2002
DOI: 10.2172/805485
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Very Long Baseline Neutrino Oscillation Experiments for Precise Measurments of Oscillation Parameters and Search for N Mu Yields N Epsilon.

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“…At the second VOM, the size of the δ-dependent interference term between the atmospheric and the solar terms is a factor of ∼ 3 larger than that at the first VOM, which would lead to higher sensitivity to δ. The favorable feature is utilized in this and in the earlier proposals, e.g., in [40][41][42][43]. Here, we consider one of the setups within the ESSνSB proposal, which consists of a 500 kt fiducial mass water Čerenkov detector placed at 540 km from the source.…”
mentioning
confidence: 99%
“…At the second VOM, the size of the δ-dependent interference term between the atmospheric and the solar terms is a factor of ∼ 3 larger than that at the first VOM, which would lead to higher sensitivity to δ. The favorable feature is utilized in this and in the earlier proposals, e.g., in [40][41][42][43]. Here, we consider one of the setups within the ESSνSB proposal, which consists of a 500 kt fiducial mass water Čerenkov detector placed at 540 km from the source.…”
mentioning
confidence: 99%