γ-Ray Strength Functions and GDR Cross Sections in the IAEA Photonuclear Data Project

Author(s):  
H. Utsunomiya ◽  
I. Gheorghe ◽  
D. M. Filipescu ◽  
K. Stopani ◽  
S. Belyshev ◽  
...  
2017 ◽  
Vol 146 ◽  
pp. 01010 ◽  
Author(s):  
K.L. Malatji ◽  
B.V. Kheswa ◽  
M. Wiedeking ◽  
F.L. Bello Garrote ◽  
C.P. Brits ◽  
...  

2021 ◽  
Vol 104 (1) ◽  
Author(s):  
M. Wiedeking ◽  
M. Guttormsen ◽  
A. C. Larsen ◽  
F. Zeiser ◽  
A. Görgen ◽  
...  
Keyword(s):  
Γ Ray ◽  

2021 ◽  
Vol 104 (1) ◽  
Author(s):  
J. L. Ullmann ◽  
T. Kawano ◽  
B. Baramsai ◽  
T. A. Bredeweg ◽  
A. Couture ◽  
...  
Keyword(s):  

2002 ◽  
Vol 90 (2) ◽  
Author(s):  
I. Fatima ◽  
Jamshed H. Zaidi ◽  
Shujaat Ahmad ◽  
M. S. Subhani

SummaryEmploying the activation technique in combination with radiochemical separations and high-resolution γ-ray spectroscopy fission neutron spectrum averaged cross sections were measured for several (


2020 ◽  
pp. 148-153
Author(s):  
A.N. Vodin ◽  
O.S. Deiev ◽  
I.S. Timchenko ◽  
S.N. Olejnik ◽  
A.S. Kachan ◽  
...  

The flux-weighted averaged over the energy range of bremsstrahlung spectrum from reaction threshold up to the maximum energy of γ-ray cross-sections <σ(E)> of the 93Nb(γ,n)92mNb and 93Nb(γ,n)92tNb photonuclear reactions were determined by the gamma-activation method within the end-point bremsstrahlung energies Еmax = 36…91 MeV. Activation of 93Nb targets has been done by a bremsstrahlung flux using an electron beam at the linear accelerator LUE-40 at RDC "Accelerator" NSC KIPT. The γ-ray spectra of irradiated targets were registered using the HPGe detector with an energy resolution of 1.8 keV for the 1332 keV line 60Co. To control the bremsstrahlung flux we used natMo witness-targets and a reaction cross-section of 100Mo(γ,n)99Mo. Obtained experimental cross-sections <σ(E)> of the studied reactions are in good agreement with the theoretical values calculated within TALYS 1.9 code and the results of other authors. The averaged cross-sections <σ(E)> of the 93Nb(γ,n)92mNb and 93Nb(γ,n)92tNb reactions in the energy range 35...45 MeV and > 70 MeV were obtained for the first time.


2022 ◽  
Author(s):  
Huseynqulu Quliyev ◽  
Nilufer Demirci Saygı ◽  
Ekber Guliyev ◽  
Ali Akbar Kuliev

Abstract The excitation of pygmy dipole resonance (PDR) and giant dipole resonance (GDR) in even-even 154-164Dy isotopes is examined through quasiparticle random-phase approximation (QRPA) with the effective interactions that restores the broken translational and Galilean invariances. In each isotope, an electric response emerges by showing ample distribution at energies below and above 10 MeV. We, therefore, study the transition cross sections and probabilities, photon strength functions, transition strengths, isospin character, and collectivity of the predicted E1 responses.


1987 ◽  
Vol 65 (6) ◽  
pp. 691-698 ◽  
Author(s):  
O. Häusser

We present here recent [Formula: see text] results from TRIUMF that are relevant to the determination of spin-flip isovector strength functions in nuclei. Distortion factors needed for the extraction of nuclear-structure information have been deduced from cross sections and analyzing powers in elastic scattering for several energies and targets. Nonrelativistic optical potentials obtained by folding effective nucleon (N)–nucleus interactions with nuclear densities are found to overpredict both elastic and reaction cross sections, whereas Dirac calculations that include Pauli blocking are in good agreement with the data. Spin observables (Snn and Ay) for the quasi-elastic region in 54Fe[Formula: see text] at 290 MeV provide some evidence for the reduction of the effective proton mass predicted in relativistic mean-field theories as a consequence of the attractive scalar field in the nuclear medium. The energy dependence of the effective N–nucleus interaction at small momentum transfers has been investigated using isoscalar and isovector 1+ states in 28Si as probe states. We find that the cross sections for the isovector transitions are in good agreement with predictions for the dominant Vστ part of the Franey–Love interaction. Gamow–Teller (GT) strength functions have been obtained in 24Mg and 54Fe from measurements of both cross sections and spin–flip probabilities Snn. The spin-flip cross sections σSnn are particularly useful in heavier nuclei to discriminate against a continuous background of ΔS = 0 excitations. In the (s, d) shell where full shell-model wave functions are available, the GT quenching factors [Formula: see text] are in good agreement with those from recent (p, n) and (n, p) experiments. We show that a state-by-state comparison of (p, p′) and (e, e′) results has the potential of identifying pionic current contributions in (e, e′). The GT quenching factors in 54Fe are smaller than in the (s, d) shell probably because of severely truncated shell-model wave functions, particularly those of the nuclear ground state.


2001 ◽  
Vol 89 (11-12) ◽  
Author(s):  
J. Kuhnhenn ◽  
U. Herpers ◽  
W. Glasser ◽  
R. Michel ◽  
P. W. Kubik ◽  
...  

Some new cross sections for proton-induced radionuclide formation from lead are presented. The results extend the previous measurements from about 70 MeV down to threshold energies. Emphasis was placed upon an improved method of γ-ray spectrum analysis which proved to be reliable and effective. The new results are compared with model calculations on the basis of an improved hybrid model of preequilibrium reactions which is able to reproduce the near target products very well. But for more than 6 emitted nucleons, experimental measurements are superior.


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