If we want to approach the problem of dark matter from a particle physics perspective, we need to make assumptions about the quantum numbers of the weakly interacting state which forms dark matter. During most of these lecture notes we assume that this new particle has a mass in the GeV to TeV range, and that its density is thermally produced during the cooling of the Universe. Moreover, we assume that the entire dark matter density of the Universe is due to one stable particle.
- 1.Plehn, T.: Lectures on LHC Physics. Lect. Notes Phys. 886 (2015). arXiv:0910.4182 [hep-ph]. http://www.thphys.uni-heidelberg.de/~plehn/?visible=review
- 3.Bramante, J., Desai, N., Fox, P., Martin, A., Ostdiek, B., Plehn, T.: Towards the final word on neutralino dark matter. Phys. Rev. D 93(6), 063525 (2016). arXiv:1510.03460 [hep-ph]
- 4.Bramante, J., Fox, P.J., Martin, A., Ostdiek, B., Plehn, T., Schell, T., Takeuchi, M.: Relic neutralino surface at a 100 TeV collider. Phys. Rev. D 91, 054015 (2015). arXiv:1412.4789 [hep-ph]