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High Sensitivity Search forν¯e's from the Sun and Other Sources at KamLAND
2004
Physical Review Letters
Data corresponding to a KamLAND detector exposure of 0.28 kton-year has been used to search for ν̅_e's in the energy range 8.3 MeV < E_ν̅_e < 14.8 MeV. No candidates were found for an expected background of 1.1±0.4 events. This result can be used to obtain a limit on ν̅_e fluxes of any origin. Assuming that all ν̅_e flux has its origin in the Sun and has the characteristic ^8B solar ν_e energy spectrum, we obtain an upper limit of 3.7 × 10^2 cm^-2 s^-1 (90 C.L.) on the ν̅_e flux. We interpret
doi:10.1103/physrevlett.92.071301
pmid:14995837
fatcat:3b5lodv64fbd7pu4xekzpeb7ky