1992
DOI: 10.1103/physrevlett.68.2429
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Particle detection by evaporation from superfluid helium

Abstract: We report the first experiments in which 5-MeV alpha particles are detected via evaporation from a bath of superfluid helium. The a excites phonons and rotons in the liquid helium, and these excitations are sufficiently energetic to evaporate helium atoms when they reach the free surface of the liquid. The approximate overall efficiency of this process has been determined, and we compare this with expectations. We have also been able to detect evaporation induced by a flux of r's from a 137 Cs source.

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Cited by 23 publications
(18 citation statements)
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“…The reader is referred to the recent review by Lanou (1995). There are significant challenges motivating these efforts, e.g., neutrino detection by coherent scattering off nuclei and real-time detectors for pp neutrinos, such as the superfluid 4 He detector HERON (Bandler et al 1992) and the high-pressure helium time projection chamber HELLAZ (Laurenti et al 1994). …”
Section: Other Future Detectorsmentioning
confidence: 99%
“…The reader is referred to the recent review by Lanou (1995). There are significant challenges motivating these efforts, e.g., neutrino detection by coherent scattering off nuclei and real-time detectors for pp neutrinos, such as the superfluid 4 He detector HERON (Bandler et al 1992) and the high-pressure helium time projection chamber HELLAZ (Laurenti et al 1994). …”
Section: Other Future Detectorsmentioning
confidence: 99%
“…Fortunately, although its cross-section is low (∼ 10 −45 cm 2 ) the expected flux is high (∼ 6 × 10 10 cm −2 · s −1 for p-p neutrinos in the standard solar model) so that ∼10 tons of target would yield about 20 p-p events and 7 7 Be events per day with recoil energies above 50 keV. HERON would use superfluid helium as the target material.…”
Section: General Principles Of Heronmentioning
confidence: 99%
“…The combination of these experiments is expected to give the first "smoking gun" evidence for or against oscillation of solar neutrinos. The maximum recoiling electron energy from elastic scattering of the principal 7 Be line is 665 keV; while that from the p-p continuum is only 261 keV. The upcoming BOREXINO detector, based on the use of a highly purified liquid scintillator, will give the first direct window on the 7 Be flux in real-time using the elastic scattering reaction but is not expected to access the p-p flux because of internal backgrounds at the lowest energies.…”
Section: Introductionmentioning
confidence: 99%
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