title: Imaging and scattering studies of the unimolecular dissociation of the BrCH2CH2O radical from BrCH2CH2ONO photolysis at 351 nm.
abstract: We report a study of the unimolecular dissociation of BrCH2CH2O radicals produced from the photodissociation of BrCH2CH2ONO at 351/355 nm. Using both a crossed laser-molecular beam scattering apparatus with electron bombardment detection and a velocity map imaging apparatus with tunable VUV photoionization detection, we investigate the initial photodissociation channels of the BrCH2CH2ONO precursor and the subsequent dissociation of the vibrationally excited BrCH2CH2O radicals. The only photodissociation channel of the precursor we detected upon photodissociation at 351 nm was O-NO bond fission. C-Br photofission and HBr photoelimination do not compete significantly with O-NO photofission at this excitation wavelength. The measured O-NO photofission recoil kinetic energy distribution peaks near 14 kcal/mol and extends from 5 to 24 kcal/mol. There is also a small signal from lower kinetic energy NO product (it would be 6% of the total if it were also from O-NO photofission). We use the O-NO photofission P(ET) peaking near 14 kcal/mol to help characterize the internal energy distribution in the nascent ground electronic state BrCH2CH2O radicals. At 351 nm, some but not all of the BrCH2CH2O radicals are formed with enough internal energy to unimolecularly dissociate to CH2Br + H2CO. Although the signal at m/e = 93 (CH2Br(+)) obtained with electron bombardment detection includes signal both from the CH2Br product and from dissociative ionization of the energetically stable BrCH2CH2O radicals, we were able to isolate the signal from CH2Br product alone using tunable VUV photoionization detection at 8.78 eV. We also sought to investigate the source of vinoxy radicals detected in spectroscopic experiments by Miller and co-workers ( J. Phys. Chem. A 2012 , 116 , 12032 ) from the photodissociation of BrCH2CH2ONO at 351 nm. Using velocity map imaging and photodissociating the precursor at 355 nm, we detected a tiny signal at m/e = 43 and a larger signal at m/e = 15 that we tentatively assign to vinoxy. An underlying signal in the time-of-flight spectra at m/e = 29 and m/e = 42, the two strongest peaks in the literature electron bombardment mass spectrum of vinoxy, is also apparent. Comparison of those signal strengths with the signal at HBr(+), however, shows that the vinoxy product does not have HBr as a cofragment, so the prior suggestion by Miller and co-workers that the vinoxy might result from a roaming mechanism is contraindicated.
authors.affiliation: The James Franck Institute and Department of Chemistry, The University of Chicago , Chicago, Illinois 60637 United States and.
authors.forename: Lei
authors.initials: L
authors.lastname: Wang
authors.forename: Chow-Shing
authors.initials: CS
authors.lastname: Lam
authors.forename: Rabi
authors.initials: R
authors.lastname: Chhantyal-Pun
authors.forename: Matthew D
authors.initials: MD
authors.lastname: Brynteson
authors.forename: Laurie J
authors.initials: LJ
authors.lastname: Butler
authors.forename: Terry A
authors.initials: TA
authors.lastname: Miller