Spectroscopic techniques are used to investigate energy transfer
and radiation-induced reactions on the surfaces
of particulate silicas. Upon subjection to high energy radiation,
hydrogen atoms are produced with significant
yields in all silica samples pretreated at 150 °C, for an example,
G(H) = 4.2 in silica gel Davisil 60.
Subsequent
hydrogen addition to aromatic adsorbates such as pyrene,
N,N-dimethylaniline, and methyl viologen
(MV2+)
proceeds on the surface in competition with the hydrogen dimerization,
leading to the formation of their H
adducts. Hydrogen scavenging studies revealed that such addition
reactions are heterogeneous in porous
silica gel with contributions from a fast intrapore reaction within
several nanoseconds and a much slower
diffusion influenced interpore process over many microseconds. The
efficient capture of H atoms by pyrene
at a small percentage of surface coverage suggests that hydrogen is
produced at the specific sites where
pyrene adsorbs. Electron scavenging by CHCl3,
Cd2+, and MV2+ leads to a suppression of H
addition and
an enhanced positive charge transfer to pyrene. Pretreatment of
silica samples at 600 °C gives rise to increased
ionic products of aromatic adsorbates, concomitant with decreased
hydrogen production. These experimental
observations are understood in terms of an exciton model. By
comparison with the electronic processes in
bulk silica materials, it is shown that surface plays a major role in
the relaxation of excitation and the activation
of adsorbate chemistry.