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COLLISION-INDUCED DISSOCIATION OF COMPLEXES CARBONACEOUS MOLECULAR SYSTEMS OF ASTROPHYSICAL INTEREST

NANOSCIENCE

 

LCAR
Lab: LCAR

Duration: NanoX master Internship (8 months part-time in-lab immersion

Latest starting date: 15/10/2025

Localisation: Laboratoire Collisions Agrégats Réactivité
University of Toulouse - Bat. 3R4 - 118 route de Narbonne - 31062 Toulouse Cedex 09 - France

Supervisors:
Alexandre MARCINIAK alexandre.marciniak@irsamc.ups-tlse.fr
Sébastien ZAMITH sebastien.zamith@irsamc.ups-tlse.fr

This research master's degree project could be followed by a PhD

Work package:
Cosmic nanograins play key roles in the physical and chemical evolution of the interstellar medium. Indeed, these nanosized catalytic platforms can interact with molecules of the gas phase (e.g. H2O, CO, etc.), through adsorption and desorption processes, which can result in the production of new species that chemically enrich star and planet forming regions. We are especially interested in carbonaceous nanograins made of polycyclic aromatic hydrocarbon (PAH) molecules and their derivatives [1]. In presence of water and UV photons, PAHs are expected to be oxidized, thus forming alcohol or ketone molecules [2,3] which are of prebiotic interest. During two previous beamtimes, the first at the SOLEIL synchrotron and the second at the ILM laboratory, we have studied PAH-water cationic complexes with different experimental setups in order to explore their dissociation properties (fragmentation channels, energetics and dynamics). These setups were equipped with an ion trap capable of performing collision induced dissociation (CID) at controlled collision energy that allows to measure the fragmentation channels of a parent species as a function of the internal energy injected into it. In particular, we could study CID of the pyrene-water cationic complex ([(C16H10):OH2]+) and its dehydrogenated form ([(C16H9)OH2]+) and the 1-hydroxypyrene cation ([C16H9OH]+) and its hydrogenated form ([HC16H9OH]+). Despite their similar compositions and structures, the raw CID data of these molecular systems are very different and show fragmentation pathways which are specific to each species. The aim of this internship will be to analyze the CID data obtained during the two beamtimes in order to shed light on the fragmentation pathways of these complex systems and to better interpret the observed differences. Depending on the student involvement and interest, she/he will also perform threshold CID measurements [4,5] with the experimental setup in LCAR [6] and/or he/she will also build a statistical model that will help to extract dissociation energies and rates.

References:
[1] Pilleri, P. et al. A&A 542, A69 (2012). [2] Bernstein, M. P. et al. Science 283, 1135-1138 (1999). [3] Bouwman, J. et al. A&A 511, A33 (2010). [4] Zamith, S. et al. J. Chem. Phys. 153, 054311 (2020). [5] Nair, A. M. et al. Phys. Chem. Chem. Phys. 26, 5947-5961 (2024). [6] Braud, I. et al. Rev. Sci. Instr. 88, 043102 (2017).

Areas of expertise:
molecular physics, collision, cluster physics, mass spectrometry, astrochemistry,

Required skills for the internship:
Good educational background in physics (quantum physics, molecular physics, electromagnetism, electronics) and strong interest and skills in experimental physics and data analysis. Knowledge in (astro-)chemistry are a not mandatory but will be appreciated.