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The Search for Dark Matter · Around

2018

The Search for Dark Matter

Baudis, Laura

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Understand

The dark matter problem is almost a century old.

Since the 1930s evidence has been growing that our cosmos is dominated by a new form of non-baryonic matter, that holds galaxies and clusters together and influences cosmic structures up to the largest observed scales.
At the microscopic level, we still do not know the composition of this dark, or invisible matter, which does not interact directly with light.
The simplest assumption is that it is made of new particles that interact with gravity and at most weakly with known elementary particles.

Built on

Zwicky F 1933 Helv.Phys.Acta
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Read J 2014 J.Phys
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Peccei R and Quinn H R 1977 Phys.Rev.Lett
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Bosma A 1981 Astron.J
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Preskill J, Wise M B and Wilczek F 1983 Phys.Lett
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Sikivie P 1983 Phys.Rev.Lett
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2008
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Frenk C S and White S D M 2012 Annalen Phys
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Then

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Ade P A R et al
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Baudis L 2016 Annalen Phys
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Moniez M 2010 Gen. Rel. Grav
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