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Isospin impurity of the Isobaric Analogue State of super-allowed beta decay. experimental technique isospin impurity determination. Bertram Blank, CEN Bordeaux-Gradignan ESNT, Saclay, April, 26-29, 2011. The idea:. T, T z. Super-allowed b decay. T, T z - 1. Proton emission.
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Isospin impurity of the Isobaric Analogue State of super-allowed beta decay • experimental technique • isospin impurity determination Bertram Blank, CEN Bordeaux-Gradignan ESNT, Saclay, April, 26-29, 2011
The idea: T, Tz Super-allowed b decay T, Tz- 1 Proton emission Gamma decay T-3/2, Tz-3/2 T - 1, Tz- 1
The idea: 52Ni: T=2, Tz=-2 Super-allowed b decay 52Co: T=2, Tz=-1 Proton emission: T=1/2, Tz = -1/2 Gamma decay 51Fe: T=1/2, Tz=-1/2 T= ½ + ½ T = 1, Tz = -1 T = 2 Can one determine the isospin impurity of the IAS?
Proton-rich nuclei in the region of Ca to Ni • Mass region (20 Z 28 et Tz -3/2) • 5 experiments at GANIL • 23 isotopes studied (39Ti au 53Ni) • Calcium: 37,36Ca • Titanium: 41,40,39Ti • Vanadium: 43V • Chromium: 45,44,43,42Cr • Manganese : 47,46Mn • Iron: 49,48,47,46,45Fe • Cobalt: 51,50Co • Nickel: 53,52,51,50,49,48Ni • Copper: 55Cu • Zinc: 56,55,54Zn
GANIL / LISE3 2000 Primary beam: 58Ni @ 75 MeV/A intensity: 3 - 4 mAe spectrometer LISE3 : degrader Be (50 mm) Wien filter detection setup SISSI target: natNi 200 mg/cm2 silicon telescope identification of implanted fragments DSSSD (X-Y): 2 x 16 x 3 mm - veto for light particles - residual energy, x-y position - energy loss - time of flight: micro-channel plate detectors RF cyclotron
Identification projectile fragments 7 to 8 identification parameters
Radioactivity of 41Ti Radioactivity of 49Fe 41Ti 41Ti Correlation time 41Ti T 41Ti A Contaminant from 49Fe and 45Cr B1 B2 Protons Proton and gamma branching ratios and energies
Background subtraction for rays Before After 49Fe 49Fe Decay of 49Fe Contaminants Decay of 49Fe C. Dossat et al., NPA 792 (2007) 18
Spectroscopy of 52Ni T1/2 = (40.8 ± 0.2) ms Pp = (31.4 ± 1.5) % • Ep = (1349 ± 10) keV • Ip = (9.4 ± 1.3) % • Ep = (1057 ± 11) keV • Ip = (2.9± 0.3) % • Ep = (2815 ± 23) keV • Ip = (0.9 ± 0.4) % C. Dossat et al., NPA 792 (2007) 18
Ep = (1013 ± 12) keV • Ip = (1.8± 0.3) % • Ep = (1500-1900) keV • Ip = (2.0 ± 0.4) % • Ep = (2000-3000) keV • Ip = (1.4 ± 0.5) % Spectroscopy of 48Fe T1/2 = (40.8 ± 0.2) ms Pp = (31.4 ± 1.5) % C. Dossat et al., NPA 792 (2007) 18
X Isospin impurities • Proton emission from the IAS is isospin forbidden • Comparison of , and of for IAS : • 48Fe : =2.1 % - = 30%=42 % • 52Ni : =10 % - = 38%=64 % • Determination of isospin impurities with these experimental data: • (experimental, theory) • ’p : Coulomb and centrifugal barrier penetration • Sp = 1
Isospin impurity:example of 48Fe Shell model (48Mn) IAS • = 2.1 % • = 42 % • II = 0.52 % W.A. Richter, B.A. Brown
Isospin impurity: example of 52Ni Shell model (52Co) IAS • = 10 % • = 64 % • II = 19 % W.A. Richter, B.A. Brown
Isospin impurity of IAS • neighboring nuclei: surprising… • however: • shell-model study: • II(36Ca) = 0.4 %, II (40Ti) = 17.3 % (Theory Jyväskylä in sd shell) • similar treatment possible for many other nuclei: 45,44Cr, 46Mn, 49Fe, 53,51Ni…. II(48Fe) = 0.52 %, II (52Ni) = 19 % B.A. Brown, N. Smirnova….