Rayleigh scattering in dense fluid helium

Autores
Rohrmann, Rene Daniel
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Iglesias et al. showed that the Rayleigh scattering from helium atoms decreases by collective effects in the atmospheres of cool white dwarf stars. Their study is here extended to consider an accurate evaluation of the atomic polarizability and the density effects involved in the Rayleigh cross-section over a wide density-temperature region. The dynamic dipole polarizability of helium atoms in the ground state is determinated with the oscillator-strength distribution approach. The spectral density of oscillator strength considered includes most significant single and doubly excited transitions to discrete and continuum energies. Static and dynamic polarizability results are confronted with experiments and other theoretical evaluations shown a very good agreement. In addition, the refractive index of helium is evaluated with the Lorentz- Lorenz equation and shows a satisfactory agreement with the most recent experiments. The effect of spatial correlation of atoms on the Rayleigh scattering is calculated with Monte Carlo simulations and effective energy potentials that represent the particle interactions, covering fluid densities between 0.005 and a few g cm-3 and temperatures between 1 000 and 15 000 K. We provide analytical fits from which the Rayleigh cross-section of fluid helium can be easily calculated at wavelength λ > 505.35 Å. Collision-induced light scattering was estimated to be the dominant scattering process at densities greater than 1-2 g cm-3 depending on the temperature.
Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Materia
ATOMIC PROCESSES
OPACITY
SCATTERING
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/63141

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network_name_str CONICET Digital (CONICET)
spelling Rayleigh scattering in dense fluid heliumRohrmann, Rene DanielATOMIC PROCESSESOPACITYSCATTERINGhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Iglesias et al. showed that the Rayleigh scattering from helium atoms decreases by collective effects in the atmospheres of cool white dwarf stars. Their study is here extended to consider an accurate evaluation of the atomic polarizability and the density effects involved in the Rayleigh cross-section over a wide density-temperature region. The dynamic dipole polarizability of helium atoms in the ground state is determinated with the oscillator-strength distribution approach. The spectral density of oscillator strength considered includes most significant single and doubly excited transitions to discrete and continuum energies. Static and dynamic polarizability results are confronted with experiments and other theoretical evaluations shown a very good agreement. In addition, the refractive index of helium is evaluated with the Lorentz- Lorenz equation and shows a satisfactory agreement with the most recent experiments. The effect of spatial correlation of atoms on the Rayleigh scattering is calculated with Monte Carlo simulations and effective energy potentials that represent the particle interactions, covering fluid densities between 0.005 and a few g cm-3 and temperatures between 1 000 and 15 000 K. We provide analytical fits from which the Rayleigh cross-section of fluid helium can be easily calculated at wavelength λ > 505.35 Å. Collision-induced light scattering was estimated to be the dominant scattering process at densities greater than 1-2 g cm-3 depending on the temperature.Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaOxford University Press2018-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/63141Rohrmann, Rene Daniel; Rayleigh scattering in dense fluid helium; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 473; 1; 1-2018; 457-4690035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2440info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/473/1/457/4222615info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1709.07076info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-29T12:17:48Zoai:ri.conicet.gov.ar:11336/63141instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-29 12:17:48.35CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Rayleigh scattering in dense fluid helium
title Rayleigh scattering in dense fluid helium
spellingShingle Rayleigh scattering in dense fluid helium
Rohrmann, Rene Daniel
ATOMIC PROCESSES
OPACITY
SCATTERING
title_short Rayleigh scattering in dense fluid helium
title_full Rayleigh scattering in dense fluid helium
title_fullStr Rayleigh scattering in dense fluid helium
title_full_unstemmed Rayleigh scattering in dense fluid helium
title_sort Rayleigh scattering in dense fluid helium
dc.creator.none.fl_str_mv Rohrmann, Rene Daniel
author Rohrmann, Rene Daniel
author_facet Rohrmann, Rene Daniel
author_role author
dc.subject.none.fl_str_mv ATOMIC PROCESSES
OPACITY
SCATTERING
topic ATOMIC PROCESSES
OPACITY
SCATTERING
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Iglesias et al. showed that the Rayleigh scattering from helium atoms decreases by collective effects in the atmospheres of cool white dwarf stars. Their study is here extended to consider an accurate evaluation of the atomic polarizability and the density effects involved in the Rayleigh cross-section over a wide density-temperature region. The dynamic dipole polarizability of helium atoms in the ground state is determinated with the oscillator-strength distribution approach. The spectral density of oscillator strength considered includes most significant single and doubly excited transitions to discrete and continuum energies. Static and dynamic polarizability results are confronted with experiments and other theoretical evaluations shown a very good agreement. In addition, the refractive index of helium is evaluated with the Lorentz- Lorenz equation and shows a satisfactory agreement with the most recent experiments. The effect of spatial correlation of atoms on the Rayleigh scattering is calculated with Monte Carlo simulations and effective energy potentials that represent the particle interactions, covering fluid densities between 0.005 and a few g cm-3 and temperatures between 1 000 and 15 000 K. We provide analytical fits from which the Rayleigh cross-section of fluid helium can be easily calculated at wavelength λ > 505.35 Å. Collision-induced light scattering was estimated to be the dominant scattering process at densities greater than 1-2 g cm-3 depending on the temperature.
Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
description Iglesias et al. showed that the Rayleigh scattering from helium atoms decreases by collective effects in the atmospheres of cool white dwarf stars. Their study is here extended to consider an accurate evaluation of the atomic polarizability and the density effects involved in the Rayleigh cross-section over a wide density-temperature region. The dynamic dipole polarizability of helium atoms in the ground state is determinated with the oscillator-strength distribution approach. The spectral density of oscillator strength considered includes most significant single and doubly excited transitions to discrete and continuum energies. Static and dynamic polarizability results are confronted with experiments and other theoretical evaluations shown a very good agreement. In addition, the refractive index of helium is evaluated with the Lorentz- Lorenz equation and shows a satisfactory agreement with the most recent experiments. The effect of spatial correlation of atoms on the Rayleigh scattering is calculated with Monte Carlo simulations and effective energy potentials that represent the particle interactions, covering fluid densities between 0.005 and a few g cm-3 and temperatures between 1 000 and 15 000 K. We provide analytical fits from which the Rayleigh cross-section of fluid helium can be easily calculated at wavelength λ > 505.35 Å. Collision-induced light scattering was estimated to be the dominant scattering process at densities greater than 1-2 g cm-3 depending on the temperature.
publishDate 2018
dc.date.none.fl_str_mv 2018-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/63141
Rohrmann, Rene Daniel; Rayleigh scattering in dense fluid helium; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 473; 1; 1-2018; 457-469
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/63141
identifier_str_mv Rohrmann, Rene Daniel; Rayleigh scattering in dense fluid helium; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 473; 1; 1-2018; 457-469
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2440
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/473/1/457/4222615
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1709.07076
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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