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Öğe High-spin states and lifetimes in S-33 and shell-model interpretation in the sd-fp space(American Physical Society, 2017) Aydın, Sezgin; Ionescu-Bujor, M.; Gavrilov, G. Tz.; Dimitrov, B. I.; Lenzi, Silvia M.; Recchia, Francesco; Tonev, Dimitar; Bouhelal, Mouna; Kavillioglu, F.; Pavlov, P.; Bazzacco, D.; Bizzeti, P. G.; Bizzeti-Sona, A. M.; de Angelis, G.; Deloncle, I.; Farnea, E.; Gadea, A.; Gottardo, A.; Goutev, N.; Haas, F.; Huyuk, T.; Laftchiev, H.; Lunardi, S.; Marinov, Tz. K.; Mengoni, D.; Menegazzo, R.; Michelagnoli, C.; Napoli, D. R.; Petkov, P.; Sahin, E.; Singh, P. P.; Stefanova, E. A.; Ur, C. A.; Valiente-Dobon, J. J.; Yavahchova, M. S.The structure of the S-33 nucleus was investigated in the Mg-24(N-14, alpha p) fusion-evaporation reaction using a 40-MeV N-14 beam. The level scheme was extended up to an excitation energy of 11.7 MeV and spin 19/2+. Lifetimes of the intermediate-and high-spin states have been investigated by the Doppler shift attenuation method. Data were compared with different shell-model calculations where effective interactions involving two main shells, the sd and the fp, are used.Öğe High-Spin Structure in K-40(American Physical Society, 2012) Soderstrom, P. -A.; Recchia, F.; Nyberg, J.; Gadea, A.; Lenzi, S. M.; Poves, A.; Atac, A.; Aydın, Sezgin; Bazzacco, D.; Bednarczyk, P.; Bellato, M.; Birkenbach, B.; Bortolato, D.; Boston, A. J.; Boston, H. C.; Bruyneel, B.; Bucurescu, D.; Calore, E.; Cederwall, B.; Charles, L.; Chavas, J.; Colosimo, S.; Crespi, F. C. L.; Cullen, D. M.; de Angelis, G.; Desesquelles, P.; Dosme, N.; Duchene, G.; Eberth, J.; Farnea, E.; Filmer, F.; Gorgen, A.; Gottardo, A.; Grebosz, J.; Gulmini, M.; Hess, H.; Hughes, T. A.; Jaworski, G.; Jolie, J.; Joshi, P.; Judson, D. S.; Jungclaus, A.; Karkour, N.; Karolak, M.; Kempley, R. S.; Khaplanov, A.; Korten, W.; Ljungvall, J.; Lunardi, S.; Maj, A.; Maron, G.; Meczynski, W.; Menegazzo, R.; Mengoni, D.; Michelagnoli, C.; Molini, P.; Napoli, D. R.; Nolan, P. J.; Norman, M.; Obertelli, A.; Podolyak, Zs.; Pullia, A.; Quintana, B.; Redon, N.; Regan, P. H.; Reiter, P.; Robinson, A. P.; Sahin, E.; Simpson, J.; Salsac, M. D.; Smith, J. F.; Stezowski, O.; Theisen, Ch.; Tonev, D.; Unsworth, C.; Ur, C. A.; Valiente-Dobon, J. J.; Wiens, A.High-spin states of K-40 have been populated in the fusion-evaporation reaction C-12(Si-30,np)K-40 and studied by means of gamma-ray spectroscopy techniques using one triple-cluster detector of the Advanced Gamma Tracking Array at the Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro. Several states with excitation energy up to 8 MeV and spin up to 10(-) have been discovered. These states are discussed in terms of J = 3 and T = 0 neutron-proton hole pairs. Shell-model calculations in a large model space have shown good agreement with the experimental data for most of the energy levels. The evolution of the structure of this nucleus is here studied as a function of excitation energy and angular momentum.Öğe High-spin structure in K-40(APS Physics, 2012) Aydın, Sezgin; Soderstrom, P. A.; Recchia, F.; Nyberg, J.; Gadea, A.; Lenzi, S. M.; Poves, A.; Atac, A.; Bazzacco, D.High-spin states of K-40 have been populated in the fusion-evaporation reaction C-12(Si-30,np)K-40 and studied by means of gamma-ray spectroscopy techniques using one triple-cluster detector of the Advanced Gamma Tracking Array at the Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro. Several states with excitation energy up to 8 MeV and spin up to 10(-) have been discovered. These states are discussed in terms of J = 3 and T = 0 neutron-proton hole pairs. Shell-model calculations in a large model space have shown good agreement with the experimental data for most of the energy levels. The evolution of the structure of this nucleus is here studied as a function of excitation energy and angular momentum.