Non-boltzmannian distributions observed in small bodies of the solar system
Autor(a) principal: | |
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Data de Publicação: | 2020 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFBA |
Texto Completo: | http://repositorio.ufba.br/ri/handle/ri/33700 |
Resumo: | Previous works have shown that some features of small bodies of the Solar System (mass, diameters, rotation periods, and apparent magnitudes) are relatively well modeled by distributions originally derived from Tsallis statistical mechanics. Some of the observed distributions are fitted in almost the entire range of the variables, different from other distributions. We revisit these previous studies and update them with recent data. Our results corroborate the previous ones, – that distributions based on the q-exponential family are usually found in statistical description of these planetary systems –, and reinforce the conjecture that the underlying mechanism that generates these observed data may have a nonextensive nature. |
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Borges, Ernesto PinheiroBetzler, Alberto SilvaBorges, Ernesto PinheiroBetzler, Alberto Silva2021-07-05T21:11:43Z2021-07-05T21:11:43Z2020-04BORGES, Ernesto Pinheiro; BETZLER, Alberto Silva. Non-boltzmannian distributions observed in small bodies of the solar system. L’accademia Nazionale Delle Scienze, Roma, v. 44, p. 89-97, abr. 2020. Disponível em: https://www.accademiaxl.it/pubblicazioni-2/rendiconti-on-line/. Acesso em: 05 jul. 2021.0392-4130http://repositorio.ufba.br/ri/handle/ri/33700v. 44Previous works have shown that some features of small bodies of the Solar System (mass, diameters, rotation periods, and apparent magnitudes) are relatively well modeled by distributions originally derived from Tsallis statistical mechanics. Some of the observed distributions are fitted in almost the entire range of the variables, different from other distributions. We revisit these previous studies and update them with recent data. Our results corroborate the previous ones, – that distributions based on the q-exponential family are usually found in statistical description of these planetary systems –, and reinforce the conjecture that the underlying mechanism that generates these observed data may have a nonextensive nature.Submitted by Alberto Silva Betzler (a_betzler@yahoo.com) on 2021-05-08T01:08:33Z No. of bitstreams: 1 14.E.P.Borges-A.S.Betzler.pdf: 315907 bytes, checksum: cc82af9e6f31e9cf6eae1997b6273b9e (MD5)Approved for entry into archive by Solange Rocha (soluny@gmail.com) on 2021-07-05T21:11:43Z (GMT) No. of bitstreams: 1 14.E.P.Borges-A.S.Betzler.pdf: 315907 bytes, checksum: cc82af9e6f31e9cf6eae1997b6273b9e (MD5)Made available in DSpace on 2021-07-05T21:11:43Z (GMT). No. of bitstreams: 1 14.E.P.Borges-A.S.Betzler.pdf: 315907 bytes, checksum: cc82af9e6f31e9cf6eae1997b6273b9e (MD5) Previous issue date: 2020-04Roma, ItaliaL’Accademia Nazionale delle ScienzeBrasilhttps://www.accademiaxl.it/pubblicazioni-2/rendiconti-on-line/reponame:Repositório Institucional da UFBAinstname:Universidade Federal da Bahia (UFBA)instacron:UFBAAsteroidsMeteorsMeteoritesStatistical mechanicsSolar systemNon-boltzmannian distributions observed in small bodies of the solar systeminfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleinfo:eu-repo/semantics/openAccessengORIGINAL14.E.P.Borges-A.S.Betzler.pdf14.E.P.Borges-A.S.Betzler.pdfapplication/pdf315907https://repositorio.ufba.br/bitstream/ri/33700/1/14.E.P.Borges-A.S.Betzler.pdfcc82af9e6f31e9cf6eae1997b6273b9eMD51LICENSElicense.txtlicense.txttext/plain1442https://repositorio.ufba.br/bitstream/ri/33700/2/license.txt817035eff4c4c7dda1d546e170ee2a1aMD52TEXT14.E.P.Borges-A.S.Betzler.pdf.txt14.E.P.Borges-A.S.Betzler.pdf.txtExtracted texttext/plain31716https://repositorio.ufba.br/bitstream/ri/33700/3/14.E.P.Borges-A.S.Betzler.pdf.txt9a2ee5f2a22a2d45b1bcd626a9a76811MD53ri/337002022-08-08 13:17:39.071oai:repositorio.ufba.br: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Repositório InstitucionalPUBhttp://192.188.11.11:8080/oai/requestopendoar:19322022-08-08T16:17:39Repositório Institucional da UFBA - Universidade Federal da Bahia (UFBA)false |
