We examine the initial
differential sticking probability of CH
4
and CD
4
on CH
4
and CD
4
ices
under nonequilibrium flow conditions using a combination of experimental
methods and numerical simulations. The experimental methods include
time-resolved
in situ
reflection–absorption
infrared spectroscopy (RAIRS) for monitoring on-surface gaseous condensation
and complementary King and Wells mass spectrometry techniques for
monitoring sticking probabilities that provide confirmatory results
via a second independent measurement method. Seeded supersonic beams
are employed so that the entrained CH
4
and CD
4
have the same incident velocity but different kinetic energies and
momenta. We found that as the incident velocity of CH
4
and
CD
4
increases, the sticking probabilities for both molecules
on a CH
4
condensed film decrease systematically, but that
preferential sticking and condensation occur for CD
4
. These observations differ when condensed
CD
4
is used as the target interface, indicating that the
film’s phonon and rovibrational densities of states, and collisional
energy transfer cross sections, have a role in differential energy
accommodation between isotopically substituted incident species. Lastly,
we employed a mixed incident supersonic beam composed of both CH
4
and CD
4
in a 3:1 ratio and measured the condensate
composition as well as the sticking probability. When doing so, we
see the same effect in the condensed mixed film, supporting an isotopic
enrichment of the heavier isotope. We propose that enhanced multi-phonon
interactions and inelastic cross sections between the incident CD
4
projectile and the CH
4
film allow for more efficacious
gas–surface energy transfer. VENUS code MD simulations show
the same sticking probability differences between isotopologues as
observed in the gas–surface scattering experiments. Ongoing
analyses of these trajectories will provide additional insights into
energy and momentum transfer between the incident species and the
interface. These results offer a new route for isotope enrichment
via preferential condensation of heavier isotopes and isotopologues
during gas–surface collisions under specifically selected substrate,
gas-mixture, and incident velocity conditions. They also yield valuable
insights into gaseous condensation under non-equilibrium conditions
such as occur in aircraft flight in low-temperature environments.
Moreover, these results can help to explain the increased abundance
of deuterium in solar system planets and can be incorporated into
astrophysical models of interstellar icy dust grain surface processes.