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O. Smirnov

Researcher at Joint Institute for Nuclear Research

Publications -  180
Citations -  6931

O. Smirnov is an academic researcher from Joint Institute for Nuclear Research. The author has contributed to research in topics: Borexino & Solar neutrino. The author has an hindex of 39, co-authored 170 publications receiving 5669 citations. Previous affiliations of O. Smirnov include Petersburg Nuclear Physics Institute.

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DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS

Craig E. Aalseth, +300 more
TL;DR: The DarkSide-20k detector as discussed by the authors is a direct WIMP search detector using a two-phase Liquid Argon Time Projection Chamber (LAr TPC) with an active mass of 23 t (20 t).
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Low-Mass Dark Matter Search with the DarkSide-50 Experiment

P. Agnes, +196 more
TL;DR: The results of a search for dark matter weakly interacting massive particles (WIMPs) in the mass range below 20 GeV/c^{2} using a target of low-radioactivity argon with a 6786.0 kg d exposure are presented.
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Direct measurement of the 7Be solar neutrino flux with 192 days of Borexino data

C. Arpesella, +135 more
TL;DR: This result is the first direct measurement of the survival probability for solar nu(e) in the transition region between matter-enhanced and vacuum-driven oscillations and improves the experimental determination of the flux of 7Be, pp, and CNO solarnu(e), and the limit on the effective neutrino magnetic moment using solar neutrinos.
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Neutrinos from the primary proton–proton fusion process in the Sun

G. Bellini, +100 more
- 27 Aug 2014 - 
TL;DR: Spectral observations of pp neutrinos are reported, demonstrating that about 99 per cent of the power of the Sun, 3.84 × 1033 ergs per second, is generated by the proton–proton fusion process.
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Measurement of the solar 8B neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector

G. Bellini, +88 more
- 05 Aug 2010 - 
TL;DR: In this paper, the authors reported the measurement of elastic scattering from {sup 8}B solar neutrinos with 3 MeV energy threshold by the Borexino detector in Gran Sasso (Italy).