We employ velocity map imaging (VMI) to investigate the photodissociation of manganese pentacarbonyl bromide (MnBr(CO)5)), both in the gas phase and on a surface. Pulsed 266 nm and/or 230 nm laser light was used to initiate the photodissociation cleaving the Mn–CO bonds. A single 230 or 266 nm photon has enough energy to lead to the dissociation of all five Mn–CO bonds. The CO is ionized using a (2+1) resonance-enhanced multiphoton ionization (REMPI) scheme via the B1Σ+–X1Σ+ transition with ∼230 nm photons. To deconvolute the contributions from the gas-phase and surface photodissociation, one- and two-color experiments are compared. In the one-color experiment, a focused 230 nm light above the sample surface was used to dissociate gas-phase MnBr(CO)5 and to ionize CO via REMPI. The two-color experiments use grazing angle illumination with a 266 nm laser beam to induce the dissociation of MnBr(CO)5 on the sample surface and probe with a focused 230 nm laser beam above the sample surface to ionize the product CO at a specific time delay. The CO from the one-color gas-phase photodissociation is seen as a background to the surface dissociation CO signal and was subtracted from both the VMI images and Q-branch REMPI spectra of CO. In the two-color time-resolved detection of CO above the surface after photodissociation at the surface, we observe a complex arrival time distribution. To explain this arrival time distribution, we hypothesize that there are four main pathways for the formation of CO: (1) hyperthermal CO ejected directly into the gas phase from the surface as a result of 266 nm photodissociation, (2) thermalized CO coming from the photodissociation of MnBr(CO)5 that resides on the surface for sufficient time to come into thermal equilibrium with the surface before desorption, (3) CO from photodissociation of intact MnBr(CO)5 ejected from the surface and dissociated by the 230 nm laser beam, and (4) CO from the gas-phase photodissociation of MnBr(CO)5 with 266 nm laser light near the surface. Q-branch REMPI spectra of CO and VMI images were collected at various time delays and are consistent with our hypothesis.
扫码关注我们
求助内容:
应助结果提醒方式:
