Non-radiative inelastic processes in lithium-helium ion-atom collisions
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10286220" target="_blank" >RIV/00216208:11320/14:10286220 - isvavai.cz</a>
Výsledek na webu
<a href="http://dx.doi.org/10.1051/0004-6361/201423578" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201423578</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201423578" target="_blank" >10.1051/0004-6361/201423578</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Non-radiative inelastic processes in lithium-helium ion-atom collisions
Popis výsledku v původním jazyce
Aims. The aims are to estimate efficiencies of non-radiative inelastic processes in lithium-helium ion-atom collisions and to compare them to those for radiative processes. Methods. Non-radiative inelastic cross-sections and rate coefficients for different lithium-helium ion-atom collisions are estimated by means of the recently proposed branching probability current method, which is based on the accurate ab initio adiabatic Born-Oppenheimer potentials that have been recently calculated for the low-lying (1,3)Sigma(+) and (1,3)Pi states of the LiHe+ ion. Results. It is shown that at low temperatures the radiative depopulation in Li+ + He and Li + He+ collisions dominates over the non-radiative processes, while in Li+ + He(2s S-3) collisions the non-radiative processes dominate over the radiative association at temperatures above 3000 K, which can be expected to have some influence on depopulations of metastable He in high temperature astrophysical environments.
Název v anglickém jazyce
Non-radiative inelastic processes in lithium-helium ion-atom collisions
Popis výsledku anglicky
Aims. The aims are to estimate efficiencies of non-radiative inelastic processes in lithium-helium ion-atom collisions and to compare them to those for radiative processes. Methods. Non-radiative inelastic cross-sections and rate coefficients for different lithium-helium ion-atom collisions are estimated by means of the recently proposed branching probability current method, which is based on the accurate ab initio adiabatic Born-Oppenheimer potentials that have been recently calculated for the low-lying (1,3)Sigma(+) and (1,3)Pi states of the LiHe+ ion. Results. It is shown that at low temperatures the radiative depopulation in Li+ + He and Li + He+ collisions dominates over the non-radiative processes, while in Li+ + He(2s S-3) collisions the non-radiative processes dominate over the radiative association at temperatures above 3000 K, which can be expected to have some influence on depopulations of metastable He in high temperature astrophysical environments.
Klasifikace
Druh
J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)
CEP obor
BN - Astronomie a nebeská mechanika, astrofyzika
OECD FORD obor
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Návaznosti výsledku
Projekt
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Návaznosti
S - Specificky vyzkum na vysokych skolach
Ostatní
Rok uplatnění
2014
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Svazek periodika
565
Číslo periodika v rámci svazku
May 2014
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
5
Strana od-do
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Kód UT WoS článku
000336730900106
EID výsledku v databázi Scopus
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