1992
DOI: 10.1016/0090-3752(92)80015-c
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Nuclear data sheets update for A = 183

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Cited by 48 publications
(11 citation statements)
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“…Transition intensities have been corrected for absorption in the source, as discussed earlier. The multipolarities in Table V are taken from ENSDF [43] where available, or assumed based on angular-momentum selection rules, and the conversion coefficients were recalculated with BRICC [16]. Figure 3 shows the population-depopulation balance for 183 W using the corresponding σ γ information from Table V calculated with various LD and PSF models.…”
Section: A 182 W(nγ ) 183 Wmentioning
confidence: 99%
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“…Transition intensities have been corrected for absorption in the source, as discussed earlier. The multipolarities in Table V are taken from ENSDF [43] where available, or assumed based on angular-momentum selection rules, and the conversion coefficients were recalculated with BRICC [16]. Figure 3 shows the population-depopulation balance for 183 W using the corresponding σ γ information from Table V calculated with various LD and PSF models.…”
Section: A 182 W(nγ ) 183 Wmentioning
confidence: 99%
“…The 11/2 + (T 1/2 = 5.2 s) isomer at 309.49 keV [43] decays by a highly converted 102.48-keV [43] M2 transition that was not resolved from the 101.93-keV transition deexciting the 308.95-keV level and the 101.80-keV transition deexciting the 302.35-keV level in 187 W, which also contributes to the observed intensity owing to a 0.5(1)% 186 W impurity (Table I) in the measured sample. The total intensity of the triplet is ∼15(2)% of the 209.69-keV TABLE V. Experimental partial γ -ray cross sections, corresponding to both primary and secondary γ -ray transitions, measured in this work from thermal neutron capture on 182 W. Quantities in brackets represent tentative assignments.…”
Section: A 182 W(nγ ) 183 Wmentioning
confidence: 99%
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“…(For ' Bi, both the ground-statetogroundstate n transition and the E3 Ml-(E2) y rays [10], which originate from 1.8-s ' Tl, have been seen). The adopted Tl [11]excitation energy of -550 keV, used by Coenen et ai. [5] to deduce the ' Bi energy of 60 keV, was initially derived by Schrewe et al [12] on the basis of systematics for vrd3/2 levels in heavier odd-mass Tl isotopes and an estimated energy for the E3 (9/2-3/2) transition.…”
mentioning
confidence: 99%
“…This estimate is based on the assumption that the 60(15)-ms ' Tl isomer deexcites only 3% of the time by n decay, with the remainder of its decay strength proceeding via emission of the F3 y ray. Clearly the adopted [11] and inferred [5] excitation energies for ' Tl and ' Bi™, respectively, are uncertain and therefore need to be determined experimentally.…”
mentioning
confidence: 99%