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Phys. Rev. C 74, 044309 (2006) [12 pages]

Extensive investigation of 0+ states in rare earth region nuclei

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D. A. Meyer1,7, V. Wood1, R. F. Casten1, C. R. Fitzpatrick1,2, G. Graw3, D. Bucurescu4, J. Jolie5, P. von Brentano5, R. Hertenberger3, H.-F. Wirth6, N. Braun5, T. Faestermann6, S. Heinze5, J. L. Jerke1, R. Krücken6, M. Mahgoub6, O. Möller5, D. Mücher5, and C. Scholl5
1Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06520-8124, USA
2University of Surrey, Guildford, United Kingdom
3Department für Physik, Ludwig-Maximilians-Universität München, D-85748 Garching, Germany
4National Institute of Physics and Nuclear Engineering, Bucharest, Romania
5Institut für Kernphysik, Universität zu Köln, D-50937 Köln, Germany
6Physik Department, Technische Universität München, D-85748 Garching, Germany
7Department of Physics, Rhodes College, Memphis, Tennessee 38112-1690, USA

Received 11 June 2006; published 24 October 2006

The nature of 0+ excitations, especially in transitional and deformed nuclei, has attracted new attention. Following a recent experiment studying 158Gd, we investigated a large group of nuclei in the rare-earth region with the (p,t) pickup reaction using the Q3D magnetic spectrograph at the University of Munich MP tandem accelerator laboratory. Outgoing tritons were recorded at various lab angles, and their angular distributions are compared to those calculated using the distorted-wave Born approximation. Using the unique shape of the L=0 angular distribution, more than double the number of 0+ states than were previously known are identified. The distribution of 0+ energies and cross sections is discussed in terms of collective and noncollective degrees of freedom, and the density of low-lying 0+ states is discussed as a corroboration of a characteristic feature of phase transition regions. The degree of level mixing, as extracted from Brody distribution fits to the energy spacings of adjacent 0+ levels, is also explored.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.74.044309
DOI:
10.1103/PhysRevC.74.044309
PACS:
21.10.Re, 24.10.Eq, 25.40.Hs, 27.70.+q