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Atom-Rydberg Atom Collisions in Hydrogen Plasmas : Cross Sections and Rate Coefficients. / Srećković, V. A.; Dimitrijević, M. S.; Ignjatović, Lj M.; Bezuglov, N. N.; Klyucharev, A. N.

в: Journal of Physics: Conference Series, Том 1289, № 1, 012022, 23.08.2019.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Srećković, VA, Dimitrijević, MS, Ignjatović, LM, Bezuglov, NN & Klyucharev, AN 2019, 'Atom-Rydberg Atom Collisions in Hydrogen Plasmas: Cross Sections and Rate Coefficients', Journal of Physics: Conference Series, Том. 1289, № 1, 012022. https://doi.org/10.1088/1742-6596/1289/1/012022

APA

Srećković, V. A., Dimitrijević, M. S., Ignjatović, L. M., Bezuglov, N. N., & Klyucharev, A. N. (2019). Atom-Rydberg Atom Collisions in Hydrogen Plasmas: Cross Sections and Rate Coefficients. Journal of Physics: Conference Series, 1289(1), [012022]. https://doi.org/10.1088/1742-6596/1289/1/012022

Vancouver

Srećković VA, Dimitrijević MS, Ignjatović LM, Bezuglov NN, Klyucharev AN. Atom-Rydberg Atom Collisions in Hydrogen Plasmas: Cross Sections and Rate Coefficients. Journal of Physics: Conference Series. 2019 Авг. 23;1289(1). 012022. https://doi.org/10.1088/1742-6596/1289/1/012022

Author

Srećković, V. A. ; Dimitrijević, M. S. ; Ignjatović, Lj M. ; Bezuglov, N. N. ; Klyucharev, A. N. / Atom-Rydberg Atom Collisions in Hydrogen Plasmas : Cross Sections and Rate Coefficients. в: Journal of Physics: Conference Series. 2019 ; Том 1289, № 1.

BibTeX

@article{f7e806c15621413482b8e9308e26f497,
title = "Atom-Rydberg Atom Collisions in Hydrogen Plasmas: Cross Sections and Rate Coefficients",
abstract = "Non-LTE modelling requires accurate atomic data e.g. collisional excitation and ionization cross-sections and rate coefficients. In order to improve the modeling of the solar photosphere, as well as to model atmospheres of other similar and cooler stars where the main constituent is also hydrogen, it is necessary to take into account the influence of all the relevant collisional processes on the excited-atom populations in weakly ionized hydrogen plasmas. In this context we present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmospheres layers. The ionization processes in collisions of excited hydrogen atoms with atoms in ground states were considered for the principal quantum numbers 2 ≤ n ≤ 20 and temperatures 4000 K ≤ T ≤ 20000 K.",
keywords = "ATOMS, Ground state, Hydrogen, Impact ionization, Quantum theory, Solar power generation, spectroscopy",
author = "Sre{\'c}kovi{\'c}, {V. A.} and Dimitrijevi{\'c}, {M. S.} and Ignjatovi{\'c}, {Lj M.} and Bezuglov, {N. N.} and Klyucharev, {A. N.}",
year = "2019",
month = aug,
day = "23",
doi = "10.1088/1742-6596/1289/1/012022",
language = "English",
volume = "1289",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",
note = "24th International Conference on Spectral Line Shapes, ICSLS 2018 ; Conference date: 17-06-2018 Through 22-06-2018",

}

RIS

TY - JOUR

T1 - Atom-Rydberg Atom Collisions in Hydrogen Plasmas

T2 - 24th International Conference on Spectral Line Shapes, ICSLS 2018

AU - Srećković, V. A.

AU - Dimitrijević, M. S.

AU - Ignjatović, Lj M.

AU - Bezuglov, N. N.

AU - Klyucharev, A. N.

PY - 2019/8/23

Y1 - 2019/8/23

N2 - Non-LTE modelling requires accurate atomic data e.g. collisional excitation and ionization cross-sections and rate coefficients. In order to improve the modeling of the solar photosphere, as well as to model atmospheres of other similar and cooler stars where the main constituent is also hydrogen, it is necessary to take into account the influence of all the relevant collisional processes on the excited-atom populations in weakly ionized hydrogen plasmas. In this context we present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmospheres layers. The ionization processes in collisions of excited hydrogen atoms with atoms in ground states were considered for the principal quantum numbers 2 ≤ n ≤ 20 and temperatures 4000 K ≤ T ≤ 20000 K.

AB - Non-LTE modelling requires accurate atomic data e.g. collisional excitation and ionization cross-sections and rate coefficients. In order to improve the modeling of the solar photosphere, as well as to model atmospheres of other similar and cooler stars where the main constituent is also hydrogen, it is necessary to take into account the influence of all the relevant collisional processes on the excited-atom populations in weakly ionized hydrogen plasmas. In this context we present the data needed for the inclusion of the specific atomic collisional processes in the investigation of the optical and kinetic properties of weakly ionized stellar atmospheres layers. The ionization processes in collisions of excited hydrogen atoms with atoms in ground states were considered for the principal quantum numbers 2 ≤ n ≤ 20 and temperatures 4000 K ≤ T ≤ 20000 K.

KW - ATOMS

KW - Ground state

KW - Hydrogen

KW - Impact ionization

KW - Quantum theory

KW - Solar power generation

KW - spectroscopy

UR - http://www.scopus.com/inward/record.url?scp=85073531603&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1289/1/012022

DO - 10.1088/1742-6596/1289/1/012022

M3 - Conference article

AN - SCOPUS:85073531603

VL - 1289

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012022

Y2 - 17 June 2018 through 22 June 2018

ER -

ID: 47804855