Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades

Detalhes bibliográficos
Autor(a) principal: Soares, B. B.
Data de Publicação: 2005
Outros Autores: Carvalho, J. C., Nascimento Júnior, José Dias do, de Medeiros, J. R.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRN
Texto Completo: https://repositorio.ufrn.br/jspui/handle/123456789/29004
Resumo: In the present study we use a Tsallis maximum entropy distribution law to fit the observed distribution of projected rotational velocity measurements of stars in the Pleiades open cluster. This new distribution function which generalizes the Maxwell–Boltzmann one is derived from the non-extensivity generalization of Boltzmann–Gibbs entropy. We present a comparison between results from the generalized distribution and the Maxwellian law and show that the generalized distribution fits more closely the data
id UFRN_d49102cf1e1fab3dea072a8ae32d49ca
oai_identifier_str oai:https://repositorio.ufrn.br:123456789/29004
network_acronym_str UFRN
network_name_str Repositório Institucional da UFRN
repository_id_str
spelling Soares, B. B.Carvalho, J. C.Nascimento Júnior, José Dias dode Medeiros, J. R.2020-05-19T17:42:42Z2020-05-19T17:42:42Z2005-09-23SOARES, B.b.; CARVALHO, J.c.; NASCIMENTO JUNIOR, J.d. do; MEDEIROS, J.r. de. Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades. Physica A: Statistical Mechanics and its Applications, [s.l.], v. 364, p. 413-422, maio 2006. Disponível em: http://dx.doi.org/10.1016/j.physa.2005.08.064. Acesso em: 12 mai. 2020. Com permissão da As“Reproduzidotronomy & Astrophysics, © ESO”.1678-765Xhttps://repositorio.ufrn.br/jspui/handle/123456789/2900410.1016/j.physa.2005.08.064In the present study we use a Tsallis maximum entropy distribution law to fit the observed distribution of projected rotational velocity measurements of stars in the Pleiades open cluster. This new distribution function which generalizes the Maxwell–Boltzmann one is derived from the non-extensivity generalization of Boltzmann–Gibbs entropy. We present a comparison between results from the generalized distribution and the Maxwellian law and show that the generalized distribution fits more closely the dataIn the present study we use a Tsallis maximum entropy distribution law to fit the observed distribution of projected rotational velocity measurements of stars in the Pleiades open cluster. This new distribution function which generalizes the Maxwell–Boltzmann one is derived from the non-extensivity generalization of Boltzmann–Gibbs entropy. We present a comparison between results from the generalized distribution and the Maxwellian law and show that the generalized distribution fits more closely the dataElsevier Inc.StarsRotationDistributionMain sequenceOpen clusterTsallis maximum entropy distribution function for stellar rotational velocities in the Pleiadesinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleengreponame:Repositório Institucional da UFRNinstname:Universidade Federal do Rio Grande do Norte (UFRN)instacron:UFRNinfo:eu-repo/semantics/openAccessORIGINALTsallisMaximumEntropyDistributionFunction_2006.pdfTsallisMaximumEntropyDistributionFunction_2006.pdfArtigoapplication/pdf232635https://repositorio.ufrn.br/bitstream/123456789/29004/1/TsallisMaximumEntropyDistributionFunction_2006.pdfec0ab3d0e19c68c211e3b3fd567b7025MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81484https://repositorio.ufrn.br/bitstream/123456789/29004/2/license.txte9597aa2854d128fd968be5edc8a28d9MD52TEXTTsallisMaximumEntropyDistributionFunction_2006.pdf.txtTsallisMaximumEntropyDistributionFunction_2006.pdf.txtExtracted texttext/plain29114https://repositorio.ufrn.br/bitstream/123456789/29004/3/TsallisMaximumEntropyDistributionFunction_2006.pdf.txt13601bad2fff40961eb658ee96c74e65MD53THUMBNAILTsallisMaximumEntropyDistributionFunction_2006.pdf.jpgTsallisMaximumEntropyDistributionFunction_2006.pdf.jpgGenerated Thumbnailimage/jpeg1712https://repositorio.ufrn.br/bitstream/123456789/29004/4/TsallisMaximumEntropyDistributionFunction_2006.pdf.jpg0066833a104d0e4ae6f4602fdf857badMD54123456789/290042020-05-24 06:21:20.929oai:https://repositorio.ufrn.br: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Repositório de PublicaçõesPUBhttp://repositorio.ufrn.br/oai/opendoar:2020-05-24T09:21:20Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN)false
dc.title.pt_BR.fl_str_mv Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
title Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
spellingShingle Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
Soares, B. B.
