XUV excitation followed by ultrafast non-adiabatic relaxation in PAH molecules as a femto-astrochemistry experiment

  • A. Marciniak
  • , V. Despré
  • , T. Barillot
  • , A. Rouzée
  • , M. C.E. Galbraith
  • , J. Klei
  • , C. H. Yang
  • , C. T.L. Smeenk
  • , V. Loriot
  • , S. Nagaprasad Reddy
  • , A. G.G.M. Tielens
  • , S. Mahapatra
  • , A. I. Kuleff
  • , M. J.J. Vrakking
  • , F. Lépine

Research output: Contribution to journalArticlepeer-review

77 Scopus citations

Abstract

Highly excited molecular species are at play in the chemistry of interstellar media and are involved in the creation of radiation damage in a biological tissue. Recently developed ultrashort extreme ultraviolet light sources offer the high excitation energies and ultrafast time-resolution required for probing the dynamics of highly excited molecular states on femtosecond (fs) (1 fs=10-15s) and even attosecond (as) (1 as=10-18s) timescales. Here we show that polycyclic aromatic hydrocarbons (PAHs) undergo ultrafast relaxation on a few tens of femtoseconds timescales, involving an interplay between the electronic and vibrational degrees of freedom. Our work reveals a general property of excited radical PAHs that can help to elucidate the assignment of diffuse interstellar absorption bands in astrochemistry, and provides a benchmark for the manner in which coupled electronic and nuclear dynamics determines reaction pathways in large molecules following extreme ultraviolet excitation.

Original languageEnglish
Article number7909
JournalNature Communications
Volume6
DOIs
StatePublished - 13 Aug 2015
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2015 Macmillan Publishers Limited. All rights reserved.

Funding

FundersFunder number
European Commission
Seventh Framework Programme284464, 246976

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