Search for neutrinos from annihilation of captured low-mass dark matter particles in the Sun by Super-Kamiokande
2015
Super-Kamiokande(SK) can search for
weakly interacting massive particles(
WIMPs) by detecting neutrinos produced from
WIMP
annihilationsoccurring inside the Sun. In this analysis, we include neutrino events with interaction vertices in the detector in addition to upward-going muons produced in the surrounding rock. Compared to the previous result, which used the upward-going muons only, the signal acceptances for light (few-GeV/$c^2$ $\sim$ 200-GeV/$c^2$)
WIMPsare significantly increased. We fit 3903 days of SK data to search for the contribution of neutrinos from
WIMP
annihilationin the Sun. We found no significant excess over expected atmospheric-neutrino background and the result is interpreted in terms of upper limits on
WIMP-nucleon elastic scattering cross sections under different assumptions about the
annihilationchannel. We set the current best limits on the spin-dependent (SD)
WIMP-proton cross section for
WIMPmasses below 200 GeV/$c^2$ (at 10 GeV/$c^2$, 1.49$\times 10^{-39}$ cm$^2$ for $\chi\chi\rightarrow b \bar{b}$ and 1.31$\times 10^{-40}$ cm$^2$ for $\chi\chi\rightarrow\tau^+\tau^-$
annihilationchannels), also ruling out some fraction of
WIMPcandidates with spin-independent (SI) coupling in the few-GeV/$c^2$ mass range.
Keywords:
-
Correction
-
Source
-
Cite
-
Save
0
References
51
Citations
NaN
KQI