Stars
Rotation
Distribution
Main sequence
Open cluster
title_short Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
title_full Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
title_fullStr Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
title_full_unstemmed Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
title_sort Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades
author Soares, B. B.
author_facet Soares, B. B.
Carvalho, J. C.
Nascimento Júnior, José Dias do
de Medeiros, J. R.
author_role author
author2 Carvalho, J. C.
Nascimento Júnior, José Dias do
de Medeiros, J. R.
author2_role author
author
author
dc.contributor.author.fl_str_mv Soares, B. B.
Carvalho, J. C.
Nascimento Júnior, José Dias do
de Medeiros, J. R.
dc.subject.por.fl_str_mv Stars
Rotation
Distribution
Main sequence
Open cluster
topic Stars
Rotation
Distribution
Main sequence
Open cluster
description In the present study we use a Tsallis maximum entropy distribution law to fit the observed distribution of projected rotational velocity measurements of stars in the Pleiades open cluster. This new distribution function which generalizes the Maxwell–Boltzmann one is derived from the non-extensivity generalization of Boltzmann–Gibbs entropy. We present a comparison between results from the generalized distribution and the Maxwellian law and show that the generalized distribution fits more closely the data
publishDate 2005
dc.date.issued.fl_str_mv 2005-09-23
dc.date.accessioned.fl_str_mv 2020-05-19T17:42:42Z
dc.date.available.fl_str_mv 2020-05-19T17:42:42Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.citation.fl_str_mv SOARES, B.b.; CARVALHO, J.c.; NASCIMENTO JUNIOR, J.d. do; MEDEIROS, J.r. de. Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades. Physica A: Statistical Mechanics and its Applications, [s.l.], v. 364, p. 413-422, maio 2006. Disponível em: http://dx.doi.org/10.1016/j.physa.2005.08.064. Acesso em: 12 mai. 2020. Com permissão da As“Reproduzidotronomy & Astrophysics, © ESO”.
dc.identifier.uri.fl_str_mv https://repositorio.ufrn.br/jspui/handle/123456789/29004
dc.identifier.issn.none.fl_str_mv 1678-765X
dc.identifier.doi.none.fl_str_mv 10.1016/j.physa.2005.08.064
identifier_str_mv SOARES, B.b.; CARVALHO, J.c.; NASCIMENTO JUNIOR, J.d. do; MEDEIROS, J.r. de. Tsallis maximum entropy distribution function for stellar rotational velocities in the Pleiades. Physica A: Statistical Mechanics and its Applications, [s.l.], v. 364, p. 413-422, maio 2006. Disponível em: http://dx.doi.org/10.1016/j.physa.2005.08.064. Acesso em: 12 mai. 2020. Com permissão da As“Reproduzidotronomy & Astrophysics, © ESO”.
1678-765X
10.1016/j.physa.2005.08.064
url https://repositorio.ufrn.br/jspui/handle/123456789/29004
dc.language.iso.fl_str_mv eng
language eng
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Elsevier Inc.
publisher.none.fl_str_mv Elsevier Inc.
dc.source.none.fl_str_mv reponame:Repositório Institucional da UFRN
instname:Universidade Federal do Rio Grande do Norte (UFRN)
instacron:UFRN
instname_str Universidade Federal do Rio Grande do Norte (UFRN)
instacron_str UFRN
institution UFRN
reponame_str Repositório Institucional da UFRN
collection Repositório Institucional da UFRN
bitstream.url.fl_str_mv https://repositorio.ufrn.br/bitstream/123456789/29004/1/TsallisMaximumEntropyDistributionFunction_2006.pdf
https://repositorio.ufrn.br/bitstream/123456789/29004/2/license.txt
https://repositorio.ufrn.br/bitstream/123456789/29004/3/TsallisMaximumEntropyDistributionFunction_2006.pdf.txt
https://repositorio.ufrn.br/bitstream/123456789/29004/4/TsallisMaximumEntropyDistributionFunction_2006.pdf.jpg
bitstream.checksum.fl_str_mv ec0ab3d0e19c68c211e3b3fd567b7025
e9597aa2854d128fd968be5edc8a28d9
13601bad2fff40961eb658ee96c74e65
0066833a104d0e4ae6f4602fdf857bad
bitstream.checksumAlgorithm.fl_str_mv MD5
MD5
MD5
MD5
repository.name.fl_str_mv Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN)
repository.mail.fl_str_mv
_version_ 1814832986503249920

Registros relacionados