The infrared absorption spectrum of the weakly bound rare-gas-spherical-top
complex Ne-CH4 was discovered and analyzed for the first time. Measurement
s were made with tunable diode laser spectrometers using a pulsed supersoni
c jet and a long-path low-temperature absorption cell. Close to the R(0) tr
ansition of the methane v(4) fundamental band at 1311.430 cm(-1),the Ne-CH4
spectrum was recorded as a very compact absorption pattern. Within a total
wave-number range of about 0.1 cm(-1), P-, Q-, and R-branches are located.
As the first step, the Ne-CH4 spectrum was recorded and analyzed in a supe
rsonic jet at low rotational temperature of about 5 K. Three branches were
identified, of which the P- and R-branches were partially resolved and the
Q-branch remained unresolved. Compared with the previously measured spectra
of Ar-CH4 and Kr-CH4 [Z. Naturforsch. A, 53, 725 (1998).], the absorption
pattern in the spectrum of Ne-CH4 is much denser and considerably more comp
act. However, by analogy with the spectra of Ar-CH4 and Kr-CH4, assignment
and analysis were carried out using a Hamiltonian model that incorporates a
Coriolis interaction between the total angular momentum of the complex and
the angular momentum of the methane monomer. This analysis then allowed us
to assign the same spectrum as recorded in a long-path (160 m) cell at a h
igher temperature of 62 K. The observed rotational constant for Ne-CH4, B"
= 0.129(9) cm(-1), corresponds to an effective intermolecular separation of
3.8 Angstrom.