Standard

Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules. / Bichutskaya, E. N.; Devdariani, A. Z.; Zagrebin, A. L.; Sebyakin, Yu N.

в: Optics and Spectroscopy (English translation of Optika i Spektroskopiya), Том 87, № 2, 01.08.1999, стр. 197-202.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Bichutskaya, EN, Devdariani, AZ, Zagrebin, AL & Sebyakin, YN 1999, 'Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules', Optics and Spectroscopy (English translation of Optika i Spektroskopiya), Том. 87, № 2, стр. 197-202.

APA

Bichutskaya, E. N., Devdariani, A. Z., Zagrebin, A. L., & Sebyakin, Y. N. (1999). Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules. Optics and Spectroscopy (English translation of Optika i Spektroskopiya), 87(2), 197-202.

Vancouver

Bichutskaya EN, Devdariani AZ, Zagrebin AL, Sebyakin YN. Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules. Optics and Spectroscopy (English translation of Optika i Spektroskopiya). 1999 Авг. 1;87(2):197-202.

Author

Bichutskaya, E. N. ; Devdariani, A. Z. ; Zagrebin, A. L. ; Sebyakin, Yu N. / Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules. в: Optics and Spectroscopy (English translation of Optika i Spektroskopiya). 1999 ; Том 87, № 2. стр. 197-202.

BibTeX

@article{f38faac1034c4492ba9410e793f4281b,
title = "Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules",
abstract = "Calculations are reported for collisionally induced emission spectra of Ca(4s4p 3P1, 3P2) and Mg(3s3p 3P1, 3P2) - He(1s2 1S0) quasi-molecules. The calculations were made in the quasi-static approximation and on the basis of the Demkov model. The shape of a spectral line depends on the parameter of nonadiabaticity and the fact whether an initial populated state was of the radiative or the forbidden type. The dynamic approach supported the formation of a satellite shifted from the position of the forbidden atomic transition to the blue wing in the case where the energy of the radiative atomic transition is lower than the energy of the forbidden transition.",
keywords = "NE INTERACTION, COLLISIONS, ATOMS, POTENTIALS, STATES, SPIN, HE",
author = "Bichutskaya, {E. N.} and Devdariani, {A. Z.} and Zagrebin, {A. L.} and Sebyakin, {Yu N.}",
year = "1999",
month = aug,
day = "1",
language = "English",
volume = "87",
pages = "197--202",
journal = "OPTICS AND SPECTROSCOPY",
issn = "0030-400X",
publisher = "Pleiades Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - Quasi-Molecular Emission and Nonadiabatic Transitions. I. Ca(4s4p3P1, 3P2) and Mg(3s3p3P1, 3P2)-He(1s21S0) Quasi-Molecules

AU - Bichutskaya, E. N.

AU - Devdariani, A. Z.

AU - Zagrebin, A. L.

AU - Sebyakin, Yu N.

PY - 1999/8/1

Y1 - 1999/8/1

N2 - Calculations are reported for collisionally induced emission spectra of Ca(4s4p 3P1, 3P2) and Mg(3s3p 3P1, 3P2) - He(1s2 1S0) quasi-molecules. The calculations were made in the quasi-static approximation and on the basis of the Demkov model. The shape of a spectral line depends on the parameter of nonadiabaticity and the fact whether an initial populated state was of the radiative or the forbidden type. The dynamic approach supported the formation of a satellite shifted from the position of the forbidden atomic transition to the blue wing in the case where the energy of the radiative atomic transition is lower than the energy of the forbidden transition.

AB - Calculations are reported for collisionally induced emission spectra of Ca(4s4p 3P1, 3P2) and Mg(3s3p 3P1, 3P2) - He(1s2 1S0) quasi-molecules. The calculations were made in the quasi-static approximation and on the basis of the Demkov model. The shape of a spectral line depends on the parameter of nonadiabaticity and the fact whether an initial populated state was of the radiative or the forbidden type. The dynamic approach supported the formation of a satellite shifted from the position of the forbidden atomic transition to the blue wing in the case where the energy of the radiative atomic transition is lower than the energy of the forbidden transition.

KW - NE INTERACTION

KW - COLLISIONS

KW - ATOMS

KW - POTENTIALS

KW - STATES

KW - SPIN

KW - HE

UR - http://www.scopus.com/inward/record.url?scp=0004550765&partnerID=8YFLogxK

M3 - Article

VL - 87

SP - 197

EP - 202

JO - OPTICS AND SPECTROSCOPY

JF - OPTICS AND SPECTROSCOPY

SN - 0030-400X

IS - 2

ER -

ID: 5239975