Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons
In recent work, the effect of a magnetic field on the line shapes via the modification of electron perturber trajectories was considered. In the present paper we revisit this idea using a variation of the Collision-time Statistics method, in order to account for <inline-formula> <math displ...
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MDPI AG
2019-05-01
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Online Access: | https://www.mdpi.com/2218-2004/7/2/52 |
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author | Spiros Alexiou |
author_facet | Spiros Alexiou |
author_sort | Spiros Alexiou |
collection | DOAJ |
description | In recent work, the effect of a magnetic field on the line shapes via the modification of electron perturber trajectories was considered. In the present paper we revisit this idea using a variation of the Collision-time Statistics method, in order to account for <inline-formula> <math display="inline"> <semantics> <mrow> <mi>a</mi> <mi>l</mi> <mi>l</mi> </mrow> </semantics> </math> </inline-formula> relevant perturbers. We also obtain line profiles for the hydrogen <inline-formula> <math display="inline"> <semantics> <msub> <mi>L</mi> <mi>α</mi> </msub> </semantics> </math> </inline-formula> line for conditions of astrophysical interest. Although the Collision-time statistics method works for both electrons and ions, we apply a simplification here that results in an excessive number of ions having to be simulated. As a result, the present, simplified version, is typically only appropriate for electrons. |
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institution | Directory Open Access Journal |
issn | 2218-2004 |
language | English |
last_indexed | 2024-12-11T12:17:43Z |
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spelling | doaj.art-0cffcaea515840c1b483d26cc16373ee2022-12-22T01:07:36ZengMDPI AGAtoms2218-20042019-05-01725210.3390/atoms7020052atoms7020052Line Shapes in a Magnetic Field: Trajectory Modifications I: ElectronsSpiros Alexiou0Hellenic Army Academy, Varis—Koropiou Avenue Vari P.O. Box 16673, GreeceIn recent work, the effect of a magnetic field on the line shapes via the modification of electron perturber trajectories was considered. In the present paper we revisit this idea using a variation of the Collision-time Statistics method, in order to account for <inline-formula> <math display="inline"> <semantics> <mrow> <mi>a</mi> <mi>l</mi> <mi>l</mi> </mrow> </semantics> </math> </inline-formula> relevant perturbers. We also obtain line profiles for the hydrogen <inline-formula> <math display="inline"> <semantics> <msub> <mi>L</mi> <mi>α</mi> </msub> </semantics> </math> </inline-formula> line for conditions of astrophysical interest. Although the Collision-time statistics method works for both electrons and ions, we apply a simplification here that results in an excessive number of ions having to be simulated. As a result, the present, simplified version, is typically only appropriate for electrons.https://www.mdpi.com/2218-2004/7/2/52stark broadeningmagnetic fieldspiralling trajectoriescollision-time statistics |
spellingShingle | Spiros Alexiou Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons Atoms stark broadening magnetic field spiralling trajectories collision-time statistics |
title | Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_full | Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_fullStr | Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_full_unstemmed | Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_short | Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_sort | line shapes in a magnetic field trajectory modifications i electrons |
topic | stark broadening magnetic field spiralling trajectories collision-time statistics |
url | https://www.mdpi.com/2218-2004/7/2/52 |
work_keys_str_mv | AT spirosalexiou lineshapesinamagneticfieldtrajectorymodificationsielectrons |