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Gaia, Fundamental Physics, and Dark Matter
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The Gaia space astrometry mission is measuring accurate distances and space motions of more than two billion stars throughout our Galaxy and beyond. This is a first look at how Gaia is contributing to fundamental physics, and in particular to our understanding of dark matter, for which a few examples are given from the current literature. One of our goals is to illustrate how deep, and often surprising, insight into very diverse areas of fundamental physics can be extracted from this new and enormous high-accuracy stellar data set. In this spirit, we finish by suggesting a search for a connection between stellar activity, dark matter streams, and planetary configuration in nearby exoplanetary systems, as has been tentatively proposed in the case of the solar system.
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Optimisation of amplification and gas mixture for directional Dark Matter searches with the CYGNO/INITIUM project
For a He:CF4 optical TPC, an extra electrode below the last GEM doubles the light yield, and 1.6% SF6 enables negative-ion drift with diffusion as low as 45 µm/√cm.
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