PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING
Autor(a) principal: | |
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Data de Publicação: | 2023 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | por |
Título da fonte: | Revista UniVap (online) |
Texto Completo: | https://revista.univap.br/index.php/revistaunivap/article/view/4386 |
Resumo: | Astrophysical water-rich ices are always exposed to ionizing radiation in space, as well as, are exposed to eventual temperature changes. In the laboratory, the studies of such ices allow us to understand their behavior and chemical changes, allowing also the quantification of important physicochemical parameters of the ice. In the present work, a sample of water ice at 12 K was irradiated by soft X-rays in the SGM beamline of LNLS/CNPEM until reaching chemical equilibrium, and then it was heated up to 220 K. Using infrared spectroscopy (IR), we mapped the chemical evolution of the sample and quantified the production of its main product, the H2O2 molecule. The study has implications for the chemistry of star-forming regions as well as cold regions of the solar system. |
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PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATINGFOTÓLISE DE GELO DE ÁGUA POR RAIOS-X MOLES E A PRODUÇÃO DE H2O2 DURANTE AS FASES DE IRRADIAÇÃO E AQUECIMENTOGelos astrofísicosH2OH2O2Espectroscopia IRFotóliseRaios-X molesAstroquímicaAstrophysical iceH2OH2O2IR spectroscopyPhotolysisSoft X-raysAstrophysical water-rich ices are always exposed to ionizing radiation in space, as well as, are exposed to eventual temperature changes. In the laboratory, the studies of such ices allow us to understand their behavior and chemical changes, allowing also the quantification of important physicochemical parameters of the ice. In the present work, a sample of water ice at 12 K was irradiated by soft X-rays in the SGM beamline of LNLS/CNPEM until reaching chemical equilibrium, and then it was heated up to 220 K. Using infrared spectroscopy (IR), we mapped the chemical evolution of the sample and quantified the production of its main product, the H2O2 molecule. The study has implications for the chemistry of star-forming regions as well as cold regions of the solar system.Gelos astrofísicos ricos em H2O (água) estão sempre expostos a radiações ionizantes no espaço, assim como a eventuais mudanças de temperatura. Seus estudos em laboratório permitem compreender seus comportamentos e mudanças químicas, além de permitir a quantificação de parâmetros físico-químicos importantes do próprio gelo. No presente trabalho, uma amostra de gelo de água a 12 K foi irradiada por raios-X moles na linha de luz SGM do LNLS/CNPEM até atingir o equilíbrio químico, e em seguida, foi aquecida até 220 K. Utilizando espectroscopia infravermelha (IR), mapeamos a evolução química da amostra e quantificamos a produção do seu principal produto, a molécula de H2O2. O estudo tem implicações na química das regiões de formação estelar, bem como em regiões frias do sistema solar.IBICT2023-03-28info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionTextoinfo:eu-repo/semantics/otherapplication/pdfhttps://revista.univap.br/index.php/revistaunivap/article/view/438610.18066/revistaunivap.v29i61.4386Revista 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:UNIVAPporhttps://revista.univap.br/index.php/revistaunivap/article/view/4386/2215NationalNacionalCopyright (c) 2023 Revista Univaphttps://creativecommons.org/licenses/by/4.0info:eu-repo/semantics/openAccessOliveira, Sergio Pilling Guapyassu deda Silva, Rita de Cassia2023-03-28T22:10:46Zoai:ojs.biblioteca.univap.br:article/4386Revistahttps://revista.univap.br/index.php/revistaunivapPRIhttps://revista.univap.br/index.php/revistaunivap/oairevista@univap.br2237-17532237-1753opendoar:2023-03-28T22:10:46Revista UniVap (online) - Universidade do Vale do Paraíba (Univap)false |
dc.title.none.fl_str_mv |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING FOTÓLISE DE GELO DE ÁGUA POR RAIOS-X MOLES E A PRODUÇÃO DE H2O2 DURANTE AS FASES DE IRRADIAÇÃO E AQUECIMENTO |
title |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
spellingShingle |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING Oliveira, Sergio Pilling Guapyassu de Gelos astrofísicos H2O H2O2 Espectroscopia IR Fotólise Raios-X moles Astroquímica Astrophysical ice H2O H2O2 IR spectroscopy Photolysis Soft X-rays |
title_short |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
title_full |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
title_fullStr |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
title_full_unstemmed |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
title_sort |
PHOTOLYSIS OF ASTROPHYSICAL WATER ICE BY SOFT X-RAYS AND THE PRODUCTION OF H2O2 DURING THE PHASES OF IRRADIATION AND HEATING |
author |
Oliveira, Sergio Pilling Guapyassu de |
author_facet |
Oliveira, Sergio Pilling Guapyassu de da Silva, Rita de Cassia |
author_role |
author |
author2 |
da Silva, Rita de Cassia |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Oliveira, Sergio Pilling Guapyassu de da Silva, Rita de Cassia |
dc.subject.por.fl_str_mv |
Gelos astrofísicos H2O H2O2 Espectroscopia IR Fotólise Raios-X moles Astroquímica Astrophysical ice H2O H2O2 IR spectroscopy Photolysis Soft X-rays |
topic |
Gelos astrofísicos H2O H2O2 Espectroscopia IR Fotólise Raios-X moles Astroquímica Astrophysical ice H2O H2O2 IR spectroscopy Photolysis Soft X-rays |
description |
Astrophysical water-rich ices are always exposed to ionizing radiation in space, as well as, are exposed to eventual temperature changes. In the laboratory, the studies of such ices allow us to understand their behavior and chemical changes, allowing also the quantification of important physicochemical parameters of the ice. In the present work, a sample of water ice at 12 K was irradiated by soft X-rays in the SGM beamline of LNLS/CNPEM until reaching chemical equilibrium, and then it was heated up to 220 K. Using infrared spectroscopy (IR), we mapped the chemical evolution of the sample and quantified the production of its main product, the H2O2 molecule. The study has implications for the chemistry of star-forming regions as well as cold regions of the solar system. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-03-28 |
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/4386 10.18066/revistaunivap.v29i61.4386 |
url |
https://revista.univap.br/index.php/revistaunivap/article/view/4386 |
identifier_str_mv |
10.18066/revistaunivap.v29i61.4386 |
dc.language.iso.fl_str_mv |
por |
language |
por |
dc.relation.none.fl_str_mv |
https://revista.univap.br/index.php/revistaunivap/article/view/4386/2215 |
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 |
_version_ |
1797042284657639424 |