Binary reaction decays from Mg24+C12

C. Beck, P. Papka, A. Sànchez i Zafra, S. Thummerer, F. Azaiez, P. Bednarczyk, S. Courtin, D. Curien, O. Dorvaux, D. Lebhertz, A. Nourreddine, M. Rousseau, W. von Oertzen, B. Gebauer, C. Wheldon, Tz. Kokalova, G. de Angelis, A. Gadea, S. Lenzi, S. Szilner, D. R Napoli, W. N. Catford, D. G. Jenkins, and G. Royer
Phys. Rev. C 80, 034604 – Published 8 September 2009

Abstract

Charged-particle and γ decays in Mg24* are investigated for excitation energies where quasimolecular resonances appear in C12+C12 collisions. Various theoretical predictions for the occurrence of superdeformed and hyperdeformed bands associated with resonance structures with low spin are discussed within the measured Mg24* excitation energy region. The inverse kinematics reaction Mg24+C12 is studied at Elab(Mg24)=130 MeV, an energy that enables the population of Mg24 states decaying into C12+C12 resonant breakup states. Exclusive data were collected with the Binary Reaction Spectrometer in coincidence with Euroball IV installed at the Vivitron tandem facility at Strasbourg. Specific structures with large deformation were selectively populated in binary reactions, and their associated γ decays studied. Coincident events associated with inelastic and α-transfer channels have been selected by choosing the excitation energy or the entry point via the two-body Q values. The analysis of the binary reaction channels is presented with a particular emphasis on Mg24γ, Ne20γ, and O16-γ coincidences. New information (spin and branching ratios) is deduced on high-energy states in Mg24 and O16, respectively.

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  • Received 18 May 2009

DOI:https://doi.org/10.1103/PhysRevC.80.034604

©2009 American Physical Society

Authors & Affiliations

C. Beck1,*, P. Papka1,†, A. Sànchez i Zafra1, S. Thummerer1,2, F. Azaiez1,‡, P. Bednarczyk1, S. Courtin1, D. Curien1, O. Dorvaux1, D. Lebhertz1, A. Nourreddine1, M. Rousseau1, W. von Oertzen2, B. Gebauer2, C. Wheldon2,§, Tz. Kokalova2, G. de Angelis3, A. Gadea3, S. Lenzi3, S. Szilner3,∥, D. R Napoli3, W. N. Catford4, D. G. Jenkins5, and G. Royer6

  • 1Institut Pluridisciplinaire Hubert Curien, Département de Recherches Subatomiques, UMR7178, IN2P3-CNRS and Université de Strasbourg, 23 rue du Loess, B. P. 28, F-67037 Strasbourg Cedex 2, France
  • 2Hahn-Meitner-Institut, Glienicker Str. 100, D-14109 Berlin, Germany
  • 3INFN-Lab. Nationali di Legnaro and Dipartimento di Fisica, I-35020 Padova, Italy
  • 4School of Physics and Chemistry, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom
  • 5Department of Physics, University of York, York YO10 5DD, United Kingdom
  • 6Subatech, IN2P3-CNRS> and Université-Ecole des Mines, 4 rue A. Kastler, F-44307 Nantes Cedex 3, France

  • *Corresponding author:christian.beck@ires.in2p3.fr
  • Present address: Department of Physics, University of Stellenbosch, Matieland, Stellenbosch 7602, South Africa.
  • Permanent address: IPN Orsay, Orsay, France.
  • §Present address: School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom.
  • Permanent address: Ruder Bošković Institute, HR-10001 Zagreb, Croatia.

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Issue

Vol. 80, Iss. 3 — September 2009

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