Dark matter self-interactions via collisionless shocks in cluster mergers
Matti Heikinheimo (National Institute of Chemical Physics and Biophysics, Rävala 10, Tallinn, 10143, Estonia); Martti Raidal (Institute of Physics, University of Tartu, Estonia, National Institute of Chemical Physics and Biophysics, Rävala 10, Tallinn, 10143, Estonia); Christian Spethmann (National Institute of Chemical Physics and Biophysics, Rävala 10, Tallinn, 10143, Estonia); Hardi Veermäe (Institute of Physics, University of Tartu, Estonia, National Institute of Chemical Physics and Biophysics, Rävala 10, Tallinn, 10143, Estonia)
While dark matter self-interactions may solve several problems with structure formation, so far only the effects of two-body scatterings of dark matter particles have been considered. We show that, if a subdominant component of dark matter is charged under an unbroken U(1) gauge group, collective dark plasma effects need to be taken into account to understand its dynamics. Plasma instabilities can lead to collisionless dark matter shocks in galaxy cluster mergers which might have been already observed in the Abell 3827 and 520 clusters. As a concrete model we propose a thermally produced dark pair plasma of vector-like fermions. In this scenario the interacting dark matter component is expected to be separated from the stars and the non-interacting dark matter halos in cluster collisions. In addition, the missing satellite problem is softened, while constraints from all other astrophysical and cosmological observations are avoided.
