| Education |
| 2009 |
Ph.D. in theoretical, analytical and physical chemistry, Université Pierre et Marie Curie, France. |
| 2006 |
Post-graduate diploma of fundamental chemistry, Specialization: theoretical and physical chemistry, Université Pierre et Marie Curie, France. |
| 2005 |
Master of fundamental chemistry, Université Pierre et Marie Curie, France. |
| 2004 |
Chemistry degree, Université Pierre et Marie Curie, France. |
| 2001 - 2003 |
Second year university diploma (D.E.U.G.) of science, Université Pierre et Marie Curie, France. |
| 2001 |
High school diploma scientific. |
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| Appoitments |
| 2008-2009 |
Teaching - general chemistry (78 hours, Ecole de Condé, France). |
| 2008 |
Teaching - general chemistry (60 hours, Institut National du Patrimoine, France). |
| 2006-2008 |
Teaching - general chemistry, analytical chemistry and physical chemistry (100urs, Université Pierre et Marie Curie, France). |
| 2006 |
5 months study of the formation of complexes between nucleic bases and cations, Université Pierre et Marie Curie, France. |
| 2005 |
3 months proposition of a method to determine the presence of judas bitumen in archeologic objects using mass spectrometry in combination with gas phase chromatography, Institut National du Patrimoine (INP). |
| 2004 |
6 weeks study of prehistorical pigments Laboratoires de Recherche des Musées de France. |
| 2002 |
5 weeks of analysing of prehistorical pigments, Ecole Supérieure de Physique et de Chimie Industrielles de Paris (ESPCI). |
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| Research interest |
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During my stay in the UOCHB, I will study the catalytic effect of oxovanadium complexes on the reactivity of alcohols, using ESI/MS experiments. I will compare the results obtained in the gas phase with those previously obtained in the liquid phase. The aim of this study is to put on light the reaction pathways involving during these reactions.
I will also study the gas phase reactivity of some species of interstellar interest, and more precisely the reactivity of dications formed by electric ionisation from aromatic molecules. Such reactions could take place in the ionosphere of Titan, and the mass spectra obtained during this study will be compared to those taken by the Cassini-Huygens probe. The aim of this study is to propose a kinetic model for the reactions of formations of different ions from methane.
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