15min:
DIRECT INFRARED ABSORPTION SPECTRA OF HELIUM CLUSTERS SEEDED WITH AN OCS MOLECULE.

JIAN TANG AND A. R. W. MCKELLAR, Steacie Institute for Molecular Sciences, National Research Council of Canada, Ottawa, Ontario K1A 0R6, Canada.

We have obtained rotationally-resolved IR spectra of van der Waals clusters composed of one OCS molecule and many helium atoms ( n = 1 to about 20). The observations are made in the region of the nu1 fundamental band of OCS, near 2062 cm-1, using a rapid-scan infrared diode laser spectrometer to probe a pulsed pinhole or slit supersonic jet expansion from a cooled (T = 230 to 280 K) nozzle with fairly high backing pressures (P = 6 to 30 atmospheres). For OCS-He n clusters with n \leq 8, the spectra have been assigned and confirmed by microwave observations [1]. For larger clusters, something changes: perhaps the effective onset of superfluid-type behavior. The spectra are still quite strong but not yet assigned in detail. As a function of n , the O-C vibrational frequency first shifts to the blue, as we already knew from the binary complex, OCS-He [2]. Once the first `solvation ring' of about 5 He atoms around the OCS becomes filled, the vibrational frequency starts to turn around and shift to the red, in accord with observations on larger helium nanodroplets (with n ~ 10,000).

\vskip 0.3 truecm \centerline References \parindent=0pt

[1] Y. Xu and W. Jäger, private communication (2001).

[2] J. Tang and A.R.W. McKellar, J. Chem. Phys. \textbf115, 3053 (2001).