Low-temperature matrix effects on orientational motion of Methyl radical trapped in gas solids: Angular tunneling vs. libration

EPR investigation of the lineshape of matrix -isolated methyl radical, CH3, spectra recorded in solid N2O and CO2 was carried out. Reversible temperature-dependent line width anisotropy was observed in both matrices. This effect is a fingerprint of the extra-slow radical rotation about the in-plane...

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Veröffentlicht in:Physica. B, Condensed matter Condensed matter, 2018-05, Vol.537, p.51-57
Hauptverfasser: Dmitriev, Yurij A., Zelenetckii, Ilia A., Benetis, Nikolas P.
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Sprache:eng
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Zusammenfassung:EPR investigation of the lineshape of matrix -isolated methyl radical, CH3, spectra recorded in solid N2O and CO2 was carried out. Reversible temperature-dependent line width anisotropy was observed in both matrices. This effect is a fingerprint of the extra-slow radical rotation about the in-plane C2 axes. The rotation was found to be anisotropic and closely correlated to the orientational dynamics of the matrix molecules. It was suggested that a recently discovered “hoping precession” effect of matrix molecules in solid CO2 is a common feature of matrices of the linear molecules CO, N2O, and CO2. A new low-temperature matrix effect, referred to as “libration trap”, was proposed which accounts for the changing CH3 reorientational motion about the radical C3-axis from rotation to libration. Temperature dependence of the intensity of the EPR satellites produced by these nonrotating—but librating methyls was presented. This allowed for a rough estimation of the rotation hindering potential due to correlation mismatch between the radical and the nearest matrix molecules' librations. •Methyl radical rotation in matrices of solid N2O and CO2 studied by EPR.•Motion of matrix isolated methyl correlates with matrix molecular motion.•Theory shows wide angle torsional oscillations of matrix isolated methyl.•Anisotropic tunneling rotation and excited libration of methyl in solid gases.
ISSN:0921-4526
1873-2135
DOI:10.1016/j.physb.2018.01.045