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Spectroscopic factor and proton formation probability for the d3/2 proton emitter 151mLu

Authors :
Wang, F.
Sun, B. H.
Liu, Z.
Page, R. D.
Qi, C.
Scholey, C.
Ashley, S. F.
Bianco, L.
Cullen, I. J.
Darby, I. G.
Eeckhaudt, S.
Garnsworthy, A. B.
Gelletly, W.
Gomez-Hornillos, M. B.
Grahn, T.
Greenlees, P. T.
Jenkins, D. G.
Jones, G. A.
Jones, P.
Joss, D. T.
Julin, R.
Juutinen, S.
Ketelhut, S.
Khan, S.
Kishada, A.
Leino, M.
Niikura, M.
Nyman, M.
Pakarinen, J.
Pietri, S.
Podolyak, Z.
Rahkila, P.
Rigby, S.
Saren, J.
Shizuma, T.
Sorri, J.
Steer, S.
Thomson, J.
Thompson, N. J.
Uusitalo, J.
Walker, P. M.
William, S.
Zhang, H. F.
Zhang, W. Q.
Zhu, L. H.
Source :
Physics Letters B 770 (2017) 83
Publication Year :
2017

Abstract

The quenching of the experimental spectroscopic factor for proton emission from the short-lived $d_{3/2}$ isomeric state in $^{151m}$Lu was a long-standing problem. In the present work, proton emission from this isomer has been reinvestigated in an experiment at the Accelerator Laboratory of the University of Jyv\"{a}skyl\"{a}. The proton-decay energy and half-life of this isomer were measured to be 1295(5) keV and 15.4(8) $\mu$s, respectively, in agreement with another recent study. These new experimental data can resolve the discrepancy in the spectroscopic factor calculated using the spherical WKB approximation. Using the R-matrix approach it is found that the proton formation probability indicates no significant hindrance for the proton decay of $^{151m}$Lu.<br />Comment: 6 pages, 5 figures

Subjects

Subjects :
Nuclear Experiment
Nuclear Theory

Details

Database :
arXiv
Journal :
Physics Letters B 770 (2017) 83
Publication Type :
Report
Accession number :
edsarx.1704.06394
Document Type :
Working Paper
Full Text :
https://doi.org/10.1016/j.physletb.2017.04.034