Study of the influence of computational parameters on the formation of a giant gaseous planet
Autor(a) principal: | |
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Data de Publicação: | 2015 |
Outros Autores: | |
Tipo de documento: | Artigo de conferência |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1088/1742-6596/641/1/012012 http://hdl.handle.net/11449/168399 |
Resumo: | Today, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper. |
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Study of the influence of computational parameters on the formation of a giant gaseous planetToday, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper.Universidade Estadual Paulista UNESP Campus de GuaratinguetáUniversidade Estadual Paulista UNESP Campus de GuaratinguetáUniversidade Estadual Paulista (Unesp)Moraes, R. A. [UNESP]Neto, E. Vieira [UNESP]2018-12-11T16:41:06Z2018-12-11T16:41:06Z2015-10-07info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectapplication/pdfhttp://dx.doi.org/10.1088/1742-6596/641/1/012012Journal of Physics: Conference Series, v. 641, n. 1, 2015.1742-65961742-6588http://hdl.handle.net/11449/16839910.1088/1742-6596/641/1/0120122-s2.0-849585975272-s2.0-84958597527.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Physics: Conference Series0,2410,241info:eu-repo/semantics/openAccess2023-11-18T06:11:17Zoai:repositorio.unesp.br:11449/168399Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T18:01:17.959961Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
title |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
spellingShingle |
Study of the influence of computational parameters on the formation of a giant gaseous planet Moraes, R. A. [UNESP] |
title_short |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
title_full |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
title_fullStr |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
title_full_unstemmed |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
title_sort |
Study of the influence of computational parameters on the formation of a giant gaseous planet |
author |
Moraes, R. A. [UNESP] |
author_facet |
Moraes, R. A. [UNESP] Neto, E. Vieira [UNESP] |
author_role |
author |
author2 |
Neto, E. Vieira [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Moraes, R. A. [UNESP] Neto, E. Vieira [UNESP] |
description |
Today, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-10-07 2018-12-11T16:41:06Z 2018-12-11T16:41:06Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
format |
conferenceObject |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1088/1742-6596/641/1/012012 Journal of Physics: Conference Series, v. 641, n. 1, 2015. 1742-6596 1742-6588 http://hdl.handle.net/11449/168399 10.1088/1742-6596/641/1/012012 2-s2.0-84958597527 2-s2.0-84958597527.pdf |
url |
http://dx.doi.org/10.1088/1742-6596/641/1/012012 http://hdl.handle.net/11449/168399 |
identifier_str_mv |
Journal of Physics: Conference Series, v. 641, n. 1, 2015. 1742-6596 1742-6588 10.1088/1742-6596/641/1/012012 2-s2.0-84958597527 2-s2.0-84958597527.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Journal of Physics: Conference Series 0,241 0,241 |
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 |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808128885227782144 |