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The nature of dark matter remains today poorly constrained,
with proposed candidates spanning 90 orders of magnitude in mass, ranging
from ultra-light bosons to massive primordial black holes. I will discuss
what we have learned about the nature of dark matter from past
experiments, and argue that a new era has begun for dark matter searches.
I highlight in particular the importance of diversifying the experimental
effort, and of exploiting the extraordinary opportunities offered by
upcoming astronomical surveys and gravitational wave interferometers.
Raffaella Schneider e Gianluca Cavoto