Dark matter self-interactions from a general spin-0 mediator
F Kahlhoefer, K Schmidt-Hoberg… - Journal of Cosmology …, 2017 - iopscience.iop.org
Dark matter particles interacting via the exchange of very light spin-0 mediators can have
large self-interaction rates and obtain their relic abundance from thermal freeze-out. At the …
large self-interaction rates and obtain their relic abundance from thermal freeze-out. At the …
Point sources from dissipative dark matter
If a component of dark matter has dissipative interactions, it can cool to form compact
astrophysical objects with higher density than that of conventional cold dark matter (sub) …
astrophysical objects with higher density than that of conventional cold dark matter (sub) …
Estimating the flux of the 14.4 keV solar axions
FT Avignone III, RJ Creswick… - … of Cosmology and …, 2018 - iopscience.iop.org
In this paper we present a calculation of the expected flux of the mono-energetic 14.4 keV
solar axions emitted by the M1 type nuclear transition of 57 Fe in the Sun. These axions can …
solar axions emitted by the M1 type nuclear transition of 57 Fe in the Sun. These axions can …