  Self-interacting Dark Matter (SIDM) models have the potential to solve the
small-scale problems that arise in the Cold Dark Matter paradigm. Simulations
are a powerful tool for studying SIDM in the context of astrophysics, but it is
numerically challenging to study differential cross-sections that favour
small-angle scattering (as in light-mediator models). Here we present a novel
approach to model frequent scattering based on an effective drag force, which
we have implemented into the N-body code Gadget-3. In a range of test problems
we demonstrate that our implementation accurately models frequent scattering.
Our implementation can be used to study differences between SIDM models that
predict rare and frequent scattering. We simulate core formation in isolated
dark matter haloes, as well as major mergers of galaxy clusters. We find that
SIDM models with rare and frequent interactions cannot be mapped onto one
another. In particular, frequent interactions are able to produce larger
offsets between the distribution of galaxies and dark matter in equal-mass
mergers.
