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Tz = -1 → 0 β decays of 54Ni, 50Fe, 46Cr, and 42Ti and comparison with mirror (³He,t) measurements.

Authors :
Molina, F.
Rubio, B.
Fujita, Y.
Gelletly, W.
Agramunt, J.
Algora, A.
Benlliure, J.
Boutachkov, P.
Cáceres, L.
Cakirli, R. B.
Casarejos, E.
Domingo-Pardo, C.
Doornenbal, P.
Gadea, A.
Ganioğlu, E.
Gascón, M.
Geissel, H.
Gerl, J.
Górska, M.
Gr?bosz, J.
Source :
Physical Review C: Nuclear Physics. Jan2015, Vol. 91 Issue 1, p1-19. 19p.
Publication Year :
2015

Abstract

We have studied the β decay of the Tz = -1, f7/2 shell nuclei 54Ni, 50Fe, 46Cr, and 42Ti produced in fragmentation reactions. The proton separation energies in the daughter Tz = 0 nuclei are relatively large (≈4-5 MeV) so studies of the γ rays are essential. The experiments were performed at GSI as part of the Stopped-beam campaign with the RISING setup consisting of 15 Euroball Cluster Ge detectors. From the newly obtained high precision β-decay half-lives, excitation energies, and β branching ratios, we were able to extract Fermi and Gamow-Teller transition strengths in these β decays. With these improved results it was possible to compare in detail the Gamow-Teller (GT) transition strengths observed in beta decay including a sensitivity limit with the strengths of the Tz = +1 to Tz = 0 transitions derived from high resolution (³He,t) reactions on the mirror target nuclei at RCNP, Osaka. The accumulated B(GT) strength obtained from both experiments looks very similar although the charge exchange reaction provides information on a broader energy range. Using the "merged analysis" one can obtain a full picture of the B(GT) over the full Qβ range. Looking at the individual transitions some differences are observed, especially for the weak transitions. Their possible origins are discussed. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
05562813
Volume :
91
Issue :
1
Database :
Academic Search Index
Journal :
Physical Review C: Nuclear Physics
Publication Type :
Academic Journal
Accession number :
101136380
Full Text :
https://doi.org/10.1103/PhysRevC.91.014301