Cross Section Calculations in Theories of Self-Interacting Dark Matter
arXiv:2206.14395 · doi:10.1103/PhysRevD.106.063013
Abstract
We study an asymmetric dark matter model with self-interacting dark matter consisting of a Dirac fermion coupled to a scalar or vector mediator, such that the reaction is well described by perturbation theory. We compute the scattering cross section , the transfer cross section , and the viscosity cross section for this reaction. As one part of our study, we give analytic and numerical comparisons of results obtained with the inclusion of both -channel and -channel exchanges and results obtained in an approximation that has often been used in the literature that includes only the -channel contribution. The velocity dependences of these cross sections are studied in detail and shown to be in accord with observational data.
15 pages, 10 figures
References in corpus (14)
- Ultralight scalars as cosmological dark matter
- A Theory of Dark Matter
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- Opening a new window for warm dark matter
- Resonant Dark Forces and Small Scale Structure
- Interacting Dark Sector and Precision Cosmology
- Supernova Bounds on the Dark Photon Using its Electromagnetic Decay
- Cosmic particle colliders: simulations of self-interacting dark matter with anisotropic scattering
- Searching in the dark: the hunt for the dark photon
- Dark matter halo shapes in the Auriga simulations
- The Semi-Classical Regime for Dark Matter Self-Interactions
- Constraints on Mirror Models of Dark Matter from Observable Neutron-Mirror Neutron Oscillation
- Neutrino Masses and Mixing in Models with Large Extra Dimensions and Localized Fermions