Rotational transitions from seven low-lying vibrational states of HCCN
and five low-lying vibrational states of DCCN have been detected in t
he frequency range from 100 to 400 GHz with (+/-1) a sensitive millime
ter-wave spectrometer. The CCH bending states nu(5)(+/-1), 2 nu(5)(+/-
2), and 3 nu(5)(+/-3), and the CCN bending state nu(4)(+/-1) have been
assigned. In addition, transitions from three vibrational states in H
CCN and one in DCCN with zero orbital angular momentum (l) were also d
etected. These states in all likelihood originate from the three lowes
t l=0 excited states, i.e., (nu(4)+nu(5)>(-0) (nu(4) + nu(5))(+0), and
2 nu(5)(0). Analysis of the high-accuracy millimeter-wave frequency d
ata establishes that HCCN is not a near-rigid bent molecule and intens
ity measurements confirm that the CCH bending states are much lower in
energy than in typical well-behaved linear molecules. The low barrier
to linearity in HCCN and DCCN of similar to 235 cm(-1), estimated fro
m intensity measurements and the ab initio calculations of Malmquist e
t al. [Theor. Chim. Acta 73, 155 (1988)], confirms that HCCN is quasil
inear. (C) 1995 American Institute of Physics.