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Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal · Around

2018

Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal

Schneider, Aurel

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Any particle dark matter (DM) scenario featuring a suppressed power spectrum of astrophysical relevance results in a delay of galaxy formation.

As a consequence, such scenarios can be constrained using the global 21-cm absorption signal initiated by the UV radiation of the first stars.
The Experiment to Detect the Global Epoch of Reionization Signature (EDGES) recently reported the first detection of such an absorption signal at redshift $\sim 17$.
While its amplitude might indicate the need for new physics, we solely focus on the timing of the signal to test non-cold DM models.

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