Abstract

In a search for high spin molecular states in $^{36}\mathrm{Ar}$, the $^{20}\mathrm{Ne}$${+}^{16}$O system was studied using a differentially pumped windowless $^{20}\mathrm{Ne}$ gas target. Angle-averaged excitation functions for the $^{20}\mathrm{Ne}$${+}^{16}$O and $^{24}\mathrm{Mg}$${+}^{12}$C mass partitions were obtained for the energy range 16.39 MeV \ensuremath{\le}${\mathit{E}}_{\mathrm{c}.\mathrm{m}.}$\ensuremath{\le} 41.67 MeV in 278 keV steps. Inelastic scattering involving the $^{16}\mathrm{O}$(${0}_{2}^{+}$, 6.05 MeV) state was separated from the nearby $^{16}\mathrm{O}$(${3}_{1}^{\mathrm{\ensuremath{-}}}$, 6.13 MeV) state by detecting the ${\mathit{e}}^{\mathrm{\ensuremath{-}}}$ and ${\mathit{e}}^{+}$ emitted from the internal pair decay of the $^{16}\mathrm{O}$(${0}_{2}^{+}$) state. A statistical fluctuation analysis indicates that several correlated structures are present in the current system. Tentative spin assignments based on angular distribution measurements suggest the resonant structures could be associated with rotational states of $^{36}\mathrm{Ar}$. The results are compared with a cranked cluster model calculation. \textcopyright{} 1996 The American Physical Society.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.