g Factor of the 7− isomer in 126Sn and first observation of spin-alignment in relativistic fission

We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-align...

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Veröffentlicht in:Physics letters. B 2010-04, Vol.687 (4-5), p.305-309
Hauptverfasser: Ilie, G., Neyens, G., Simpson, G.S., Jolie, J., Blazhev, A., Grawe, H., Lozeva, R.L., Vermeulen, N., Atanasova, L., Balabanski, D.L., Becker, F., Bednarczyk, P., Brandau, C., Caceres, L., Chamoli, S.K., Daugas, J.M., Doornenbal, P., Gerl, J., Górska, M., Grȩbosz, J., Hass, M., Ionescu-Bujor, M., Jungclaus, A., Kmiecik, M., Kojouharov, I., Kurz, N., Maj, A., Mallion, S., Perru, O., Pfützner, M., Podolyák, Zs, Prokopowicz, W., De Rydt, M., Saito, T.R., Schaffner, H., Turzó, K., Walker, J., Werner-Malento, E., Wollersheim, H.J.
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Sprache:eng
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Zusammenfassung:We report on the g factor measurement of the isomeric 7− state (E*=2219 keV, T1/2=5.9(8) μs) in the neutron-rich 126Sn nucleus. The nucleus was produced by the fission of a relativistic 238U beam and reaction products were selected by the FRS fragment separator at GSI. For the first time, spin-alignment was observed after relativistic fission. It was used to deduce the g factor of the 7− isomeric state, g(7−)=−0.098(9), from the measured perturbed angular distribution of its γ decay using the RISING Cluster detectors. The observed value confirms the suggested ν(h11/2−1d3/2−1) dominant configuration, which has been proposed for the 7− isomers in neutron-rich Sn isotopes. The failure of the g factor additivity rule and the importance of core polarization evolution with increasing distance from the doubly-magic 132Sn is discussed. The first observation of 18(8)% of spin-alignment produced by the relativistic fission of a 238U beam paves the way to study moments of neutron-rich (sub-)microsecond isomers, which are difficult to align by other means.
ISSN:0370-2693
1873-2445
DOI:10.1016/j.physletb.2010.03.033