Abstract
We present a summary of recent progress towards the development of a solar neutrino detector in which superfluid helium is used as a target material. In this detector phonons and rotons generated in the liquid by a recoiling particle propagate through the liquid and then cause a shower of atoms to be quantum evaporated from the liquid surface. We describe recent results which indicate that roton-roton interactions close to the track of the recoiling particle may make it possible to obtain information about the track direction.
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