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Irradiation effects in CO and CO2 ices induced by swift heavy Ni ions at 46 MeV and 537 MeV

Authors :
Domaracka, Alicja
Seperuelo Duarte, Eduardo
Boduch, Philippe
Rothard, Hermann
Balanzat, Emmanuel
Dartois, Emmanuel
Pilling, Sergio
Farenzena, L. S.
Da Silveira, Enio Frota
Centre de recherche sur les Ions, les MAtériaux et la Photonique (CIMAP - UMR 6252)
Centre National de la Recherche Scientifique (CNRS)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN)
Normandie Université (NU)-Normandie Université (NU)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Caen Normandie (UNICAEN)
Normandie Université (NU)
Pontifícia Universidade Católica, Departamento de Física (PUC)
Pontifícia Universidade Católica
Grupo de Fisica e Astronomia (CEFET/Quimica de Nilopolis)
CEFET-RN : Federal Center for Technological Education of Rio Grande do Norte
Institut d'astrophysique spatiale (IAS)
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Instituto de Pesquisa & Desenvolvimento (IP&D)
Universidade do Vale do Paraiba (UNIVAP)
Departamento de Física [Universidade Federal de Santa Catarina]
Universidade Federal de Santa Catarina = Federal University of Santa Catarina [Florianópolis] (UFSC)
K. Cunha
M. Spite
B. Barbuy
Université de Caen Normandie (UNICAEN)
Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN)
Normandie Université (NU)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche sur les Matériaux Avancés (IRMA)
Normandie Université (NU)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Rouen Normandie (UNIROUEN)
Normandie Université (NU)-Institut national des sciences appliquées Rouen Normandie (INSA Rouen Normandie)
Institut National des Sciences Appliquées (INSA)-Normandie Université (NU)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Rouen Normandie (UNIROUEN)
Institut National des Sciences Appliquées (INSA)-Normandie Université (NU)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
Source :
Proceedings of the International Astronomical Union 5 (2010) 428-429 / Symposium S265-Chemical abundances in the Universe – connecting First Stars to Planets, Proceedings of the International Astronomical Union 5 (2010) 428-429 / Symposium S265-Chemical abundances in the Universe – connecting First Stars to Planets, 2009, France. pp.428-429
Publication Year :
2009
Publisher :
HAL CCSD, 2009.

Abstract

International audience; In order to simulate the effects of the heavy ion component of cosmic rays on ices in astrophysical environments, the CO and CO2 ices were irradiated with swift nickel ions in the electronic energy loss regime. The ices were prepared by condensing gas onto a CsI substrate at a temperature of 14 K and analyzed by means of infrared (FTIR) spectroscopy. The physical process of deposition by Ni ions is similar to more important and abundant heavy cosmic rays such as Fe ions. Dissociation of the ice molecules, and formation of new molecules were observed. Also, sputtering (leading to desorption of molecules from the solid surface to the gas phase) was observed. It was found that the sputtering yield due to heavy ions cannot be neglected with respect to desorption induced by weakly ionizing particles such as UV photons and protons.

Details

Language :
English
Database :
OpenAIRE
Journal :
Proceedings of the International Astronomical Union 5 (2010) 428-429 / Symposium S265-Chemical abundances in the Universe – connecting First Stars to Planets, Proceedings of the International Astronomical Union 5 (2010) 428-429 / Symposium S265-Chemical abundances in the Universe – connecting First Stars to Planets, 2009, France. pp.428-429
Accession number :
edsair.dedup.wf.001..7ad2358535ed8de5148904ca1f792660