We investigate the possibility of reproducing the recently reported 3.55 keV line in some simple decaying dark matter scenarios. In all cases a keV scale decaying DM is coupled with a scalar field charged under SM gauge interactions and thus capable of pair production at the LHC. We will investigate how the demand of a DM lifetime compatible with the observed signal, combined with the requirement of the correct DM relic density through the freeze-in mechanism, impacts the prospects of observation at the LHC of the decays of the scalar field. © 2015 IOP Publishing Ltd and Sissa Medialab srl.

Arcadi, G., Covi, L., Dradi, F. (2015). 3.55 keV line in minimal decaying dark matter scenarios. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2015(7) [10.1088/1475-7516/2015/07/023].

3.55 keV line in minimal decaying dark matter scenarios

Arcadi, G.;
2015

Abstract

We investigate the possibility of reproducing the recently reported 3.55 keV line in some simple decaying dark matter scenarios. In all cases a keV scale decaying DM is coupled with a scalar field charged under SM gauge interactions and thus capable of pair production at the LHC. We will investigate how the demand of a DM lifetime compatible with the observed signal, combined with the requirement of the correct DM relic density through the freeze-in mechanism, impacts the prospects of observation at the LHC of the decays of the scalar field. © 2015 IOP Publishing Ltd and Sissa Medialab srl.
Arcadi, G., Covi, L., Dradi, F. (2015). 3.55 keV line in minimal decaying dark matter scenarios. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2015(7) [10.1088/1475-7516/2015/07/023].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/351211
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