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Biennial Report 2005-2007 - Saha Institute of Nuclear Physics

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44 <strong>Biennial</strong> <strong>Report</strong> <strong>2005</strong>-072.2.1.3 Sub-Barrier Coulomb Excitation <strong>of</strong> 110 Sn and its implications for the 100 Snshell closureWe had performed an experiment at CERN, REX-ISOLDE to measure B(E2; 0 + → 2 + ) <strong>of</strong> unstable106,108,110 Sn isotopes by ‘safe’ Coulomb excitation in inverse kinematics. The γ-rays were detectedby MINIBALL detector array in coincidence with 110 Sn detected in very forward angle (for safeCoulomb excitation) by double sided silicon strip detector. The B(E2; 0 + → 2 + ) <strong>of</strong> 110 Sn, obtainedfrom detailed data analysis is 0.22(0.022)e 2 b 2 . This strengthens the observation <strong>of</strong> the evoluation<strong>of</strong> the B(E2) values <strong>of</strong> neutron deficient Sn isotopes that has been observed recently in intermediateenergy Coulomb excitation <strong>of</strong> 108 Sn. It implies that the trend <strong>of</strong> these reduced transition probabilitiesin the even-even Sn isotopes is not symmetric with respect to midshell mass number A=116as 100 Sn (N=Z) is approached.J Cederkaell†, A Ekstrom†, C Fahlander†, A Hurst†, M Hjorth-Jensen†, F Ames†, A Banu†, PButler†, T Davinson†, U Datta Pramanik, J Eberth†, S Franchoo†, G Georgiev†, M Gorka† etalNAP2.2.1.4 Dipole strength measurements in the 130,132 Sn at GSI, Darmstadt, GermanyProperties <strong>of</strong> the Giant Dipole Resonance in the nuclei far <strong>of</strong>f stability provide information on theisospin dependence <strong>of</strong> effective nuclear interaction. However, as theoretically predicted for neutronrichnuclei, a low-lying dipole strength is expected below normal GDR region. The existence <strong>of</strong>such low-lying strength would have pronounced consequences for astrophysical r-process scenarios.Measurements <strong>of</strong> the dipole strength functions in neutron-rich nuclei around doubly magic nucleus130,132 Sn were performed with LAND-FRS facility at GSI. The beam <strong>of</strong> 132 Sn and about 20 otherisotopes <strong>of</strong> similar A/Z ratio were produced by in flight fission <strong>of</strong> 238 U primary beam. The secondarybeams with energies around 500 MeV/A were separated by FRS and transfer to cave-B whereprojectiles were excited by means <strong>of</strong> Coulomb excitation in a secondary lead target. The momenta<strong>of</strong> the neutrons and fragments after dissociation were measured by LAND-setup detectors. Inaddition to the giant dipole resonance, a resonance-like structure (pigmy resonance) is observed atlower excitation energy around 10 MeV which can be new dipole mode due to oscillation betweenexcess neutrons and core.P Adrich†, A Klimkiewicz†, M Fallot†, T Aumann†, K Boretzky†, U Datta Pramanik, H Emling†,H Geissel†, M Hellstroem†, KL Jones†, JV Kratz†, R Kulessa†, Y Leifels†, C Nociforo†, R Palit†,H Simon†, K Suemmerer†, W Walus†NAP2.2.1.5 Study <strong>of</strong> room background at the laboratory <strong>of</strong> SINP through γ-ray spectroscopyWe have studied the room background through γ-ray spectroscopy. The characteristic γ-rays <strong>of</strong>the nuclei were detected using semiconductor (HPGe) and scintillator (CsI, NaI) detectors. Wehave observed members <strong>of</strong> Thorium, Uranium series <strong>of</strong> natural background. In addition to thenaturally occurring activities, background also consists <strong>of</strong> some fission products activities whichoriginated with atmospheric fallout from past weapons testing; 137 Cs, 125 Sb, 95 Zr, 95 Nb etc. Weobserved that passive Pb shielding was not useful for low energy background reduction in gamma-

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