Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries

Detalhes bibliográficos
Autor(a) principal: Pelisoli, Ingrid Domingos
Data de Publicação: 2015
Outros Autores: Santos, Marcio Gabriel dos, Kepler, Souza Oliveira
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/115355
Resumo: We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.
id UFRGS-2_e6f3cbab4c257086b9536cdf220d2e00
oai_identifier_str oai:www.lume.ufrgs.br:10183/115355
network_acronym_str UFRGS-2
network_name_str Repositório Institucional da UFRGS
repository_id_str
spelling Pelisoli, Ingrid DomingosSantos, Marcio Gabriel dosKepler, Souza Oliveira2015-04-15T01:58:22Z20150035-8711http://hdl.handle.net/10183/115355000955058We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.application/pdfengMonthly notices of the royal astronomical society. Oxford [recurso eletrônico]. Vol. 448, n. 3 (April 2015), p. 2332-2343Anãs brancasHidrogênioPrótonsSatélitesAtomic dataLine: profilesWhite dwarfsUnified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetriesEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000955058.pdf000955058.pdfTexto completo (inglês)application/pdf3759592http://www.lume.ufrgs.br/bitstream/10183/115355/1/000955058.pdfd9673535119179dcad2f318850abc27aMD51TEXT000955058.pdf.txt000955058.pdf.txtExtracted Texttext/plain56870http://www.lume.ufrgs.br/bitstream/10183/115355/2/000955058.pdf.txt5cc53f2a55e842d838a88696ad57bbe0MD52THUMBNAIL000955058.pdf.jpg000955058.pdf.jpgGenerated Thumbnailimage/jpeg2087http://www.lume.ufrgs.br/bitstream/10183/115355/3/000955058.pdf.jpg511b5e0215d456b7f7d0b9da3319bb05MD5310183/1153552022-06-17 04:47:17.847584oai:www.lume.ufrgs.br:10183/115355Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2022-06-17T07:47:17Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
spellingShingle Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
Pelisoli, Ingrid Domingos
Anãs brancas
Hidrogênio
Prótons
Satélites
Atomic data
Line: profiles
White dwarfs
title_short Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_full Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_fullStr Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_full_unstemmed Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
title_sort Unified line profiles for hydrogen perturbed by collisions with protons : satellites and asymmetries
author Pelisoli, Ingrid Domingos
author_facet Pelisoli, Ingrid Domingos
Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
author_role author
author2 Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
author2_role author
author
dc.contributor.author.fl_str_mv Pelisoli, Ingrid Domingos
Santos, Marcio Gabriel dos
Kepler, Souza Oliveira
dc.subject.por.fl_str_mv Anãs brancas
Hidrogênio
Prótons
Satélites
topic Anãs brancas
Hidrogênio
Prótons
Satélites
Atomic data
Line: profiles
White dwarfs
dc.subject.eng.fl_str_mv Atomic data
Line: profiles
White dwarfs
description We present new calculations of unified line profiles for hydrogen perturbed by collisions with protons. We report on new calculations of the potential energies and dipole moments which allow the evaluation of profiles for the lines of the Lyman series up to Lyman δ and the Balmer series up to Balmer 10. Unified calculations only existed for the lines Lyman α to Lyman γ and Balmer α including the H+ 2 quasi-molecule. These data are available as online material accompanying this paper and should be included in atmosphere models, in place of the Stark effect of protons, since the quasi-molecular contributions cause not only satellites, but large asymmetries that are unaccounted for in models that assume that Stark broadening of electrons and that of protons are equal.
publishDate 2015
dc.date.accessioned.fl_str_mv 2015-04-15T01:58:22Z
dc.date.issued.fl_str_mv 2015
dc.type.driver.fl_str_mv Estrangeiro
info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10183/115355
dc.identifier.issn.pt_BR.fl_str_mv 0035-8711
dc.identifier.nrb.pt_BR.fl_str_mv 000955058
identifier_str_mv 0035-8711
000955058
url http://hdl.handle.net/10183/115355
dc.language.iso.fl_str_mv eng
language eng
dc.relation.ispartof.pt_BR.fl_str_mv Monthly notices of the royal astronomical society. Oxford [recurso eletrônico]. Vol. 448, n. 3 (April 2015), p. 2332-2343
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:Repositório Institucional da UFRGS
instname:Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
instname_str Universidade Federal do Rio Grande do Sul (UFRGS)
instacron_str UFRGS
institution UFRGS
reponame_str Repositório Institucional da UFRGS
collection Repositório Institucional da UFRGS
bitstream.url.fl_str_mv http://www.lume.ufrgs.br/bitstream/10183/115355/1/000955058.pdf
http://www.lume.ufrgs.br/bitstream/10183/115355/2/000955058.pdf.txt
http://www.lume.ufrgs.br/bitstream/10183/115355/3/000955058.pdf.jpg
bitstream.checksum.fl_str_mv d9673535119179dcad2f318850abc27a
5cc53f2a55e842d838a88696ad57bbe0
511b5e0215d456b7f7d0b9da3319bb05
bitstream.checksumAlgorithm.fl_str_mv MD5
MD5
MD5
repository.name.fl_str_mv Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)
repository.mail.fl_str_mv
_version_ 1815447579985444864