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We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. We found no statistical excess of neutrinos and established 90% confidence level upper limits of $8.4 times 10^7$,cm$^{-2}$ ($3.0 times 10^{9}$,cm$^{-2}$) on electron anti-neutrino (electron neutrino) fluence at 20,MeV normalized to the X12 flare, assuming that the neutrino fluence is proportional to the X-ray intensity. The 90% C.L. upper limits from this work exclude the entire region of parameter space associated with the Homestake event excess for the large solar flare in 1991.
Neutrinos generated during solar flares remain elusive. However, after $50$ years of discussion and search, the potential knowledge unleashed by their discovery keeps the search crucial. Neutrinos associated with solar flares provide information on o
It has been speculated that quantum gravity might induce a foamy space-time structure at small scales, randomly perturbing the propagation phases of free-streaming particles (such as kaons, neutrons, or neutrinos). Particle interferometry might then
There are many theories where a dark matter particle is part of a multiplet with an electrically charged state. If WIMP dark matter ($chi^{0}$) is accompanied by a charged excited state ($chi^{-}$) separated by a small mass difference, it can form a
We report a measurement of the neutrino-electron elastic scattering rate from 8B solar neutrinos based on a 123 kton-day exposure of KamLAND. The background-subtracted electron recoil rate, above a 5.5 MeV analysis threshold is 1.49+/-0.14(stat)+/-0.
We present an upper limit on the flux of ultra-high-energy down-going neutrinos for $E > 10^{18} mbox{eV}$ derived with the nine years of data collected by the Telescope Array surface detector (05-11-2008 -- 05-10-2017). The method is based on the mu