Study of the atmospheric neutrino flux in the multi-GeV energy range

Abstract

The flavor ratio of the atmospheric neutrino flux and its zenith angle dependence have been studied in the multi-GeV energy range using an exposure of 25.5 kiloton-years of the Super-Kamiokande detector. By comparing the data to a detailed Monte Carlo simulation, the ratio $(\mu /e{)}_{DATA}/(\mu /e{)}_{MC}$ was measured to be $0.66\pm 0.06(stat.)\pm 0.08(sys.)$. In addition, a strong distortion in the shape of the $\mu$-like event zenith angle distribution was observed. The ratio of the number of upward to downward $\mu$-like events was found to be 0.52${}_{-0.06}^{+0.07}(stat.)\pm 0.01(sys.)$, with an expected value of $0.98\pm 0.03(stat.)\pm 0.02(sys.)$, while the same ratio for the $e$-like events was consistent with unity.

14 pages with 6 figures, minor changes for publication

References in corpus (1)

• Measurement of a small atmospheric ${\nu }_{\mu }/{\nu }_e$ ratio

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