María Benito Castaño
In this talk, current shortcomings in our understanding of how dark matter is distributed in our Galaxy will be reviewed. In addition, we will cover ongoing strategies for using the Milky Way as a laboratory to investigate the underlying particle physics model that governs DM on microscopic scales.
Seminar toimub Tartu observatooriumis Tõraveres ja on jälgitav Zoomis.