A computationally
affordable methodology is developed to predict
cross sections and rate coefficients for collisional quenching and
excitation of large molecules in space, such as PAHs. Mixed quantum/classical
theory of inelastic scattering (MQCT) is applied, in which quantum
state-to-state transitions between the internal states of the molecule
are described using a time-dependent Schrodinger equation, while the
scattering of collision partners is described classically using mean-field
trajectories. To boost the numerical performance even further, a decoupling
scheme for the equations of motion and a Monte Carlo sampling of the
initial conditions are implemented. The method is applied to compute
cross sections for rotational excitation and quenching of a benzene
molecule (C6H6) by collisions with He atoms
in a broad range of energies, using a very large basis set of rotational
eigenstates up to j = 60, and close to one million
nonzero matrix elements for state-to-state transitions. The properties
of collision cross sections for C6H6 + He are
reported and discussed. The accuracy of the approximations is rigorously
tested and is found to be suitable for astrophysical/astrochemical
simulations. The method and code developed here can be employed to
generate a database of collisional quenching rate coefficients for
PAHs and other large molecules, such as iCOMs, or for molecule–molecule
collisions in cometary comas.