Total neutron cross sections and resonance parameters of175, 176Lu up to 200 eV

Kalebin, S. M.; Artamonov, V. S.; Ivanov, R. N.; Rukolaine, G. V.; Belanova, T. S.; Kolesov, A. G.; Poruchikov, V. A.

doi:10.1007/bf01118236

Cited by 9 publications

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“…IV A. The resonance parameters of the 176 Lu(n,γ) were determined by few sets of data from: Kalebin [15] up to 136 eV, Block [16] up to 46.7 eV, Vertebnyy [17] and Foote [40] up to 15 eV, Wider [19] from thermal neutron energy to 1.9 eV, and Brunner [18] for two first resonances.…”

Section: Resonance Region Up To 400 Evmentioning

confidence: 99%

“…The contribution of the resonance energy region to MACS is often determined by using the evaluated cross sections from data compilation as given by Kopecky [14]. For the 176 Lu isotope, resonance energies and neutron widths were obtained by Kalebin [15] in one important absolute measurement of transmission cross section up to 200 eV. These data are only overlapped by data up to 47 eV from Block [16], up to 12 eV from Vertebnyy [17] and up to 1.56 eV from Brunner [18] and Widder [19].…”

Section: Introductionmentioning

confidence: 99%

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Radiative neutron capture cross sections onLu176at DANCE

et al. 2016

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The cross section of the neutron capture reaction 176 Lu(n,γ) has been measured for a wide incident neutron energy range with the Detector for Advanced Neutron Capture Experiments at the Los Alamos Neutron Science Center. The thermal neutron capture cross section was determined to be (1967±137) b for one of the Lu natural isotopes, 176 Lu. The resonance part was measured and compared to the Mughabghab's atlas using the R-matrix code, SAMMY. At higher neutron energies the measured cross sections are compared to ENDF/B-VII.1, JEFF-3.2 and BRC evaluated nuclear data. The Maxwellian averaged cross sections in a stellar plasma for thermal energies between 5 keV and 100 keV were extracted using these data.

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Section: Resonance Region Up To 400 Evmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%