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Neutron-Rich Ti Isotopes And Possible N = 32 And N = 34 Shell Gaps.

Authors :
Dinca, D.-C.
Janssens, R. V. F.
Gade, A.
Fornal, B.
Zhu, S.
Bazin, D.
Broda, R.
Campbell, C. M.
Carpenter, M. P.
Chowdhury, P.
Cook, J. M.
Daly, P. J.
Deacon, A. N.
Freeman, S. J.
Glasmacher, T.
Grabowski, Z. W.
Hammond, N. J.
Kondev, F. G.
Królas, W.
Lauritsen, T.
Source :
AIP Conference Proceedings. 2005, Vol. 764 Issue 1, p131-135. 5p.
Publication Year :
2005

Abstract

The possible occurrence of sub-shell gaps at N = 32 and N = 34 in neutron-rich titanium isotopes is discussed in light of new experimental results from (i) deep-inelastic reactions measured with Gammasphere at the ATLAS facility at Argonne National Laboratory and from (ii) intermediate-energy Coulomb excitation performed at the National Superconducting Cyclotron Laboratory at Michigan State University. © 2005 American Institute of Physics [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0094243X
Volume :
764
Issue :
1
Database :
Academic Search Index
Journal :
AIP Conference Proceedings
Publication Type :
Conference
Accession number :
16932915
Full Text :
https://doi.org/10.1063/1.1905301