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

Journal Article · Tue Apr 05 04:00:00 EDT 2005 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.1905301· OSTI ID:20630828

Dinca, D -C; Campbell, C M; Cook, J M; Oiliver, H; Starosta, K; Terry, J R ^[1]; Janssens, R V.F.; Zhu, S; Carpenter, M P; Hammond, N J; Lauritsen, T; Lister, C J; Moore, E F; Seweryniak, D ^[2]; Gade, A; Bazin, D; Glasmacher, T; Lecouey, J -L; Mueller, W F; Yoneda, K ^[3]

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1. Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States)
2. Physics Division, Argonne National Laboratory, Argonne, IL 60439 (United States)
3. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI 48824 (United States); and others

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.

• OSTI ID: 20630828
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 764; ISSN APCPCS; ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ANL
COULOMB EXCITATION
DEEP INELASTIC SCATTERING
NEUTRON-RICH ISOTOPES
NEUTRONS
SUPERCONDUCTING CYCLOTRONS
TITANIUM ISOTOPES