UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS
Autor(a) principal: | |
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Data de Publicação: | 2023 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Revista UniVap (online) |
Texto Completo: | https://revista.univap.br/index.php/revistaunivap/article/view/4415 |
Resumo: | Astrophysical ices (formed by water, among other molecules) act as a catalyst and a reservoir of carbonaceous species, both of which have major implications for astrobiology. In this work, we studied the formation of astrophysical ice nanostructures found in the interstellar medium, having a sheet of graphene as a catalyst substrate, using the classical molecular dynamics technique to model these astrophysical environments. For this, two systems were designed: the first composed of graphene and and the second composed of graphene, and . Initially, a simulation box was built where the area was delimited by graphene whose height varied from 4, 6, 8 and 10 nm. The molecules were evenly distributed throughout the box. The molecular dynamics technique proved to be a promising tool to understand the phenomenon of adsorption of molecules on the substrate, allowing us to realize that the random distribution of molecules in the system interferes with the geometric structure formed by an ice nanostructure. This study allows us to understand, from the nanometric point of view, the influence of some physical-chemical parameters, regarding the formation of nanostructures of astrophysical ices, such as the number of hydrogen bonds, the initial size of the simulation box, and its density during the freezing process |
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UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICSCOMPREENDENDO A FORMAÇÃO DE NANOESTRUTURAS EM GELO ASTROFÍSICOS ATRAVÉS DA DINÂMICA MOLECULAR CLÁSSICAdinâmica molecular clássicagelo astrofísicoformação de nanoestruturas de gelos adsorvidas a substratoastroquímicaastrofísicaAstrophysical iceMolecular dynamicsAstrochemistryClassical molecular dynamicsastrophysical iceformation of substrate-adsorbed ice nanostructuresastrochemistryastrophysicsAstrophysical ices (formed by water, among other molecules) act as a catalyst and a reservoir of carbonaceous species, both of which have major implications for astrobiology. In this work, we studied the formation of astrophysical ice nanostructures found in the interstellar medium, having a sheet of graphene as a catalyst substrate, using the classical molecular dynamics technique to model these astrophysical environments. For this, two systems were designed: the first composed of graphene and and the second composed of graphene, and . Initially, a simulation box was built where the area was delimited by graphene whose height varied from 4, 6, 8 and 10 nm. The molecules were evenly distributed throughout the box. The molecular dynamics technique proved to be a promising tool to understand the phenomenon of adsorption of molecules on the substrate, allowing us to realize that the random distribution of molecules in the system interferes with the geometric structure formed by an ice nanostructure. This study allows us to understand, from the nanometric point of view, the influence of some physical-chemical parameters, regarding the formation of nanostructures of astrophysical ices, such as the number of hydrogen bonds, the initial size of the simulation box, and its density during the freezing processGelos astrofísicos (formados pela água, entre outras moléculas) atuam como um catalisador e um reservatório de espécies carbonáceas, ambas com grandes implicações para a astrobiologia. Neste trabalho, nós estudamos a formação de nanoestruturas de gelo astrofísico encontradas no meio interestelar, tendo uma folha de grafeno como substrato catalisador, utilizando-se a técnica de dinâmica molecular clássica para modelar esses ambientes astrofísicos. Para isso, projetou-se dois sistemas: o primeiro composto por grafeno e e o segundo composto por grafeno, e . Inicialmente construiu-se uma caixa de simulação onde a área foi delimitada pelo grafeno cuja altura variava de 4, 6, 8 e 10 nm. As moléculas foram distribuídas uniformemente por toda a caixa. A técnica de dinâmica molecular provou ser uma ferramenta promissora para entender o fenômeno da adsorção de moléculas no substrato, permitindo-nos perceber que a distribuição aleatória de moléculas no sistema interfere com a estrutura geométrica formada por uma nanoestrutura de gelo. Este estudo nos permite compreender, do ponto de vista nanométrico, a influência de alguns parâmetros físico-químicos, no que tange a formação das nanoestruturas de gelos astrofísicos, como o número de ligações de hidrogênio, o tamanho inicial da caixa de simulação, e sua densidade durante o processo de congelamentoIBICT2023-10-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionTextoinfo:eu-repo/semantics/otherapplication/pdfhttps://revista.univap.br/index.php/revistaunivap/article/view/441510.18066/revistaunivap.v29i61.4415Revista Univap; Vol. 29 No. 61 (2023): Revista UnivapRevista Univap; v. 29 n. 61 (2023): Revista Univap2237-17531517-327510.18066/revistaunivap.v29i61reponame:Revista UniVap (online)instname:Universidade do Vale do Paraíba (Univap)instacron:UNIVAPenghttps://revista.univap.br/index.php/revistaunivap/article/view/4415/2256NationalNacionalCopyright (c) 2023 Revista Univaphttps://creativecommons.org/licenses/by/4.0info:eu-repo/semantics/openAccessSilva, Priscila Alves da Oliveira, Sergio Pilling Guapyassu deAmarim, Rodrigo Garcia2023-04-20T12:47:41Zoai:ojs.biblioteca.univap.br:article/4415Revistahttps://revista.univap.br/index.php/revistaunivapPRIhttps://revista.univap.br/index.php/revistaunivap/oairevista@univap.br2237-17532237-1753opendoar:2023-04-20T12:47:41Revista UniVap (online) - Universidade do Vale do Paraíba (Univap)false |
