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Detecting electron neutrinos from solar dark matter annihilation by JUNO · Around

2015

Detecting electron neutrinos from solar dark matter annihilation by JUNO

Guo, Wan-Lei

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We explore the electron neutrino signals from light dark matter (DM) annihilation in the Sun for the large liquid scintillator detector JUNO.

In terms of the spectrum features of three typical DM annihilation channels $\chi \chi \rightarrow \nu \bar{\nu},\tau^+ \tau^-, b \bar{b}$, we take two sets of selection conditions to calculate the expected signals and atmospheric neutrino backgrounds based on the Monte Carlo simulation data.
Then the JUNO sensitivities to the spin independent DM-nucleon and spin dependent DM-proton cross sections are presented.
It is found that the JUNO projected sensitivities are much better than the current spin dependent direct detection experimental limits for the $\nu \bar{\nu}$ and $\tau^+ \tau^-$ channels.

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