4.6 Article

Ultrafast Photodissociation Dynamics of Nitromethane

Journal

JOURNAL OF PHYSICAL CHEMISTRY A
Volume 120, Issue 4, Pages 519-526

Publisher

AMER CHEMICAL SOC
DOI: 10.1021/acs.jpca.5b09776

Keywords

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Funding

  1. Los Alamos National Laboratory (LANL) Directed Research and Development funds (LDRD)
  2. Richard P. Feynman Fellowship in Theory and Computing
  3. National Nuclear Security Administration of the U.S. Department of Energy [DE-AC52-06NA25396]
  4. Center for Nonlinear Studies (CNLS), a U.S. Department of Energy
  5. Center for Integrated Nanotechnology (CINT), a U.S. Department of Energy
  6. Office of Basic Energy Sciences user facility

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Nitromethane (NM), a high explosive (HE) with low sensitivity, is known to undergo photolysis upon ultraviolet (UV) irradiation. The optical transparency, homogeneity, and extensive study of NM make it an ideal system for studying photodissociation mechanisms in conventional HE materials. The photochemical processes involved in the decomposition of NM could Be applied to the future design of controllable photoactive HE materials. In this study, the photodecomposition of NM from the n pi* state excited at 266 nm is being investigated on the femtosecond time scale. UV femtosecond transient absorption (TA) spectroscopy and excited state femtosecond stimulated Raman spectroscopy (FSRS) are combined with nonadiabatic excited state molecular dynamics (NA-ESMD) simulations to provide a unified picture of NM photodecomposition. The FSRS spectrum of the photoproduct exhibits peaks in the NO2 region and slightly shifted C-N vibrational peaks pointing to methyl nitrite formation as the dominant photoproduct. A total photolysis quantum yield of 0.27 and an n pi* state lifetime of similar to 20 fs were predicted from NA-ESMD simulations. Predicted time scales revealed that No-2 dissociation occurs in 81 +/- 4 fs and methyl nitrite formation is much slower having a time scale of 452 +/- 9 fs corresponding to the excited state absorption feature with a decay of 480 +/- 17 fs observed in the TA spectrum. Although simulations predict C-N bond cleavage as the primary photochemical process, the relative time scales are consistent with isomerization occurring via NO2 dissociation and subsequent rebinding of the methyl radical and nitrogen dioxide.

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