Photodissociation dynamics of OCS at ∼210 nm: The role of c(2A″) state.

J Chem Phys

Hefei National Laboratory for Physical Sciences at the Microscale, Department of Chemical Physics, and Synergetic Innovation Center of Quantum Information and Quantum Physics, University of Science and Technology of China, Hefei, Anhui 230026, People's Republic of China.

Published: July 2017

AI Article Synopsis

  • The study uses a time-sliced ion velocity map imaging technique to explore how carbonyl sulfide (OCS) breaks apart when exposed to deep UV light around 210 nm.
  • Three distinct channels of kinetic energy release during the photodissociation process are identified, with a new high-energy channel emerging specifically at this wavelength.
  • The findings highlight the role of strong spin-orbit coupling in the dissociation dynamics, indicating that direct excitation to a triplet state significantly affects how OCS dissociates into sulfur and carbon monoxide.

Article Abstract

Photodissociation dynamics of carbonyl sulfide (OCS) in the deep ultraviolet region is investigated using a time-sliced ion velocity map imaging technique. The measured total kinetic energy release spectra from the photodissociation of OCS at ∼210 nm shows three dissociation channels to the fragment S(D), corresponding to low, medium, and high kinetic energy release (E), respectively. The high E channel is found to be a new dissociation channel opening with photolysis wavelength at ∼210 nm. Based on the a(p) polarization parameters as well as the anisotropy parameters β determined from the images of S(D), the dissociation of OCS to S(D) + CO at 210 nm is concluded to involve a direct vertical excitation of the triplet c(2A) state from the ground state, followed by processes as: the low E component arises from a non-adiabatic transition from the repulsive A(2A) state to the electronic ground state X(1A); the medium E component arises from a simultaneous excitation to two repulsive excited states; and the high E component arises from the intersystem crossing from the triplet c(2A) state to the repulsive A(2A) state. The present study shows that, due to the strong spin-orbit coupling between the triplet c(2A) state and the repulsive A(2A) state, a direct excitation to c(2A) significantly contributes to the photodissociation dynamics of OCS in the deep-UV region.

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http://dx.doi.org/10.1063/1.4982684DOI Listing

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