High Energy / Nuclear Theory / RIKEN Seminars

[SPECIAL TIME] Celine Boehm, Sydney [HET Seminar] Can we use caustic skeleton theory to decipher the nature of dark matter?

→ US/Eastern
Small Seminar Room

Small Seminar Room

Description

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