TY  - JOUR
AU  - Guadilla, V.
AU  - Algora, A.
AU  - Tain, J. L.
AU  - Agramunt, J.
AU  - Jordan, D.
AU  - Monserrate, M.
AU  - Montaner-Piza, A.
AU  - Orrigo, S. E. A.
AU  - Rubio, B.
AU  - Valencia, E.
PY  - 2019
DA  - 2019//
TI  - Total absorption gamma-ray spectroscopy of niobium isomers
T2  - Phys. Rev. C
JO  - Physical Review C
SP  - 024311
EP  - 15pp
VL  - 100
IS  - 2
PB  - Amer Physical Soc
AB  - The beta-intensity distributions of the decays of Nb-100gs,Nb-100m and Nb-102gs,Nb-102m have been determined using the total absorption gamma-ray spectroscopy technique. The JYFLTRAP double Penning trap system was employed in a campaign of challenging measurements performed with the decay total absorption gamma-ray spectrometer at the Ion Guide Isotope Separator On-Line facility in Jyvaskyla. Different strategies were applied to disentangle the isomeric states involved, lying very close in energy. The low-spin component of each niobium case was populated through the decay of the zirconium parent, which was treated as a contaminant. We have applied a method to extract this contamination, and additionally we have obtained beta-intensity distributions for these zirconium decays. The beta-strength distributions evaluated with these results were compared with calculations in a quasiparticle random-phase approximation, suggesting a prolate configuration for the ground states of Zr-100,Zr-102. The footprint of the Pandemonium effect was found when comparing our results for the analyses of the niobium isotopes with previous decay data. The beta-intensities of the decay of Nb-102m, for which there were no previous data, were obtained. A careful evaluation of the uncertainties was carried out, and the consistency of our results was validated taking advantage of the segmentation of our spectrometer. The final results were used as input in reactor summation calculations. A large impact on antineutrino spectrum calculations was already reported, and here we detail the significant impact on decay heat calculations.
SN  - 2469-9985
UR  - https://arxiv.org/abs/1904.07036
UR  - https://doi.org/10.1103/PhysRevC.100.024311
DO  - 10.1103/PhysRevC.100.024311
LA  - English
N1  - WOS:000480237600001
ID  - Guadilla_etal2019
ER  -