15min:
PHOTODISSOCIATION SPECTROSCOPY AND DISSOCIATION DYNAMICS OF TiO+(CO2).

MANORI PERER, Department of Chemistry, University of Massachusetts Amherstb, Amherst, MA.

TiO+(CO2) is produced by reaction of laser-ablated titianium atoms with CO2 and subsequent clustering, supersonically cooled and its electronic spectroscopy characterized by photofragment spectroscopy, monitoring loss of CO2. The photodissociation spectrum consists of a vibrationally-resolved band in the visible, with extensive progressions in the covalent Ti-O stretch (952 cm-1 vibrational frequency and 5 cm-1 anharmonicity), and in the TiO+-(CO2) stretch (186 cm-1) and rock (45 cm-1). The band origin is at 13918 cm-1, assigned using titanium isotope shifts, and the spectrum extends to 17350 cm-1. The excited state lifetime decreases dramatically with increasing internal energy, from 1100 ns for the lowest energy band (vTiO=0), to <50 ns for vTiO=3. The long photodissociation lifetime substantially reduces the photodissociation quantum yield at low energy, likely due to competition with fluorescence. Electronic structure calculations help to assign the spectrum of TiO+(CO2) and predict allowed electronic transitions of TiO+ in the visible, which have not been previously measured. Time-dependent density functional calculations predict that the observed transition is due to B, 2 Pi leftarrow X, 2 Delta in the TiO+ chromophore, and that binding to CO2 red shifts the TiO+ transition by 1508 cm-1, and lowers the Ti-O stretch frequency by 16 cm-1. Combining the computational and experimental results, the 2 Pi state of TiO+ is predicted to lie at T0=15426 cm-1, with frequency omegae = 968 cm-1 and anharmonicity omegaexe = 5 cm-1. The calculations also predict that there is only one low-lying 2 Sigma state of TiO+, contrary to conclusions derived from photoelectron spectroscopy of TiO. Prospects for astronomical observation of TiO+ via the 2 Pi-2 Delta transition are also discussed.