Bereiche | Tage | Auswahl | Suche | Aktualisierungen | Downloads | Hilfe
HK: Fachverband Physik der Hadronen und Kerne
HK 35: Instrumentation
HK 35.1: Gruppenbericht
Mittwoch, 21. März 2012, 16:30–17:00, P 3
PRESPEC-AGATA: New prespectives for γ-spectroscopy. — F. Ameil1, •P. Boutachkov2, M.L. Cortes2, J. Gerl1, A. Givechev2, N. Goel1, M. Gorska1, E. Gregor2, G. Guastalla2, T. Habermann3, I. Kojouharov1, V. Lushta2, E. Merchan1,2, T. Moeller2, P.T. Patchakui2, N. Pietralla2, S. Pietri1, D. Ralet2, M. Reese2, H. Schaffner1, P.P. Singh2, B. Szczepanczyk2, H.J. Wollersheim1, A. Gadea4, and W. Korten5 — 1GSI — 2IKP, TU Darmstadt — 3Uni. of Frankfurt — 4Uni. of Valencia, Spain — 5CEA Saclay, France
The PRESPEC-AGATA setup is a unique combination of the GSI accelerator facility, the Fragment Separator(FRS), the Advanced Gamma Tracking Array(AGATA), the HECTOR array and the LYCCA-0 Calorimeter. With this setup high-resolution in-flight spectroscopy of relativistic(β∼0.4-0.5) exotic nuclei will be performed. A thick target positioned at the final focal plane of the FRS will be used for Coulomb excitation or fragmentation of the exotic ions separated with the FRS. The γ-rays emitted in these reactions will be detected by the AGATA and HECTOR arrays. The fragments produced at the secondary target will be identified and tracked by LYCCA-0. Compared to the RISING array, the improved energy resolution and efficency of the AGATA array is expected to lead to a gain in sensitivity of a factor of 10 and 100 for γ-particles and γ-γ-particle coincidences, respectively. The perspectives of the new setup will be discussed. Supported by the BMBF under 06DA9040I, by HICforFAIR, and by the HGF under VH-VI-417.