22-25 October 2024
Hotel Intourist Kolomenskoye 4*
Europe/Moscow timezone
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Status and Physics Potential of SATURNE

25 Oct 2024, 18:25
15m
Petrovskiy 1 ()

Petrovskiy 1

Oral talk Neutrino physics Neutrino

Speaker

Konstantin Kouzakov (Lomonosov Moscow State University)

Description

The Sarov tritium neutrino experiment (SATURNE) is part of the scientific program of the National Center for Physics and Mathematics (NCPM) [1] that was founded in Sarov in 2021. The experiment is under preparation, with the first taking of data expected for 2025.
Being motivated by fundamental problems in neutrino physics, SATURNE will primarily search for neutrino electromagnetic interactions [2,3] in elastic and ionizing neutrino-atom collisions. It will employ a high-intensity tritium neutrino source, with an initial activity of at least 10 MCi and possibly up to 40 MCi. The tritium source will be used in combination with the He-4, Si and SrI$_2$(Eu) targets in order to study the elastic and ionization channels of neutrino-atom collisions at unprecedentedly low energies. The Si and SrI$_2$(Eu) detectors with record low-energy thresholds for such detector types will measure the ionization channel of neutrino-atom collisions. With the 1-year data from either detector, one may expect to achieve a sensitivity on the order of $\sim10^{-12}\,\mu_B$ at 90% C.L. to the neutrino magnetic moment $\mu_\nu$, which is the most studied theoretically and actively searched experimentally among the neutrino electromagnetic properties. The measurements with the liquid He-4 detector in a superfluid state are expected to provide the first observation of coherent elastic neutrino-atom scattering (CEνAS) [4,5]. This will bring the experimental studies of coherent elastic neutrino-nucleus scattering (CEνNS) [6] to a qualitatively new level, namely when one will be able to explore the neutrino elastic scattering not only on a nucleus as a whole, but also on an atom as a whole. With the 5-year data using the liquid He-4 detector, it is also expected to achieve a record-high $\mu_\nu$-sensitivity of $\sim10^{-13}\,\mu_B$ at 90% C.L.

References

  1. А.А. Yukhimchuk et al., FIZMAT 1 (2023) 5 (in Russian)
  2. C. Giunti and A. Studenikin, Rev. Mod. Phys. 87 (2015) 531
  3. A.I. Studenikin and K.A. Kouzakov, Mosc. Univ. Phys. Bull. 75 (2020) 379
  4. Yu.V. Gaponov and V.N. Tikhonov, Sov. J. Nucl. Phys. 26 (1977) 314
  5. M. Cadeddu, F. Dordei, C. Giunti, K. Kouzakov, E. Picciau, and A. Studenikin, Phys. Rev. D 100 (2019) 073014
  6. V. Pandey, Prog. Part. Nucl. Phys. 134 (2024) 104078

Primary authors

Matteo Cadeddu (Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Cagliari) Francesca Dordei (Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Cagliari) Carlo Giunti (Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Torino) Alexander Ivashkin (Institute for Nuclear Research RAS) Konstantin Kouzakov (Lomonosov Moscow State University) Fedor Lazarev (Lomonosov Moscow State University) Oleg Moskalev (Russian Federal Nuclear Center – All-Russian Scientific Research Institute of Experimental Physics) Ivan Stepantsov (Lomonosov Moscow State University) Alexander Studenikin (Lomonosov Moscow State University) Igor Tkachev (Institute for Nuclear Research RAS) Vladimir Trofimov (Joint Institute for Nuclear Research) Maxim Verkhovtsev (Branch of Lomonosov Moscow State University in Sarov) Maxim Vyalkov (Branch of Lomonosov Moscow State University in Sarov) Arkady Yukhimchuk (Russian Federal Nuclear Center – All-Russian Scientific Research Institute of Experimental Physics) Elvira Zagirdinova (Lomonosov Moscow State University)

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