IIA Institutional Repository

Full non-LTE multi-level radiative transfer: I. An atom with three bound infinitely sharp levels

Show simple item record

dc.contributor.author Lagache, T
dc.contributor.author Paletou, F
dc.contributor.author Sampoorna, M
dc.date.accessioned 2025-08-05T06:35:42Z
dc.date.available 2025-08-05T06:35:42Z
dc.date.issued 2025-07
dc.identifier.citation Astronomy & Astrophysics, Vol. 699, A198 en_US
dc.identifier.issn 0004-6361
dc.identifier.uri http://hdl.handle.net/2248/8775
dc.description Open Access en_US
dc.description Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstract Context. The standard nonlocal thermodynamic equilibrium (non-LTE) multi-level radiative transfer problem only takes into account the deviation of the radiation field and atomic populations from their equilibrium distribution. Aims. We aim to show how to solve for the full non-LTE (FNLTE) multi-level radiative transfer problem, also accounting for deviation of the velocity distribution of the massive particles from Maxwellian. We considered, as a first step, a three-level atom with zero natural broadening. Methods. In this work, we present a new numerical scheme. Its initialisation relies on the classic, multi-level approximate Λ-iteration (MALI) method for the standard non-LTE problem. The radiative transfer equations, the kinetic equilibrium equations for atomic populations, and the Boltzmann equations for the velocity distribution functions were simultaneously iterated in order to obtain self-consistent particle distributions. During the process, the observer’s frame absorption and emission profiles were re-computed at every iterative step by convolving the atomic frame quantities with the relevant velocity distribution function. Results. We validate our numerical strategy by comparing our results with the standard non-LTE solutions in the limit of a two-level atom with Hummer’s partial redistribution in frequency, and with a three-level atom with complete redistribution. In this work, we considered the so-called cross-redistribution problem. We then show new FNLTE results for a simple three-level atom while evaluating the assumptions made for the emission and absorption profiles of the standard non-LTE problem with partial and cross-redistribution. en_US
dc.language.iso en en_US
dc.publisher EDP Sciences en_US
dc.relation.uri https://doi.org/10.1051/0004-6361/202555008
dc.rights © The Authors 2025
dc.subject Line: formation en_US
dc.subject Line: profiles en_US
dc.subject Radiative transfer en_US
dc.subject Stars: atmospheres en_US
dc.title Full non-LTE multi-level radiative transfer: I. An atom with three bound infinitely sharp levels en_US
dc.type Article en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Browse

My Account