We present the infrared (IR) absorption spectrum of the jet-cooled naphthal
ene-Ar van der Waals cluster cation in the 400-1600 cm(-1) range, which is
expected to resemble closely the IR spectrum of the bare naphthalene cation
. Cluster cations are produced in their ground states via resonance-enhance
d two-color ionization. Subsequent irradiation of the ions with IR light of
a free-electron laser causes cluster dissociation, if this light is resona
nt with IR-active transitions of the cationic cluster. Mass-selective measu
rement of the dissociated fraction as a function of IR wavelength yields th
e IR spectrum of the cationic duster. Comparison with previously reported A
r matrix isolation spectra of naphthalene(+) shows good agreement, with mor
e bands observed in the present study. The IR spectrum observed is compared
to a calculated spectrum of the naphthalene cation, allowing for unambiguo
us assignments of all the observed modes. The experimental method presented
is generally applicable to obtain laboratory IR spectra of ionized polyaro
matic hydrocarbons under astrophysically relevant conditions.