The level density is found to be consistent with a statistical model encompassing nuclear temperature. The reduced E1 strength function of 140La was found to be (1.4 ± 0.4) × 10−9 MeV−3. The giant dipole resonance model seems to overestimate the E1 strength in this nucleus. The separation energy of 140La is found to be 5161.00 ± 0.05 keV.


2020 ◽  
Vol 125 (10) ◽  
Author(s):  
M. Spieker ◽  
A. Heusler ◽  
B. A. Brown ◽  
T. Faestermann ◽  
R. Hertenberger ◽  
...  

2013 ◽  
Vol 906 ◽  
pp. 94-107 ◽  
Author(s):  
V. Derya ◽  
J. Endres ◽  
M. Elvers ◽  
M.N. Harakeh ◽  
N. Pietralla ◽  
...  

2010 ◽  
Vol 25 (34) ◽  
pp. 2905-2913 ◽  
Author(s):  
KUTSAL BOZKURT

We investigate isovector pygmy dipole resonance (IVPDR) for the case of neutron-rich nuclei 68 Ni , 130 Sn and 134 Sn using effective nucleon–nucleon Skyrme interaction. We use the Hartree–Fock–Bogoliubov (HFB) theory and employ the (quasiparticle) random phase approximation (Q)RPA. We calculate and compare the PDR strength in the PDR energy region for the case of density dependent central and full interaction modes for RPA and QRPA calculations. We observe that the results for the pygmy dipole resonance for neutron-rich soft nuclei 68 Ni that we consider are in reasonable agreement with their experimental results in both interactions and calculations. We also study the PDR for highly neutron-rich heavy nuclei, such as 130 Sn and 134 Sn . We see that only the QRPA calculation with full interaction is in good agreement with the experimental results for these nuclei and with a recent study in the literature. We find that the PDR strength distribution sensitively depends on the chosen interaction modes, especially for the neutron-rich heavy nuclei 134 Sn .


2009 ◽  
Author(s):  
A. Avdeyenkov ◽  
F. Gruemmer ◽  
S. Kamerdzhiev ◽  
S. Krewald ◽  
N. Lyutorovich ◽  
...  

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