Ultrafast structural dynamics in the photodissociation of iodobenzene captured with ultrafast electron diffraction and a genetic algorithm

ORAL

Abstract

We investigate the fragmentation dynamics of iodobenzene following UV-induced photodissociation using a kilo-electron-volt ultrafast electron diffraction setup. The dissociation of the iodine atom takes place on a sub-picosecond timescale via two distinct dissociation channels (fast and slow), which we have identified in the diffraction signal. We use a genetic algorithm to retrieve the structure of the phenyl ring after dissociation directly from the diffraction data, representing the ensemble-averaged geometry. The retrieved phenyl ring shows that the C2v symmetry is preserved. The correlations among retrieved internal coordinates indicate an in-plane vibrational mode, which is assigned to the ν10 (“squatting”) mode, as the dominant mode. Ab-initio calculations of the dissociation also indicate that the C2v symmetry is preserved and the same active molecular vibration is present in both dissociation channels. The agreement between calculation and experiment suggests a similar relaxation pathway of the fragment despite different initial excited states in both the fast and slow dissociation channels.

*The authors ackowledge support from the US Department of Energy, Office of Science, Basic Energy Sciences under award no. DE-SC0014170

Presenters

  • Cuong Le

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska-Lincoln

Authors

  • Cuong Le

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska-Lincoln
  • Mehmood Saad

    • Department of Physics, Kansas State University, Manhattan, Kansas 66506, USA
  • Yanwei Xiong

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • Haoran Zhao

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • Sri Bhavya Muvva

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • Sajib Kumar Saha

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • Lauren Heald

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • Jackson T Lederer

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln
  • T. Madhu Trivikram

    • Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • Loren Greenman

    • Kansas State University
    • Department of Physics, Kansas State University, Manhattan, Kansas 66506, USA
  • Daniel S Slaughter

    • Lawrence Berkeley National Laboratory
    • Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • Martin Centurion

    • Department of Physics and Astronomy, University of Nebraska-Lincoln, Lincoln, Nebraska 68588, USA
    • University of Nebraska - Lincoln