High-spin spectroscopy of natural and unnatural parity states in the mirror-pair 45V/45Ti
Bentley, M. A., Chandler, C., Bednarczyk, P., Brandolini, F., Bruce, A. M., Curien, D., Dorvaux, O., Ekman, J., Farnea, E., Gelletly, W., Joss, D. T., Lenzi, S. M., Napoli, D. R., Nyberg, J., O'Leary, C. D., Williams, S. J. and Warner, D. D. (2006) High-spin spectroscopy of natural and unnatural parity states in the mirror-pair 45V/45Ti Physical Review C, 73 (024304).
High-spin states in the proton-rich nucleus 45V have been identified for the first time. A comprehensive gamma-ray decay scheme has been established following an experiment performed at the Vivitron accelerator at IReS Strasbourg by using the Euroball gamma-ray detector array coupled to the Neutron Wall and Euclides detector arrays. The natural (negative-) parity scheme is identified up to the f7/2 band termination in addition to a positive-parity collective structure based on a d3/2 particle-hole excitation. Comparison of this scheme with that of the mirror partner, 45Ti, has yielded detailed information on the variation of Coulomb energy as a function of excitation energy and angular momentum. This is the first time that such an analysis has been performed for a collective structure built on a cross-shell excitation. Comparison of the observed Coulomb energies with those predicted by large-scale shell-model calculations is presented. In this case, unusually, the calculations do not fare as well as for heavier nuclei in the shell. In addition, stark differences between the two nuclei are observed for the decay intensities of the parity-changing E1 decays that de-excite the positive-parity deformed bands.
|Divisions :||Faculty of Engineering and Physical Sciences > Physics|
|Date :||8 February 2006|
|Identification Number :||https://doi.org/10.1103/PhysRevC.73.024304|
|Additional Information :||Published in Physical Review C, 73, 024304 (2006). © 2006 The American Physical Society.|
|Depositing User :||Mr Adam Field|
|Date Deposited :||27 May 2010 14:06|
|Last Modified :||23 Sep 2013 18:26|
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