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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doaj-0cffcaea515840c1b483d26cc16373ee2020-11-25T02:10:47ZengMDPI 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 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Spiros Alexiou |
spellingShingle |
Spiros Alexiou Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons Atoms stark broadening magnetic field spiralling trajectories collision-time statistics |
author_facet |
Spiros Alexiou |
author_sort |
Spiros Alexiou |
title |
Line Shapes in a Magnetic Field: Trajectory Modifications I: Electrons |
title_short |
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_sort |
line shapes in a magnetic field: trajectory modifications i: electrons |
publisher |
MDPI AG |
series |
Atoms |
issn |
2218-2004 |
publishDate |
2019-05-01 |
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. |
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 |
_version_ |
1724917437640474624 |