4.8 Article

Ultrafast isomerization initiated by X-ray core ionization

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NATURE COMMUNICATIONS
卷 6, 期 -, 页码 -

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NATURE PUBLISHING GROUP
DOI: 10.1038/ncomms9199

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资金

  1. US Department of Energy Office of Science by Stanford University
  2. National Science Foundation [PHY-0649578]
  3. US Department of Energy, Office of Science, Basic Energy Sciences
  4. STFC
  5. EPSRC UK programme
  6. ERC ASTEX
  7. Max Planck Society
  8. Helmholtz Gemeinschaft through the Young Investigator Program
  9. LCLS, a DOE Office of Science User Facility
  10. Atomic and Molecular Optical Scisnces program within the Chemical Sciences, Geosciences, and Biosciences Division of the Office of Basic Energy Sciences, Office of Science, US Department of Energy
  11. Chemical Sciences, Geosciences, and Biosciences Division, Office of Basic Energy Sciences, Office of Science, US Department of Energy
  12. EPSRC [EP/I032517/1] Funding Source: UKRI
  13. Engineering and Physical Sciences Research Council [1227506, EP/I032517/1] Funding Source: researchfish
  14. Direct For Mathematical & Physical Scien
  15. Division Of Physics [0969322] Funding Source: National Science Foundation

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Rapid proton migration is a key process in hydrocarbon photochemistry. Charge migration and subsequent proton motion can mitigate radiation damage when heavier atoms absorb X-rays. If rapid enough, this can improve the fidelity of diffract-before-destroy measurements of biomolecular structure at X-ray-free electron lasers. Here we study X-ray-initiated isomerization of acetylene, a model for proton dynamics in hydrocarbons. Our time-resolved measurements capture the transient motion of protons following X-ray ionization of carbon K-shell electrons. We Coulomb-explode the molecule with a second precisely delayed X-ray pulse and then record all the fragment momenta. These snapshots at different delays are combined into a 'molecular movie' of the evolving molecule, which shows substantial proton redistribution within the first 12 fs. We conclude that significant proton motion occurs on a timescale comparable to the Auger relaxation that refills the K-shell vacancy.

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