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Physical and spectroscopic properties of pure C2H4 and CH4:C2H4 ices

Authors :
Universitat Politècnica de València. Centro de Tecnologías Físicas: Acústica, Materiales y Astrofísica - Centre de Tecnologies Físiques: Acústica, Materials i Astrofísica
Universitat Politècnica de València. Escuela Politécnica Superior de Alcoy - Escola Politècnica Superior d'Alcoi
European Commission
Ministerio de Economía y Competitividad
Ministerio de Ciencia e Innovación
European Research Council
Molpeceres, Germán
Satorre Aznar, Miguel Ángel
Ortigoso, Juan
Zanchet, Alexandre
Luna Molina, Ramón
Millán Verdú, Carlos
Escribano, Rafael
Tanarro, Isabel
Juan Herrero, Víctor de
Maté, Belén
Universitat Politècnica de València. Centro de Tecnologías Físicas: Acústica, Materiales y Astrofísica - Centre de Tecnologies Físiques: Acústica, Materials i Astrofísica
Universitat Politècnica de València. Escuela Politécnica Superior de Alcoy - Escola Politècnica Superior d'Alcoi
European Commission
Ministerio de Economía y Competitividad
Ministerio de Ciencia e Innovación
European Research Council
Molpeceres, Germán
Satorre Aznar, Miguel Ángel
Ortigoso, Juan
Zanchet, Alexandre
Luna Molina, Ramón
Millán Verdú, Carlos
Escribano, Rafael
Tanarro, Isabel
Juan Herrero, Víctor de
Maté, Belén
Publication Year :
2017

Abstract

[EN] Physical and spectroscopic properties of ices of C2H4 and CH4:C2H4 mixtures with 3:1, 1:1 and 1:3 ratios have been investigated at 30 K. Two laboratories are involved in this work. In one of them, the density and refractive index of the samples have been measured by using a cryogenic quartz microbalance and laser interferometric techniques. In the other one, IR spectra have been recorded in the near- and mid-infrared regions, and band shifts with respect to the pure species, band strengths of the main bands, and the optical constants in both regions have been determined. Previous data on ethylene and the mixtures studied here were scarce. For methane, both the wavenumbers and band strengths have been found to follow a regular pattern of decrease with increasing dilution, but no pattern has been detected for ethylene vibrations. The method employed for the preparation of the samples, by vapour deposition under vacuum, is thought to be adequate to mimic the structure of astrophysical ices. Possible astrophysical implications, especially by means of the optical constants reported here, have been discussed.

Details

Database :
OAIster
Notes :
TEXT, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1138439215
Document Type :
Electronic Resource