dc.title.pt_BR.fl_str_mv |
Non-boltzmannian distributions observed in small bodies of the solar system |
title |
Non-boltzmannian distributions observed in small bodies of the solar system |
spellingShingle |
Non-boltzmannian distributions observed in small bodies of the solar system Borges, Ernesto Pinheiro Asteroids Meteors Meteorites Statistical mechanics Solar system |
title_short |
Non-boltzmannian distributions observed in small bodies of the solar system |
title_full |
Non-boltzmannian distributions observed in small bodies of the solar system |
title_fullStr |
Non-boltzmannian distributions observed in small bodies of the solar system |
title_full_unstemmed |
Non-boltzmannian distributions observed in small bodies of the solar system |
title_sort |
Non-boltzmannian distributions observed in small bodies of the solar system |
author |
Borges, Ernesto Pinheiro |
author_facet |
Borges, Ernesto Pinheiro Betzler, Alberto Silva |
author_role |
author |
author2 |
Betzler, Alberto Silva |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Borges, Ernesto Pinheiro Betzler, Alberto Silva Borges, Ernesto Pinheiro Betzler, Alberto Silva |
dc.subject.por.fl_str_mv |
Asteroids Meteors Meteorites Statistical mechanics Solar system |
topic |
Asteroids Meteors Meteorites Statistical mechanics Solar system |
description |
Previous works have shown that some features of small bodies of the Solar System (mass, diameters, rotation periods, and apparent magnitudes) are relatively well modeled by distributions originally derived from Tsallis statistical mechanics. Some of the observed distributions are fitted in almost the entire range of the variables, different from other distributions. We revisit these previous studies and update them with recent data. Our results corroborate the previous ones, – that distributions based on the q-exponential family are usually found in statistical description of these planetary systems –, and reinforce the conjecture that the underlying mechanism that generates these observed data may have a nonextensive nature. |
publishDate |
2020 |
dc.date.issued.fl_str_mv |
2020-04 |
dc.date.accessioned.fl_str_mv |
2021-07-05T21:11:43Z |
dc.date.available.fl_str_mv |
2021-07-05T21:11:43Z |
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 |
BORGES, Ernesto Pinheiro; BETZLER, Alberto Silva. Non-boltzmannian distributions observed in small bodies of the solar system. L’accademia Nazionale Delle Scienze, Roma, v. 44, p. 89-97, abr. 2020. Disponível em: https://www.accademiaxl.it/pubblicazioni-2/rendiconti-on-line/. Acesso em: 05 jul. 2021. |
dc.identifier.uri.fl_str_mv |
http://repositorio.ufba.br/ri/handle/ri/33700 |
dc.identifier.issn.none.fl_str_mv |
0392-4130 |
dc.identifier.number.pt_BR.fl_str_mv |
v. 44 |
identifier_str_mv |
BORGES, Ernesto Pinheiro; BETZLER, Alberto Silva. Non-boltzmannian distributions observed in small bodies of the solar system. L’accademia Nazionale Delle Scienze, Roma, v. 44, p. 89-97, abr. 2020. Disponível em: https://www.accademiaxl.it/pubblicazioni-2/rendiconti-on-line/. Acesso em: 05 jul. 2021. 0392-4130 v. 44 |
url |
http://repositorio.ufba.br/ri/handle/ri/33700 |
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 |
L’Accademia Nazionale delle Scienze |
dc.publisher.country.fl_str_mv |
Brasil |
publisher.none.fl_str_mv |
L’Accademia Nazionale delle Scienze |
dc.source.pt_BR.fl_str_mv |
https://www.accademiaxl.it/pubblicazioni-2/rendiconti-on-line/ |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFBA instname:Universidade Federal da Bahia (UFBA) instacron:UFBA |
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Universidade Federal da Bahia (UFBA) |
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Repositório Institucional da UFBA |
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