http://arxiv.org/abs/2203.06200
We present an overview of future observational facilities that will significantly enhance our understanding of the fundamental nature of dark matter. These facilities span a range of observational techniques including optical/near-infrared imaging and spectroscopy, measurements of the cosmic microwave background, pulsar timing, 21-cm observations of neutral hydrogen at high redshift, and the measurement of gravitational waves. Such facilities are a critical component of a multi-pronged experimental program to uncover the nature of dark matter, while often providing complementary measurements of dark energy, neutrino physics, and inflation.
S. Chakrabarti, A. Drlica-Wagner, T. Li, et. al.
Tue, 15 Mar 22
66/108
Comments: Contribution to Snowmass 2021. 31 pages, 6 figures, 2 tables
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