Time-resolved X-ray Absorption Spectroscopy of aromatic Carbonyls using Spectral Domain Ghost Imaging

ORAL

Abstract

We studied UV-induced ultrafast photochemistry of aromatic carbonyls using time-resolved soft X-ray absorption spectroscopy. By utilizing the specific sensitivity of near edge X-ray absorption fine structure spectroscopy (NEXAFS) to the electronic character of the excited states (e.g., ππ* and nπ* states) we were able to elucidate the initial steps in the photodissociation mechanisms of Norrish Type-I reactions involving internal conversion and a subsequent interplay between the singlet and triplet states in one of the smallest aromatic carbonyls, Acetophenone (C6H5COCH3). We excited the gas phase sample with a 266 nm pump pulse and probed the reaction by scanning the X-ray photo energy across around the O K-edge (~520 to 540 eV). We monitored the X-ray absorbance through the measure of Auger-Meitner electron yield together with the photon spectrum. The experiment was carried out at the TMO instrument of the LCLS. The X-ray pulses generated by the free-electron laser (FEL) driven by self-amplified spontaneous emission (SASE) exhibit a strong shot to shot spectral jitter with a bandwidth of several eV. To overcome this spectral bandwidth limitation to resolve dynamics in the fine structure spectrum at an order of less than 1 eV we exploit the correlation present in the shot-to-shot fluctuations in the incoming X-ray pulses and the detected electron signal by employing spectral domain ghost imaging. Utilizing this technique we are able to resolve a pre-edge absorption feature, around 527 eV, which is attributed to the population of the nπ* state. The initial formation of this feature is observed with a rise time in the order of 100 fs. Subsequently a slow decay combined with spectral shift can be seen persisting for over 20ps, indicating dynamics to the triplet manifolds before dissociation. Our experimental results are corroborated by theoretical simulations.

*This work was supported by the AMOS program within the DOE Office of Science, Basic Energy Sciences, Chemical Sciences, Geosciences, and Biosciences Division. Use of the Linac Coherent Light Source (LCLS), SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515

Presenters

  • Martin Grassl

    • SLAC National Accelerator Laboratory

Authors

  • Martin Grassl

    • SLAC National Accelerator Laboratory
  • Yusong Liu

    • SLAC National Laboratory
  • Alice Green

    • Stanford PULSE Institute
    • SLAC National Accelerator Laboratory
  • Felix Allum

    • Stanford University
  • Kurtis D Borne

    • Kansas State University
  • Martin Centurion

    • University of Nebraska - Lincoln
  • xinxin Cheng

    • SLAC National Accelerator Laboratory
    • SLAC National Acccelerator Laboratory
  • Taran Driver

    • SLAC
  • Ruaridh Forbes

    • SLAC National Accelerator Laboratory
  • James M Glownia

    • SLAC - Natl Accelerator Lab
    • SLAC National Accelerator Laboratory
  • Erik Isele

    • Stanford University
  • Andrei Kamalov

    • SLAC National Accelerator Laboratory
  • Kirk Larsen

    • SLAC National Accelerator Laboratory
  • Xiang Li

    • SLAC - Natl Accelerator Lab
  • Ming-Fu Lin

    • SLAC - Natl Accelerator Lab
    • SLAC National Accelerator Laboratory
  • Razib Obaid

    • SLAC National Accelerator Laboratory
  • Adam Summers

    • SLAC National Accelerator Laboratory
    • Stanford University
    • Linac Coherent Light Source, SLAC National Accelerator Laboratory
    • SLAC, National Accelerator Laboratory
  • Jun Wang

    • Stanford University
  • Thomas Weinacht

    • Stony Brook University
  • James P Cryan

    • SLAC National Accelerator Laboratory
  • Thomas J Wolf

    • SLAC National Accelerator Laboratory
  • Todd J Martinez

    • Stanford Univ
  • Pablo A Unzueta

    • Stanford University
  • Dip Hait

    • Stanford University