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Astrophysical implications of the fermionic dark matter in galaxies

2017
The main aim of this thesis is to use a fermionic dark matter (DM) model (the Ruffini-Arg\"uelles-Rueda (RAR) model) to describe the distribution of dark matter in galactic halos as an astrophysical probe of the fermionic nature of dark matter. My thesis work focuses then on testing possible effects that are caused by DM (and modeled by the RAR model ...
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The astrophysics of galaxy groups and Clusters with Athena+

2013
Ettori, S.   +30 more
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