Ontology type: schema:ScholarlyArticle
2003-12
AUTHORSTs Venkova, R. M. Lieder, W. Gast, D. Bazzacco, G. de Angelis, E. Podsvirova, H. M. Jäger, L. Mihailescu, R. Menegazzo, S. Lunardi, C. Rossi Alvarez, C. Ur, T. Martinez, M. Axiotis, D. Napoli, W. Urban, T. Rzaca-Urban
ABSTRACT.High-spin states in the odd-proton nucleus 173Lu have been populated in a 170Er(7Li,4n) reaction and the emitted \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\gamma$\end{document}-radiation was detected with the GASP array. The favoured and unfavoured sequences of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\pi 1/2^- [541]$\end{document} band have been considerably extended. The favoured sequence does not show any indication of a band crossing up to a rotational frequency of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\approx$\end{document} 0.45 MeV. This is the largest crossing frequency ever observed for 1/2- [541] bands of odd-proton nuclei with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$67 \leq Z \leq 77$\end{document} and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$90 \leq N \leq 106$\end{document}. Previous Cranked Shell Model (CSM) calculations underestimate the crossing frequency by 100 keV. More... »
PAGES577-581
http://scigraph.springernature.com/pub.10.1140/epja/i2003-10068-4
DOIhttp://dx.doi.org/10.1140/epja/i2003-10068-4
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