Experimental Computational Simulation of a Galaxy Cluster
Autor(a) principal: | |
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Data de Publicação: | 2023 |
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Tipo de documento: | Artigo |
Idioma: | por |
Título da fonte: | The Journal of Engineering and Exact Sciences |
Texto Completo: | https://periodicos.ufv.br/jcec/article/view/16537 |
Resumo: | Galaxy clusters are large structures composed of galaxies, intra-cluster gas, and dark matter. The kinematics of their constituent galaxies are still studied observationally, although computational experiments serve as true simulation laboratories, reproducing observational aspects in these systems. In fact, while astrophysicists observe two-dimensional projections of three-dimensional objects in the sky with telescopes, computer models simulate three-dimensional systems, using the laws of physics in an attempt to recover observational aspects. In light of the above, this work focuses on the computational simulation of a galaxy cluster, examining its dynamic stability, the physical aspects of its galaxies, and the observational counterpart of its member galaxies. |
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Experimental Computational Simulation of a Galaxy ClusterExperimento Computacional de uma Simulação de um Aglomerado de Galáxiasgravitação, n-corpos, Gadget-2.gravitation, n-body, Gadget-2.Galaxy clusters are large structures composed of galaxies, intra-cluster gas, and dark matter. The kinematics of their constituent galaxies are still studied observationally, although computational experiments serve as true simulation laboratories, reproducing observational aspects in these systems. In fact, while astrophysicists observe two-dimensional projections of three-dimensional objects in the sky with telescopes, computer models simulate three-dimensional systems, using the laws of physics in an attempt to recover observational aspects. In light of the above, this work focuses on the computational simulation of a galaxy cluster, examining its dynamic stability, the physical aspects of its galaxies, and the observational counterpart of its member galaxies.Os aglomerados de galáxias são grandes estruturas composta por galáxias, gás intra-aglomerado e matéria escura. A cinemática de suas galáxias constituintes ainda é estudada observacionalmente, embora experimentos computacionais constituam em verdadeiros laboratórios de simulação, reproduzindo os aspectos observacionais nestes sistemas. De fato, enquanto os astrofísicos observam projeções bidimensionais de objetos tridimensionais no céu com os telescópios, no computador são modelados sistemas tridimensionais, usando as leis da física na tentativa de se recuperar os aspectos observacionais. Diante do exposto, estudamos neste trabalho a simulação computacional de um aglomerado de galáxias, verificando sua estabilidade dinâmica, os aspectos físicos de suas galáxias e a contrapartida observacional de suas galáxias membros.Universidade Federal de Viçosa - UFV2023-09-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://periodicos.ufv.br/jcec/article/view/1653710.18540/jcecvl9iss7pp16537-01eThe Journal of Engineering and Exact Sciences; Vol. 9 No. 7 (2023); 16537-01eThe Journal of Engineering and Exact Sciences; Vol. 9 Núm. 7 (2023); 16537-01eThe Journal of Engineering and Exact Sciences; v. 9 n. 7 (2023); 16537-01e2527-1075reponame:The Journal of Engineering and Exact Sciencesinstname:Universidade Federal de Viçosa (UFV)instacron:UFVporhttps://periodicos.ufv.br/jcec/article/view/16537/8223Copyright (c) 2023 The Journal of Engineering and Exact Scienceshttps://creativecommons.org/licenses/by/4.0info:eu-repo/semantics/openAccessBrandão, Claudio Soriano de SouzaSales, Jorge Henrique de Oliveira2023-09-22T19:34:35Zoai:ojs.periodicos.ufv.br:article/16537Revistahttp://www.seer.ufv.br/seer/rbeq2/index.php/req2/oai2527-10752527-1075opendoar:2023-09-22T19:34:35The Journal of Engineering and Exact Sciences - Universidade Federal de Viçosa (UFV)false |
dc.title.none.fl_str_mv |
Experimental Computational Simulation of a Galaxy Cluster Experimento Computacional de uma Simulação de um Aglomerado de Galáxias |
title |
Experimental Computational Simulation of a Galaxy Cluster |
spellingShingle |
Experimental Computational Simulation of a Galaxy Cluster Brandão, Claudio Soriano de Souza gravitação, n-corpos, Gadget-2. gravitation, n-body, Gadget-2. |
title_short |
Experimental Computational Simulation of a Galaxy Cluster |
title_full |
Experimental Computational Simulation of a Galaxy Cluster |
title_fullStr |
Experimental Computational Simulation of a Galaxy Cluster |
title_full_unstemmed |
Experimental Computational Simulation of a Galaxy Cluster |
title_sort |
Experimental Computational Simulation of a Galaxy Cluster |
author |
Brandão, Claudio Soriano de Souza |
author_facet |
Brandão, Claudio Soriano de Souza Sales, Jorge Henrique de Oliveira |
author_role |
author |
author2 |
Sales, Jorge Henrique de Oliveira |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Brandão, Claudio Soriano de Souza Sales, Jorge Henrique de Oliveira |
dc.subject.por.fl_str_mv |
gravitação, n-corpos, Gadget-2. gravitation, n-body, Gadget-2. |
topic |
gravitação, n-corpos, Gadget-2. gravitation, n-body, Gadget-2. |
description |
Galaxy clusters are large structures composed of galaxies, intra-cluster gas, and dark matter. The kinematics of their constituent galaxies are still studied observationally, although computational experiments serve as true simulation laboratories, reproducing observational aspects in these systems. In fact, while astrophysicists observe two-dimensional projections of three-dimensional objects in the sky with telescopes, computer models simulate three-dimensional systems, using the laws of physics in an attempt to recover observational aspects. In light of the above, this work focuses on the computational simulation of a galaxy cluster, examining its dynamic stability, the physical aspects of its galaxies, and the observational counterpart of its member galaxies. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-09-08 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
https://periodicos.ufv.br/jcec/article/view/16537 10.18540/jcecvl9iss7pp16537-01e |
url |
https://periodicos.ufv.br/jcec/article/view/16537 |
identifier_str_mv |
10.18540/jcecvl9iss7pp16537-01e |
dc.language.iso.fl_str_mv |
por |
language |
por |
dc.relation.none.fl_str_mv |
https://periodicos.ufv.br/jcec/article/view/16537/8223 |
dc.rights.driver.fl_str_mv |
Copyright (c) 2023 The Journal of Engineering and Exact Sciences https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess |
rights_invalid_str_mv |
Copyright (c) 2023 The Journal of Engineering and Exact Sciences https://creativecommons.org/licenses/by/4.0 |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.publisher.none.fl_str_mv |
Universidade Federal de Viçosa - UFV |
publisher.none.fl_str_mv |
Universidade Federal de Viçosa - UFV |
dc.source.none.fl_str_mv |
The Journal of Engineering and Exact Sciences; Vol. 9 No. 7 (2023); 16537-01e The Journal of Engineering and Exact Sciences; Vol. 9 Núm. 7 (2023); 16537-01e The Journal of Engineering and Exact Sciences; v. 9 n. 7 (2023); 16537-01e 2527-1075 reponame:The Journal of Engineering and Exact Sciences instname:Universidade Federal de Viçosa (UFV) instacron:UFV |
instname_str |
Universidade Federal de Viçosa (UFV) |
instacron_str |
UFV |
institution |
UFV |
reponame_str |
The Journal of Engineering and Exact Sciences |
collection |
The Journal of Engineering and Exact Sciences |
repository.name.fl_str_mv |
The Journal of Engineering and Exact Sciences - Universidade Federal de Viçosa (UFV) |
repository.mail.fl_str_mv |
|
_version_ |
1808845241383387136 |