180 likes | 325 Views
Proton emission from deformed rare earth nuclei. Robert Page. AREA. µ. t. e. 1. /. 2. Simple model for spherical proton emitters. Proton decay of 160 Re. Q p = 1271 keV. Proton emission as a spectroscopic tool. 160 Re Half-life (ms) E p ( keV ) d 3/2 h 11/2 Expt
E N D
Proton emission from deformed rare earth nuclei Robert Page
AREA µ t e 1 / 2 Simple model for spherical proton emitters Proton decay of 160Re Qp = 1271 keV
Proton emission as a spectroscopic tool 160Re Half-life (ms) Ep (keV) d3/2h11/2Expt 1263 0.24480 0.67 h11/2 d3/2
Deformed proton emitters 135Tb P.J. Woods et al., PRC69 (2004) 051302
Known Proton Emitters B. Blank & M.J.G. Borge, Progress in Particle and Nuclear Physics 60 (2008) 403
Why are there so few known proton emitters in this region? Known Proton Emitters Selectivity Yield B. Blank & M.J.G. Borge, Progress in Particle and Nuclear Physics 60 (2008) 403
Counts (106) / 10 keV Decay Particle Energy (MeV) Implantation – proton – alpha correlation
The proton emitter 159Re Counts / 10 keV t1/2 = 21 ms Decay Particle Energy (MeV) D.T. Joss et al., Physics Letters B641 (2006) 34
Implantation – proton correlations 50Cr + 92Mo → 135Tb + p6n Argonne FMA A = 135 only 60 mm thick DSSD P.J. Woods et al., PRC69 (2004) 051302
Beta-decay half-lives Moller, Nix & Kratz, Atomic Data & Nuclear Data Tables 66 (1997) 131
Fusion-evaporation reactions Compound nuclei
Fusion-evaporation pxn reactions ~3 nb ~30 mb
(Super-)FRS A & Z separation AIDA Isomer g decays or known p for unique A & Z identification Selectivity
Atomic number Z = 3.6 / hour = 0.6 / week Neutron number N Predicted Super FRS Yields @ 1012/s Yield
Predicted Super FRS Yields @ 1012/s Yield Atomic number Z = 3.6 / hour = 0.6 / week Neutron number N
Some physics opportunities • New proton emitters • Weak proton-decay branches • Proton-decay fine structure • Precision measurements • Beta-delayed gamma spectroscopy
Outstanding questions • Background from b and bp decays • (1 mm thick DSSDs cf. 60 mm) • Identify best physics cases • Choose best primary beam • Your input is welcome... Robert Page