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Please use this identifier to cite or link to this item: http://dspace.ucuenca.edu.ec/handle/123456789/37693
Title: Radiolysis of carbon-dioxide ice by swift Ti and Xe ions
Authors: Rothard, Hermann
Trautmann, Christina
Boduch, PHilippe
Bender, Markus
Bordalo, Vinicius
LV, Xue Yang
Mejia Guaman, Christian Fernando
Domaracka, Alicja
Martínez Rodríguez, Rafael Eduardo
Severin, Daniel
metadata.dc.ucuenca.correspondencia: Rothard, Hermann, rothard@ganil.fr
Keywords: Carbon dioxide
Radiolysis
Irradiation
metadata.dc.ucuenca.areaconocimientofrascatiamplio: 1. Ciencias Naturales y Exactas
metadata.dc.ucuenca.areaconocimientofrascatidetallado: 1.3.1 Física Atómica, Molecular y Química(Colisión,etc)
metadata.dc.ucuenca.areaconocimientofrascatiespecifico: 1.3 Ciencias Físicas
metadata.dc.ucuenca.areaconocimientounescoamplio: 05 - Ciencias Físicas, Ciencias Naturales, Matemáticas y Estadísticas
metadata.dc.ucuenca.areaconocimientounescodetallado: 0533 - Física
metadata.dc.ucuenca.areaconocimientounescoespecifico: 053 - Ciencias Físicas
Issue Date: 2015
metadata.dc.ucuenca.volumen: Volumen 365
metadata.dc.source: Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
metadata.dc.identifier.doi: 10.1016 / j.nimb.2015.09.039
metadata.dc.type: ARTÍCULO
Abstract: 
Ices (H2O, CO, CO2, NH3, ..) are omnipresent in space on comets, the moons of giant planets, dust grains in dense clouds (the birthplaces of stars and planetary systems). They are exposed to cosmic rays, which in turn induce radiolysis, i.e. fragmentation of initial molecules, formation of radicals, and subsequent synthesis of molecules. Even complex pre-biotic molecules such as amino acids can be formed. Due to their high electronic energy loss the heavy ion fraction in cosmic rays yields nonnegligible contributions to sputtering and radiolysis, even if protons and alpha particles are more abundant [1]. Heavy-ion beams from large accelerator facilities are useful to simulate the specific effects induced by the heavy ion fraction of cosmic radiation in the laboratory. We complemented the experiments (550 MeV Ti beams) reported in [2] at the UNILAC M-branch, by irradiation with 630 MeV Xe beams. On-line Fourier transform infrared absorption spectroscopy (FTIR) allowed us to follow molecule destruction and synthesis in CO2 ice deposited at approx. 20 K on a CsI substrate.
URI: http://dspace.ucuenca.edu.ec/handle/123456789/37693
https://repository.gsi.de/record/183987/files/APPA-MML-MR-01.pdf
metadata.dc.ucuenca.urifuente: https://www.journals.elsevier.com/
ISSN: 0168-583X
Appears in Collections:Artículos

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