Vanishing spin alignment: Experimental indication of a triaxial<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>28</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Si</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>+</mml:mo></mml:mrow><mml:mrow><mml:mn>28</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Si</mml:mi></mml:math>nuclear molecule
R. NouicerInstitut National de Physique Nucléaire et de Physique des ParticulesChristian BeckUniversité de StrasbourgR. M. FreemanUniversité de StrasbourgF. HaasIReS, UMR7500, CNRS-IN2P3 et Université Louis Pasteur, F-67037 Strasbourg, Cedex 2, FranceNadia AissaouiUniversité de StrasbourgT. BellotInstitut National de Physique Nucléaire et de Physique des ParticulesG. de FranceIReS, UMR7500, CNRS-IN2P3 et Université Louis Pasteur, F-67037 Strasbourg, Cedex 2, FranceD. DisdierInstitut National de Physique Nucléaire et de Physique des ParticulesG. DuchêneInstitut National de Physique Nucléaire et de Physique des ParticulesA. ElaniqueIReS, UMR7500, CNRS-IN2P3 et Université Louis Pasteur, F-67037 Strasbourg, Cedex 2, FranceA. HachemInstitut National de Physique Nucléaire et de Physique des ParticulesF. HoellingerIReS, UMR7500, CNRS-IN2P3 et Université Louis Pasteur, F-67037 Strasbourg, Cedex 2, FranceD. MahboubUniversité de StrasbourgV. RauchUniversité de StrasbourgS. SandersDepartment of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045A. DummerDepartment of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045F. W. ProsserDepartment of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045A. Szanto de ToledoInstituto de Fisica da Universidade de São Paulo, São Paulo, BrazilS. CavallaroE. UegakiDepartment of Physics, Akita University, Akita 010, JapanYasuhisa AbeYukawa Institute for Theoretical Physics, Kyoto University, Kyoto, Japan
1999lv
ABI
Annotatsiya
Fragment-fragment-$\ensuremath{\gamma}$ coincidences have been measured for ${}^{28}\mathrm{Si}{+}^{28}\mathrm{Si}$ at an energy corresponding to the population of a conjectured resonance in ${}^{56}\mathrm{Ni}.$ Fragment angular distributions as well as $\ensuremath{\gamma}$-ray angular correlations indicate that the spin orientations of the outgoing fragments are perpendicular to the orbital angular momentum. This differs from the ${}^{24}\mathrm{Mg}{+}^{24}\mathrm{Mg}$ and the ${}^{12}\mathrm{C}{+}^{12}\mathrm{C}$ resonances, and suggests two oblate ${}^{28}\mathrm{Si}$ nuclei interacting in an equator-to-equator molecular configuration.
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