Full non-LTE spectral line formation

In the present paper we consider the full nonlocal thermodynamic equilibrium (non-LTE) radiation transfer problem. This formalism allows us to account for deviation from equilibrium distribution of both the radiation field and the massive particles. In the present study, two-level atoms with broadened upper level represent the massive particles. In the absence of velocity-changing collisions, we demonstrate the analytic equivalence of the full non-LTE source function with the corresponding standard non-LTE partial frequency redistribution (PFR) model. We present an iterative method based on operator splitting techniques that can be used to numerically solve the problem at hand. We benchmark it against the standard non-LTE transfer problem for a two-level atom with PFR. We illustrate the deviation of the velocity distribution function of excited atoms from the equilibrium distribution. We also discuss the dependence of the emission profile and the velocity distribution function on elastic collisions and velocity-changing collisions.

Authors

Institutions

Publication Details

Journal
Astronomy and Astrophysics
Published
2024-08-29
DOI
https://doi.org/10.1051/0004-6361/202449722
Citations
3
Primary Topic
Quantum optics and atomic interactions
Type
article
Field-Weighted Citation Impact
1.01

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Full non-LTE spectral line formation

M. Sampoorna, Thibault Lagache, V. Bommier, F. Paletou
3 citations
Astronomy and Astrophysics
Quantum optics and atomic interactions
1.01
article

Full non-LTE spectral line formation

M. Sampoorna, Thibault Lagache, V. Bommier, F. Paletou
article en
3 citations

Abstract

In the present paper we consider the full nonlocal thermodynamic equilibrium (non-LTE) radiation transfer problem. This formalism allows us to account for deviation from equilibrium distribution of both the radiation field and the massive particles. In the present study, two-level atoms with broadened upper level represent the massive particles. In the absence of velocity-changing collisions, we demonstrate the analytic equivalence of the full non-LTE source function with the corresponding standard non-LTE partial frequency redistribution (PFR) model. We present an iterative method based on operator splitting techniques that can be used to numerically solve the problem at hand. We benchmark it against the standard non-LTE transfer problem for a two-level atom with PFR. We illustrate the deviation of the velocity distribution function of excited atoms from the equilibrium distribution. We also discuss the dependence of the emission profile and the velocity distribution function on elastic collisions and velocity-changing collisions.

Astronomy and AstrophysicsVol. 690
Université Toulouse III - Paul Sabatier (FR), Indian Institute of Astrophysics (IN), Laboratoire d’études spatiales et d’instrumentation en astrophysique (FR), Observatoire Midi-Pyrénées (FR), Institut de Recherche en Astrophysique et Planétologie (FR)
Science and Engineering Research Board
Openalex Percentile: Top 25%
Quantum optics and atomic interactions
1.01
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.