Speaker
Description
Summary
Our research focuses on the analytical estimation and subsequent numerical simulation of a time-resolved observation of the solar neutrino day-night effect. The regeneration factor in the Earth depends on the solar elevation in a highly oscillatory way, the latter on the time of day and the season, so that an experiment observing nighttime solar neutrinos virtually measures an expectation value (with some variance) of a rapidly-oscillating function over the observation time window. Usually making the window smaller reduces the signal-to-noise ratio, however, as we show in [arXiv.org/1509.08073], such a logic applies only to the cumulative, non-oscillating component of the signal. The signal in question, however, also contains a peculiar, time-localized contribution, mathematically corresponding to a stationary point of an oscillatory function, that can be drawn out of noise by restriction of the observation time window. Such 'time-resolved' observations lead to a number of effects at the level of the resulting recoil electron spectrum, whose isolation could, e.g., help to precisely measure the neutrino mass-squared difference.