Standard

Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band. / Devdariani, A. Z.; Zagrebin, A. L.; Kryukov, N. A. ; Lednev, M. G.; Timofeev, N. A. .

в: OPTICS AND SPECTROSCOPY, Том 126, № 5, 01.05.2019, стр. 455-457.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Devdariani, AZ, Zagrebin, AL, Kryukov, NA, Lednev, MG & Timofeev, NA 2019, 'Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band', OPTICS AND SPECTROSCOPY, Том. 126, № 5, стр. 455-457. https://doi.org/10.1134/S0030400X19050060

APA

Devdariani, A. Z., Zagrebin, A. L., Kryukov, N. A., Lednev, M. G., & Timofeev, N. A. (2019). Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band. OPTICS AND SPECTROSCOPY, 126(5), 455-457. https://doi.org/10.1134/S0030400X19050060

Vancouver

Devdariani AZ, Zagrebin AL, Kryukov NA, Lednev MG, Timofeev NA. Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band. OPTICS AND SPECTROSCOPY. 2019 Май 1;126(5):455-457. https://doi.org/10.1134/S0030400X19050060

Author

Devdariani, A. Z. ; Zagrebin, A. L. ; Kryukov, N. A. ; Lednev, M. G. ; Timofeev, N. A. . / Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band. в: OPTICS AND SPECTROSCOPY. 2019 ; Том 126, № 5. стр. 455-457.

BibTeX

@article{5ad1e8c11a864a5ea64a4533a3eef5bb,
title = "Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band",
abstract = "The reasons for the discrepancies between the experimental data on the shape of long-wavelength continua near the 6(3)P(1) 6(1)S(0) resonance line of a mercury atom in a xenon atmosphere obtained by different authors are analyzed. Calculations of spectral profiles for limiting cases of high and low densities of buffer gas atoms lead to the conclusion that the discrepancies are mainly due to the dependence of the rates of three-particle recombination and relaxation processes on the xenon density. Different types of a non-equilibrium or almost equilibrium (at high xenon concentrations) population of rovibrational states of a HgXe(A(3)0(+)) excimer molecule are formed at different rates of these processes, which affects emission spectral profiles.",
keywords = "INTERATOMIC POTENTIALS, DISCHARGE, EMISSION",
author = "Devdariani, {A. Z.} and Zagrebin, {A. L.} and Kryukov, {N. A.} and Lednev, {M. G.} and Timofeev, {N. A.}",
year = "2019",
month = may,
day = "1",
doi = "10.1134/S0030400X19050060",
language = "Английский",
volume = "126",
pages = "455--457",
journal = "OPTICS AND SPECTROSCOPY",
issn = "0030-400X",
publisher = "Pleiades Publishing",
number = "5",

}

RIS

TY - JOUR

T1 - Influence of the Density of Buffer Gas Atoms on the Shape of the HgXe(A(3)0(+)) HgXe(X(1)0(+)) Excimer Band

AU - Devdariani, A. Z.

AU - Zagrebin, A. L.

AU - Kryukov, N. A.

AU - Lednev, M. G.

AU - Timofeev, N. A.

PY - 2019/5/1

Y1 - 2019/5/1

N2 - The reasons for the discrepancies between the experimental data on the shape of long-wavelength continua near the 6(3)P(1) 6(1)S(0) resonance line of a mercury atom in a xenon atmosphere obtained by different authors are analyzed. Calculations of spectral profiles for limiting cases of high and low densities of buffer gas atoms lead to the conclusion that the discrepancies are mainly due to the dependence of the rates of three-particle recombination and relaxation processes on the xenon density. Different types of a non-equilibrium or almost equilibrium (at high xenon concentrations) population of rovibrational states of a HgXe(A(3)0(+)) excimer molecule are formed at different rates of these processes, which affects emission spectral profiles.

AB - The reasons for the discrepancies between the experimental data on the shape of long-wavelength continua near the 6(3)P(1) 6(1)S(0) resonance line of a mercury atom in a xenon atmosphere obtained by different authors are analyzed. Calculations of spectral profiles for limiting cases of high and low densities of buffer gas atoms lead to the conclusion that the discrepancies are mainly due to the dependence of the rates of three-particle recombination and relaxation processes on the xenon density. Different types of a non-equilibrium or almost equilibrium (at high xenon concentrations) population of rovibrational states of a HgXe(A(3)0(+)) excimer molecule are formed at different rates of these processes, which affects emission spectral profiles.

KW - INTERATOMIC POTENTIALS

KW - DISCHARGE

KW - EMISSION

UR - http://www.scopus.com/inward/record.url?scp=85067980441&partnerID=8YFLogxK

UR - http://www.mendeley.com/research/influence-density-buffer-gas-atoms-shape-hgxea-30-hgxex-10-excimer-band

U2 - 10.1134/S0030400X19050060

DO - 10.1134/S0030400X19050060

M3 - статья

VL - 126

SP - 455

EP - 457

JO - OPTICS AND SPECTROSCOPY

JF - OPTICS AND SPECTROSCOPY

SN - 0030-400X

IS - 5

ER -

ID: 43511736