dc.title.none.fl_str_mv |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS COMPREENDENDO A FORMAÇÃO DE NANOESTRUTURAS EM GELO ASTROFÍSICOS ATRAVÉS DA DINÂMICA MOLECULAR CLÁSSICA |
title |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
spellingShingle |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS Silva, Priscila Alves da dinâmica molecular clássica gelo astrofísico formação de nanoestruturas de gelos adsorvidas a substrato astroquímica astrofísica Astrophysical ice Molecular dynamics Astrochemistry Classical molecular dynamics astrophysical ice formation of substrate-adsorbed ice nanostructures astrochemistry astrophysics |
title_short |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
title_full |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
title_fullStr |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
title_full_unstemmed |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
title_sort |
UNDERSTANDING THE ASTROPHYSICAL-ICE NANOSTRUCTURES FORMATION THROUGH CLASSICAL MOLECULAR DYNAMICS |
author |
Silva, Priscila Alves da |
author_facet |
Silva, Priscila Alves da Oliveira, Sergio Pilling Guapyassu de Amarim, Rodrigo Garcia |
author_role |
author |
author2 |
Oliveira, Sergio Pilling Guapyassu de Amarim, Rodrigo Garcia |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Silva, Priscila Alves da Oliveira, Sergio Pilling Guapyassu de Amarim, Rodrigo Garcia |
dc.subject.por.fl_str_mv |
dinâmica molecular clássica gelo astrofísico formação de nanoestruturas de gelos adsorvidas a substrato astroquímica astrofísica Astrophysical ice Molecular dynamics Astrochemistry Classical molecular dynamics astrophysical ice formation of substrate-adsorbed ice nanostructures astrochemistry astrophysics |
topic |
dinâmica molecular clássica gelo astrofísico formação de nanoestruturas de gelos adsorvidas a substrato astroquímica astrofísica Astrophysical ice Molecular dynamics Astrochemistry Classical molecular dynamics astrophysical ice formation of substrate-adsorbed ice nanostructures astrochemistry astrophysics |
description |
Astrophysical ices (formed by water, among other molecules) act as a catalyst and a reservoir of carbonaceous species, both of which have major implications for astrobiology. In this work, we studied the formation of astrophysical ice nanostructures found in the interstellar medium, having a sheet of graphene as a catalyst substrate, using the classical molecular dynamics technique to model these astrophysical environments. For this, two systems were designed: the first composed of graphene and and the second composed of graphene, and . Initially, a simulation box was built where the area was delimited by graphene whose height varied from 4, 6, 8 and 10 nm. The molecules were evenly distributed throughout the box. The molecular dynamics technique proved to be a promising tool to understand the phenomenon of adsorption of molecules on the substrate, allowing us to realize that the random distribution of molecules in the system interferes with the geometric structure formed by an ice nanostructure. This study allows us to understand, from the nanometric point of view, the influence of some physical-chemical parameters, regarding the formation of nanostructures of astrophysical ices, such as the number of hydrogen bonds, the initial size of the simulation box, and its density during the freezing process |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-10-04 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Texto info:eu-repo/semantics/other |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
https://revista.univap.br/index.php/revistaunivap/article/view/4415 10.18066/revistaunivap.v29i61.4415 |
url |
https://revista.univap.br/index.php/revistaunivap/article/view/4415 |
identifier_str_mv |
10.18066/revistaunivap.v29i61.4415 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
https://revista.univap.br/index.php/revistaunivap/article/view/4415/2256 |
dc.rights.driver.fl_str_mv |
Copyright (c) 2023 Revista Univap https://creativecommons.org/licenses/by/4.0 info:eu-repo/semantics/openAccess |
rights_invalid_str_mv |
Copyright (c) 2023 Revista Univap https://creativecommons.org/licenses/by/4.0 |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.coverage.none.fl_str_mv |
National Nacional |
dc.publisher.none.fl_str_mv |
IBICT |
publisher.none.fl_str_mv |
IBICT |
dc.source.none.fl_str_mv |
Revista Univap; Vol. 29 No. 61 (2023): Revista Univap Revista Univap; v. 29 n. 61 (2023): Revista Univap 2237-1753 1517-3275 10.18066/revistaunivap.v29i61 reponame:Revista UniVap (online) instname:Universidade do Vale do Paraíba (Univap) instacron:UNIVAP |
instname_str |
Universidade do Vale do Paraíba (Univap) |
instacron_str |
UNIVAP |
institution |
UNIVAP |
reponame_str |
Revista UniVap (online) |
collection |
Revista UniVap (online) |
repository.name.fl_str_mv |
Revista UniVap (online) - Universidade do Vale do Paraíba (Univap) |
repository.mail.fl_str_mv |
revista@univap.br |
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1797042284667076608 |