Making the halo of Andromeda with the QCD Axion?

start date: 

Mardi, décembre 13, 2016 - 14:00

Place: 

483 A - Malevitch

Speaker: 

Sacha Davidson

Home Institute: 

IPN Lyon

organized by: 

The  QCD axion is a curious Dark Matter candidate, having a mass like the neutrino, but behaving as Cold Dark Matter during linear structure formation. I will review how this occurs, and  speculate on the interesting question  of how  axions make galactic halos during non-linear structure formation, and whether  observations could distinguish them from WIMPs.