02-2-1148-2010/2028
   

Baikal-GVD
Baikal Deep Underwater Gigaton Volume Neutrino Telescope


Leaders:  

Deputy: 

I.A. Belolaptikov

S.V. Rozov


Participating countries and international organizations:
Czech Republic, Kazakhstan, Russia, Slovakia.
 

The problem under study and the main purpose of the research:
Implementation of the project that includes modernization and development of the Baikal deepwater detector up to the detection volume of 1 km3 in studies of high-energy neutrino fluxes of astrophysical origin.

 

Project:

 Name of the project Project Leaders Project code
Laboratory     Responsible from laboratories     Status
1. Baikal-GVD

I.A. Belolaptikov
Deputy:
S.V. Rozov

02-2-1148-1-2010/2028

Realization
DLNP V.F. Allakhverdyan, P.I. Antonov, I.V. Borina, V. Dik, I.S. Dotsenko, A.A. Doroshenko, T.V. Elzhov, A.N. Emelianov, A.Golubev, K.V. Golubkov, N.A. Gorshkov, B. Kalinova, I. Kamnev, S.A. Katulin, S.L. Katyulina, E.V. Khramov, M.M. Kolbin, K.V. Konisсhev, A.V. Korobchenko, M.V. Kruglov, E. Kulkova, T. Lednitska, N.V. Mazarskaya, M.L. Minaev, T.А. Morozova, D.V. Naumov, D.A. Orlov, D.P. Petukhov, E.N. Pliskovski, V.G. Sandukovsky, G.B. Safronov, I. Scherbakova ,A.E. Sirenko, M.N. Sorokovikov, N.I. Sosunov, I.A. Stepkin, A.P. Stromakov, B.A. Shaybonov, K.I. Shevchenro, M. Shevchenko, B.B. Ulzutuev, V. Volnykh, Yu.V. Yablokova, E.Yakushev, D.V. Zvezdov, S. Zavialov, A. Zaikin

MLIT M.S. Katulin, A. Soloviev


Brief annotation and scientific rationale:
The Baikal-GVD project is aimed at the further development of the gigaton-scale neutrino telescope for conducting research in multimessenger astronomy, study of fundamental properties of the most energetic cosmic neutrinos, indirect search for galactic dark matter and applied research. The international collaboration of the Baikal-GVD project is constructing a neutrino telescope in Lake Baikal. The arrays of light-sensitive elements, housed in optical modules, detect Cherenkov light produced by charged particles in the water of the lake while travelling with the speed exceeding the speed of light in water. These particles could originate from interactions of neutrinos in water or in the rock of the lake bed. The energy and direction of original neutrinos are reconstructed from the amount of Cherenkov photons and time of their detection by light-sensitive elements. The telescope is capable of investigating cosmic neutrinos and identifying their sources, searching for neutrinos from dark matter annihilation and other rare phenomena. The scientific programme of the project is focused on solving fundamental problems of astrophysics and elementary particle physics: identification of astrophysical sources of ultrahigh-energy neutrinos, revealation of mechanisms of formation and evolution of galaxies, etc. In particular, one of the short-range goals is mapping the high-energy neutrino sky in the Southern Hemisphere, including the region of the Galactic Centre. Other topics include the indirect search for dark matter by detecting neutrinos produced in WIMP annihilations in the Sun or in the Earth’s interior. Baikal-GVD will also search for exotic particles, such as magnetic monopoles, supersymmetric Q-balls or nuclearities. Baikal-GVD, the unique neutrino telescope, is one of the basic facilities at JINR.
 
Expected results upon completion of the project:
Construction of a deep-underwater neutrino telescope on a scale of 1 km3 in Lake Baikal. Study of high-energy neutrino fluxes from space, search for hypothetical particles – magnetic monopoles, as well as particles – candidates for dark matter. A large detection volume, in combination with a high angular and energy resolution and also with moderate background conditions typical of fresh water, makes it possible to effectively study the diffusive neutrino flux and fluxes from individual astrophysical objects with constant and variable luminosity.

Expected results for the project in the current year:
Data taking by 13 already installed clusters of the Baikal-GVD neutrino telescope. Search for and study of events from high-energy neutrinos of astrophysical origin. Preparation for and deployment of the following detector clusters. Testing of a new system of data acquisition and transmission which ensures the reduction of the threshold of detectable energies.

Collaboration

Country or International Organization City Institute or laboratory
Czech Republic Prague CTU
Kazakhstan Almaty INP
Russia Irkutsk ISU
  Moscow SINP MSU
  Moscow, Troitsk INR RAS
  Nizhny Novgorod NNSTU
  Saint Petersburg SMTU
Slovakia Bratislava CU