Öğe Interaction position resolution simulations and in-beam measurements of the AGATA HPGe detectors(Elsevier, 2011) Soderstrom, P. -A.; Recchia, F.; Nyberg, J.; Al-Adili, A.; Ataç, A.; Aydın, S.; Bazzacco, D.; Bednarczyk, P.; Birkenbach, B.; Bortolato, D.; Boston, A. J.; Boston, H. C.; Bruyneel, B.; Bucurescu, D.; Calore, E.; Colosimo, S.; Crespi, F. C. L.; Dosme, N.; Eberth, J.; Farnea, E.; Filmer, F.; Gadea, A.; Gottardo, A.; Grave, X.; Grebosz, J.; Griffiths, R.; Gulmini, M.; Habermann, T.; Hess, H.; Jaworski, G.; Jones, P.; Joshi, P.; Judson, D. S.; Kempley, R.; Khaplanov, A.; Legay, E.; Lersch, D.; Ljungvall, J.; Lopez-Martens, A.; Meczynski, W.; Mengoni, D.; Michelagnoli, C.; Molini, P.; Napoli, D. R.; Orlandi, R.; Pascovici, G.; Pullia, A.; Reiter, P.; Sahin, E.; Smith, J. F.; Strachan, J.; Tonev, D.; Unsworth, C.; Ur, C. A.; Valiente-Dobon, J. J.; Veyssiere, C.; Wiens, A.The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected gamma-ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted gamma-ray. The gamma-ray tracking was used to determine the full energy of the gamma-rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of <1 mm in the FVVHM of the interaction position resolution for the gamma-ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a (30)5i beam at 64 MeV on a thin (12)C target. Pulse-shape analysis of the digitized detector waveforms and gamma-ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the gamma-ray energy and on the energy, axial location and type of the first interaction point, are presented. The FVVHM of the interaction position resolution varies roughly linearly as a function of gamma-ray energy from 8.5 mm at 250 key to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the gamma-ray energy range from 1.5 to 4 MeV. (C) 2011 Elsevier B.V. All rights reserved.Öğe Performance of an AGATA prototype detector estimated by Compton-imaging techniques(Elsevier, 2009) Recchia, F.; Bazzacco, D.; Farnea, E.; Venturelli, R.; Aydın, Sezgin; Suliman, G.; Ur, C. A.The imaging capabilities of an AGATA detector have been determined experimentally. Fundamental information on the detector performance can be obtained by a back-projection of the events consisting in a Compton scattering and a subsequent photoelectric absorption. The procedure presented will allow to obtain a feedback on the over-all position resolution of tracking detectors with a high energy resolution. Thanks to its simplicity the method will be used to guarantee the maximal operational performance of tracking arrays such as AGATA. (C) 2009 Elsevier B.V. All rights reserved.Öğe Spectroscopy of neutron-rich Fe isotopes populated in the 70Zn+238U reaction(Jagiellonian University, 2024) Bazzacco, D.; Lenzi, S.M.; Recchia, F.; Axiotis, M.; Aydın, S.; Benito, J.; Benzoni, G; Bizzeti, P.G.; Bizzeti-Sona, A.M.; Bracco, A.; Broda, R.; Bucurescu, D.The excited states of neutron-rich Fe isotopes have been studied through a multinucleon transfer reaction of a 70Zn beam on a 238U target. Unambiguous identification of prompt ? rays belonging to each nucleus was performed by coincidence detection of the ions in a high-acceptance magnetic spectrometer. The observed spectra are compared with large-scale shell-model calculations in the fpgd model space.
