[SPECIAL TIME] Celine Boehm, Sydney [HET Seminar] Can we use caustic skeleton theory to decipher the nature of dark matter?
Small Seminar Room
One of the most robust pieces of evidence for dark matter comes from the formation and evolution of the intricate large-scale structure of the Universe.
By comparing the results of N-body (and hydro) simulations with observations, one can infer some important properties that the dark matter particles should have (mass, maximal scattering cross section etc). However there comes a point where we lack sufficient resolution to distinguish between different models. In this talk, I will show that analysing the topology of the large-scale-structure in the Universe could provide a wealth of information that has been so far inaccessible and may help discriminate between dark matter models.
https://bnl.zoomgov.com/j/1653048131?pwd=fkT0TgSQn5wqXX55rQa3jABDwMj8sE.1