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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Main Author: Spiros Alexiou
Format: Article
Language:English
Published: MDPI AG 2019-05-01
Series:Atoms
Subjects:
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>&#945;</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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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>&#945;</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