Structure of Ti-55 from relativistic one-neutron knockout

Autor: I. Kojouharov, C. Pascual-Izarra, T. Le Bleis, R. Krücken, D. Cortina-Gil, Björn Jonson, L. Maier, A. Burger, Joachim Enders, A. Prochazka, P. G. Hansen, P. Maierbeck, W. D. M. Rae, K. Sümmerer, A. Chatillon, Enrique Casarejos, Branislav Sitar, F. Aksouh, Olof Tengblad, S. Winkler, J. Gerl, N. Kurz, Ángel Perea, M. Caamaño, T. Kröll, L. V. Chulkov, V. Bildstein, J. A. Tostevin, M. Stanoiu, C. Nociforo, O. Kiselev, M. Gascon, B. Alex Brown, Takaharu Otsuka, T. Kurtukian, Roman Gernhäuser, T. Faestermann, A. Klimkiewicz, M. Böhmer, S. Schwertel, D. M. Rossi, H. Schaffner, Thomas Aumann, Herbert A. Simon, Rituparna Kanungo, J. Benlliure, J. Friese, Gunnar Nyman, A. Brünle, Laura Fabbietti, M. J. G. Borge, C. Rodriguez-Tajes, G. Schrieder, K. Boretzky, Kristian Larsson, Hans Geissel, E. A. Benjamim, K. Mahata, Dolores Pérez, Helmut Weick, M. Górska, H. Alvarez-Pol, K. Eppinger, K.-H. Behr, Thomas Nilsson
Jazyk: angličtina
Rok vydání: 2009
Předmět:
Zdroj: Digital.CSIC. Repositorio Institucional del CSIC
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Popis: 6 pages, 4 figures.-- PACS nrs.: 21.60.Cs; 23.20.Lv; 24.50.+g; 25.60.Gc; 27.40.+z.-- Printed version published May 4, 2009.-- ArXiv pre-print available at: http://arxiv.org/abs/0810.3157
Results are presented from a one-neutron knockout reaction at relativistic energies on Ti-56 using the GSI FRS as a two-stage magnetic spectrometer and the Miniball array for gamma-ray detection. Inclusive and exclusive longitudinal momentum distributions and cross-sections were measured enabling the determination of the orbital angular momentum of the populated states. First-time observation of the 955(6) keV vp(3/2)(-1)-hole state in Ti-55 is reported. The measured data for the first time proves that the ground state of Ti-55 is a 1/2(−) state, in agreement with shell-model calculations using the GXPF1A interaction that predict a sizable N=34 gap in Ca-54.
This work was supported by the BMBF under contract 06MT238, by the DFG cluster of excellence "Origin and Structure of the Universe"(http://www.universe-cluster.de) and by the European Commission within the Sixth Framework Programme through I3-EURONS (contract No. RII3-CT-2004-506065). J. Tostevin acknowledges support from the United Kingdom Science and Technology Facilities Council (STFC) under Grant No. EP/D003628. T. Nilsson acknowledges the support of the Knut and Alice Wallenberg Foundation, Sweden. R. Kanungo gratefully acknowledges the support of the AvH foundation. B.A. Brown acknowledges support from NSF grant PHY-0758099.
Databáze: OpenAIRE