Compaction of porous ices rich in water by swift heavy ions

dc.contributor.authorMejía Guamán, Christian Fernando
dc.contributor.authorFerreira de Barros, Ana Lucía
dc.contributor.authorSeperuelo Duarte, Eduardo
dc.contributor.authorDa silveira, Énio Frota
dc.contributor.authorDartois, Emmanuel
dc.contributor.authorDomaracka, Alicja
dc.contributor.authorRothard, Hermann
dc.contributor.authorBoduch, Philippe
dc.date.accessioned2021-03-11T14:57:39Z
dc.date.available2021-03-11T14:57:39Z
dc.date.issued2015
dc.description.abstractPorous water ice and water ice mixtures H2O:X (X = CO, CO2 and CH4) produced at 15 K, with film thicknesses in the 0.5–1 μm range, were irradiated by swift ions and monitored by mid-infrared spectroscopy (FTIR). The analysis of the evolution of the pure water ice infrared absorption on ion beam dose reveals a strong correlation among three quantities: (i) the absorbance of the most intense band (3250 cm−1), (ii) the wavelength of the maximum absorbance of this band and (iii) the absorbance of the OH-dangling bonds. This correlation is interpreted as indications of the water ice compaction by irradiation: as the beam fluence increases, the ice porosity decreases, the dangling bond peaks collapse and the area and position of the 3250 cm−1 band vary exponentially, all of them evolving with the same compaction cross section (). The linear dependence ( being the electronic stopping power) is observed for both pure and mixed water ices, confirming previous results. We suggests that the infrared absorption A-value varies with dose as during the compaction process ( eV/molec being the effective energy density to eliminate the OH-db, and is a parameter characterizing the porosity). These findings may be used as a diagnostic tool to probe the morphology of water ices occurring in the outer Solar System and in the ISM.
dc.identifier.doi10.1016/j.icarus.2014.12.002
dc.identifier.issn1090-2643
dc.identifier.urihttps://www.sciencedirect.com/science/article/abs/pii/S0019103514006812
dc.language.isoes_ES
dc.sourceIcarus
dc.subjectCosmic rays
dc.subjectSolar wind
dc.subjectIces
dc.subjectIR spectroscopy
dc.subjectCollisional physics
dc.titleCompaction of porous ices rich in water by swift heavy ions
dc.typeARTÍCULO
dc.ucuenca.afiliacionMejia, C., Pontificia Universidade Católica do Rio de Janeiro, Rio de Janeiro, Brasil; Mejia, C., Universidad de Cuenca, Facultad de Ciencias Químicas, Cuenca, Ecuador
dc.ucuenca.afiliacionFerreira de, A., Centro Federal de Educacao Tecnológica Celso Suckow da Fonseca, Río de Janeiro, Brasil
dc.ucuenca.afiliacionSeperuelo, E., Instituto Federal de Educación, Ciencia e Tecnología do Rio de Janeiro, Rio de Janeiro, Brasil
dc.ucuenca.afiliacionDa silveira, É., Pontificia Universidade Católica do Rio de Janeiro, Rio de Janeiro, Brasil
dc.ucuenca.afiliacionDartois, E., Université Paris Saclay, Saclay, Francia
dc.ucuenca.afiliacionDomaracka, A., École nationale supérieure d ingénieurs de Caen (ENSICAEN), Caen, Francia
dc.ucuenca.afiliacionRothard, H., Normandie Université, Caen, Francia
dc.ucuenca.afiliacionBoduch, P., Normandie Université, Caen, Francia
dc.ucuenca.areaconocimientofrascatiamplio1. Ciencias Naturales y Exactas
dc.ucuenca.areaconocimientofrascatidetallado1.3.8 Astronomía(Incluye Astrofísica, Ciencia Espacial)
dc.ucuenca.areaconocimientofrascatiespecifico1.3 Ciencias Físicas
dc.ucuenca.areaconocimientounescoamplio05 - Ciencias Físicas, Ciencias Naturales, Matemáticas y Estadísticas
dc.ucuenca.areaconocimientounescodetallado0533 - Física
dc.ucuenca.areaconocimientounescoespecifico053 - Ciencias Físicas
dc.ucuenca.correspondenciaMejia Guaman, Christian Fernando, christian.mejia@ucuenca.edu.ec
dc.ucuenca.cuartilQ1
dc.ucuenca.factorimpacto4.21
dc.ucuenca.idautor0301511556
dc.ucuenca.idautor0001-7023-8282
dc.ucuenca.idautor0003-4587-3764
dc.ucuenca.idautor0003-4351-5365
dc.ucuenca.idautor0003-1197-7143
dc.ucuenca.idautorSgrp-4192-6
dc.ucuenca.idautorSgrp-4192-7
dc.ucuenca.idautorSgrp-4192-8
dc.ucuenca.indicebibliograficoSCOPUS
dc.ucuenca.numerocitaciones33
dc.ucuenca.urifuentehttps://www.sciencedirect.com/journal/icarus
dc.ucuenca.versionVersión publicada
dc.ucuenca.volumenVolumen 250

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