Indico has been upgraded. It is back in production.

11–15 Jun 2018
Geological Museum, University of Copenhagen
Europe/Copenhagen timezone

VUV photoprocessing of large PAH cations: an experimental study

12 Jun 2018, 14:00
15m
Main Auditorium (Geological Museum, University of Copenhagen)

Main Auditorium

Geological Museum, University of Copenhagen

Øster Voldgade 5 - 7, 1350 København K, Denmark
Board: 104
Poster The creation and evolution of dust Poster Presentations

Speaker

Ms Gabi Wenzel (IRAP, Université de Toulouse, CNRS, CNES, Toulouse, France)

Description

As a part of interstellar dust, polycyclic aromatic hydrocarbons (PAHs) are processed by the interaction with vacuum ultraviolet (VUV) photons that are emitted by young stars [1]. After absorption of a VUV photon, an isolated PAH can undergo different relaxation processes: ionization, dissociation and radiative cooling, including infrared (IR) fluorescence which results in the aromatic infrared bands (AIBs) observed in many astronomical objects [2].
Following an earlier work on smaller PAHs [3], we investigate in this experimental study the two relaxation processes of photofragmentation and photoionization of large PAH cations ranging in size from 30 to 48 carbon atoms. The ions are trapped in the LTQ linear ion trap of the DESIRS beamline at the synchrotron SOLEIL and energized by VUV photons in the range of 8 - 20 eV. All resulting photoproducts are mass-analyzed and recorded as a function of photon energy. The photoionization process is found to strongly dominate the competition, with the photoionization yield increasing with number of carbon atoms. From the relative intensities of the photoproducts, action spectra are obtained and compared to the photoabsorption cross sections. The latter have been computed using the real time, real space implementation of time dependent density functional theory (TD-DFT) from the Octopus code [4]. This study gives insights into the photostability of interstellar PAHs in astrophysical environments.

References

[1] J. Montillaud, C. Joblin, and D. Toublanc, A&A, 552, A15 (2013)
[2] C. Joblin & A. G. G. M. Tielens, PAHs and the Universe, EAS Publication Series, Vol. 46 (2011)
[3] J. Zhen, S. Rodriguez Castillo, C. Joblin, G. Mulas, H. Sabbah, A. Giuliani, L. Nahon, S. Martin, J. Champeaux, and P. M. Mayer, ApJ, 822, 2 (2016)
[4] G. Malloci, G. Mulas, and C. Joblin, A&A, 426, 105 (2004)

Acknowledgements: We are grateful to the general staff from SOLEIL for the smooth running of the facility. We acknowledge funding by the European Union (EU) under the Horizon 2020 framework for the Marie Skłodowska-Curie action EUROPAH, Grant Agreement no. 722346. We also acknowledge support from the European Research Council under the European Union's Seventh Framework Programme ERC-2013-SyG, Grant Agreement no. 610256 NANOCOSMOS.

Consider for a poster? Yes

Primary author

Ms Gabi Wenzel (IRAP, Université de Toulouse, CNRS, CNES, Toulouse, France)

Co-authors

Dr Ming-Chao Ji (IRAP, Université de Toulouse, CNRS, CNES, Toulouse, France) Ms Sarah Rodriguez Castillo (IRAP, LCPQ/IRSAMC, Université de Toulouse, CNRS, CNES, Toulouse, France) Dr Giacomo Mulas (Istituto Nazionale di Astrofisica - Osservatorio Astronomico di Cagliari, Selargius (CA), Italy) Dr Hassan Sabbah (IRAP, LCAR/IRSAMC, Université de Toulouse, CNRS, CNES, Toulouse, France) Dr Alexandre Giuliani (Synchrotron SOLEIL, L'Orme des Merisiers, Saint Aubin, Gif-sur-Yvette, France) Dr Laurent Nahon (Synchrotron SOLEIL, L'Orme des Merisiers, Saint Aubin, Gif-sur-Yvette, France) Dr Christine Joblin (IRAP, Université de Toulouse, CNRS, CNES, Toulouse, France)

Presentation materials