Nonmonotonic distribution of population of the a3Σu+ triplet state rotational levels in corona discharge in cryogenic helium gas


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We observed the spectra within the wavelength range of 910–990 nm of emission of the corona discharge in supercritical helium gas at 6–11 K. This spectral range contains the molecular bands of the He*2 excimer radiative transitions (c3Σg+a3Σu+) between the electron-vibrational-rotational levels of the c3Σg+ and the a3Σu+ triplet states. We have determined the populations of the rotational levels (quantity of molecules in the given excited state among the excited molecules of the discharge) of the c3Σg+ excited state from experimental values of the intensity of the respective electron-vibrational-rotational lines. The calculated population distribution is nonmonotonous. The population of the level with the rotation quantum number K′ = 18 (the level number) is higher than those of the levels with the other K′ values.

作者简介

N. Bonifaci

Laboratoire G2Elab CNRS & Grenoble University

Email: atrazhev@yandex.ru
法国, Grenoble

V. Atrazhev

Joint Institute for High Temperatures

编辑信件的主要联系方式.
Email: atrazhev@yandex.ru
俄罗斯联邦, Moscow, 127412

V. Shakhatov

Topchiev Institute of Petrochemical Synthesis

Email: atrazhev@yandex.ru
俄罗斯联邦, Moscow, 119991

R. Boltnev

Joint Institute for High Temperatures; Institute of Problems of Chemical Physics

Email: atrazhev@yandex.ru
俄罗斯联邦, Moscow, 127412; Chernogolovka, Moscow region, 142432

K. von Haeften

Department of Physics and Astronomy

Email: atrazhev@yandex.ru
英国, Leicester

J. Eloranta

Department of Chemistry and Biochemistry

Email: atrazhev@yandex.ru
美国, Northridge

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