G. Berden et al., HIGH-RESOLUTION UV SPECTROSCOPY OF PHENOL AND THE HYDROGEN-BONDED PHENOL-WATER CLUSTER, The Journal of chemical physics, 104(3), 1996, pp. 972-982
The S-1<--S0O00 transitions of phenol and the hydrogen bonded phenol(H
2O)(1) cluster have been studied by high resolution fluorescence excit
ation spectroscopy. All lines in the monomer spectrum are split by 56/-4 MHz due to the internal rotation of the -OH group about the a axis
. The barrier for this internal motion is determined in the ground and
excited states; V-2 '' = 1215 cm(-1), and V-2' = 710 cm(-1). The rota
tional constants for the monomer in the ground state are in agreement
with those reported in microwave studies. The excited state rotational
constants were found to be A' = 5313.7 MHz, B' = 2620.5 MHz an C' = 1
756.08 MHz. The region of the redshifted 0(0)(0) transition of phenol(
H2O)(1) shows two distinct bands which are 0.85 cm(-1) apart. Their sp
litting arises from a torsional motion which interchanges the two equi
valent H atoms in the (HO)-O-2 moiety of the cluster. This assignment
was confirmed by spin statistical considerations. Both bands could be
fit to rigid rotor Hamiltonians. Due to the interaction between the ov
erall rotation of the entire cluster and the internal rotation, both b
ands have different rotational constants. They show that V-2'< V-2 '',
and that the internal rotation axis is nearly parallel to the a-axis
of the cluster. If it is assumed that the structure of the rotor part
does not change upon electronic excitation, the internal motion become
s simply a rotation of the water around it symmetry axis. Assuming thi
s motion, barriers of 180 and 130 cm(-1) could be estimated for the S-
0 and S-1 states, respectively. The analysis of the rotational constan
ts of the cluster yielded an O-O distance of the hydrogen bond of 2.93
Angstrom in the ground state and 2.89 Angstrom in the electronically
excited state. In the equilibrium structure of the cluster, the plane
containing phenol bisects the plane of the water molecule. (C) 1996 Am
erican Institute of Physics.