6533b830fe1ef96bd1296ff4

RESEARCH PRODUCT

Tz=−1→0βdecays ofNi54,Fe50,Cr46, andTi42and comparison with mirror(He3,t)measurements

D. PauwelsJ. L. TainJ. J. Valiente-dobónHiroshi MatsubaraP. DoornenbalA. AlgoraA. AlgoraS. PietriS. VermaA. I. MoralesD. Pérez-loureiroM. GasconF. MolinaW. GelletlyJ. GrȩboszJ. GrȩboszH. J. WollersheimRobert HoischenAtsushi TamiiRajesh KumarYoshitaka FujitaStanislav TashenovE. GaniogluP. BoutachkovH. SchaffnerL. Amon SusamY. OktemA. GadeaC. Domingo-pardoC. Domingo-pardoB. RubioS. J. SteerW. ProkopowiczHans GeisselEnrique CasarejosI. KojouharovL. CaceresL. CaceresJ. AgramuntJ. BenlliureDirk RudolphR. B. CakirliN. KurzM. GórskaZs. PodolyákJ. Gerl

subject

PhysicsNuclear physicsNuclear and High Energy PhysicsFragmentation (mass spectrometry)High resolutionGamma spectroscopySensitivity limitAtomic physicsBeta decayExcitationCharge exchangeFermi Gamma-ray Space Telescope

description

We have studied the β decay of the Tz=−1, f7/2 shell nuclei Ni54, Fe50, Cr46, and Ti42 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. (Less)

https://doi.org/10.1103/physrevc.91.014301