Solar $\gamma$-rays as a Complementary Probe of Dark Matter
Phys. Rev. D 96, 063010 (2017) We show that observations of solar $\gamma$-rays offer a novel probe of dark matter in scenarios where interactions with the visible sector proceed via a long-lived mediator. As a proof of principle, we demonstrate that there exists a class of models which yield solar...
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Main Authors | , , , |
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Format | Journal Article |
Language | English |
Published |
23.03.2017
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Subjects | |
Online Access | Get full text |
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Summary: | Phys. Rev. D 96, 063010 (2017) We show that observations of solar $\gamma$-rays offer a novel probe of dark
matter in scenarios where interactions with the visible sector proceed via a
long-lived mediator. As a proof of principle, we demonstrate that there exists
a class of models which yield solar $\gamma$-ray fluxes observable with the
next generation of $\gamma$-ray telescopes, while being allowed by a variety of
current experimental constraints. The parameter space allowed by big bang
nucleosynthesis and beam dump experiments naturally leads to mediator lifetimes
sufficient to produce observable solar $\gamma$-ray signals. The model allows
for solar $\gamma$-ray fluxes up to orders of magnitude larger compared to
dwarf spheroidal galaxies, without reaching equilibrium between dark matter
annihilation and capture rate. Our results suggest that solar $\gamma$-ray
observations are complementary, and in some cases superior, to existing and
future dark matter detection efforts. |
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Bibliography: | CP3-17-08, TTK-17-07 |
DOI: | 10.48550/arxiv.1703.08087 |