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Heavy concerns about the light axino explanation of the 3.5 keV X-ray line
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. Although still under scrutiny, decaying dark matter could be responsible for this signal. We investigate whether an axino with a mass of 7 keV could explain the line, keeping the discussion as model i...
Autores principales: | Colucci, Stefano, Dreiner, Herbi K., Staub, Florian, Ubaldi, Lorenzo |
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Lenguaje: | eng |
Publicado: |
2015
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2015.09.009 http://cds.cern.ch/record/2036914 |
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