Russia, Moscow

EC NEVOD
Experimental complex NEVOD

Operational

The Unique Scientific Facility “Experimental Complex NEVOD” is the only in the world that allows conducting basic (particle physics and astrophysics) and applied (monitoring of the state of the atmosphere and magnetosphere of the Earth and of extra-terrestrial space) research based on the analysis of detected of natural fluxes of the particles at the Earth’s surface over the entire range of zenith angles (from 0 to 180 degrees) and in the record energy range (1 – 1010 GeV).

The Unique Scientific Facility “Experimental Complex NEVOD” is the experimental site ground for the development, testing and calibration of the new nuclear physics equipment and new methods and approaches.

Commissioning: 2025
PRESENTATION CONTACT US OFFICIAL WEB-SITE

National Research Nuclear University MEPhI

https://eng.mephi.ru/

SCIENTIFIC DOMAINS

Particle Physics, High and Ultra-high Energy Physics

Key words: high energy physics, cosmic rays, extensive air showers

SCIENTIFIC GOALS

 

Fundamental goals: the study of characteristics of the primary cosmic ray flux, processes of generation and interaction of known particles, the search for new particles and states of matter in a wide range of energies, including energies 10 times higher than those accessible at the Large Hadron Collider.

Applied goals: the distant monitoring and forecasting of the state of the Earth’s atmosphere and magnetosphere aimed at the early recognition of potentially dangerous magnetospheric and atmospheric phenomena over the territory of about 10,000 square kilometers.

 

FACILITIES

The Unique Scientific Facility “Experimental Complex NEVOD” combines ten different detectors that have no analogues in the world: a Cherenkov water detector (CWD) with a volume of 2000 cubic meters capable to measure the energy deposit of charged particles in a wide dynamic range, the coordinate-tracking detectors DECOR with a total area of 72 square meters with angular (better than 1 degree) and spatial (1 cm) accuracy and TREK with an area 250 square meters with spatial (1 mm) resolution, the muon hodoscopes URAGAN with an area of 46 square meters and ScMH with an area of 23 square meters providing muonographs of the upper hemisphere in real-time mode, a calibration telescope system (CTS) that allows allocation of 1600 different muon trajectories and detection of electromagnetic and muon components of extensive air showers (EAS), a NEVOD-EAS array with an area of 10 000 square meters for measuring charged EAS component, the neutron arrays PRISMA-36, URAN and “Neutron” providing thermal neutrons detection under different conditions (inside the building, underground and on the buildings roofs).

CHALLENGES

Conducting research in the record energy range of 1010 – 1019 eV, development, testing and calibrating nuclear-physics equipment, as well as training students and postgraduates through their direct participation in real physical experiments.

PARTNERSHIP PROPOSAL

– Dipartimento di Fisica dell’ Universita di Torino (DF UT), Italy

– Observatorio Astrofisico di Torino – INAF (OAT, assignee of IFSI), Torino, Italy

– A. I. Alikhanyan National Scientific Laboratory (YerPhI), Armenia

– University Santiago de Compostela, Spain

– University of Michigan, USA

– University of Muenster, Germany

PARTNERS

PUBLICATIONS

  1. A.A. Petrukhin. Muon Puzzle in Cosmic Rays and Its Possible Solution. Physics of Atomic Nuclei (2021). Vol. 84, № 1, pp. 92-99. 2021. ISSN 1063-7788, DOI: 10.1134/S1063778821010142
  2. I.I. Yashin, M.B. Amelchakov, I.I. Astapov, N.S. Barbashina, et al. NEVOD — An experimental complex for multi-component investigations of cosmic rays and their interactions in the energy range 1–10^10 GeV. Journal of Instrumentation (2021). 16 (8), T08014. DOI: 10.1088/1748-0221/16/08/T08014
  3. M. B. Amelchakov, N. S. Barbashina, A. G. Bogdanov, A. Chiavassa, et al. The NEVOD-EAS air-shower array. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment (2022). Vol. 1026, 166184. DOI: 10.1016/j.nima.2021.166184
  4. M. B. Amelchakov, A. G. Bogdanov, A. Chiavassa, A. N. Dmitrieva, et al. Cosmic-Ray Anisotropy Study by Means of Detection of Muon Bundles. The Astrophysical Journal, V. 945, № 2, 123 (10pp), 2023 March 14. DOI: 10.3847/1538-4357/acb1fc
  5. G. Bogdanov, N. S. Barbashina, S. S. Khokhlov, V. V. Kindin, et al. Studying Muon Bundles of Inclined Air Showers in the NEVOD-DECOR Experiment. Physics of Atomic Nuclei (2023). Vol. 86, Is. 6, pp. 1027-1037. DOI: 10.1134/S1063778824010137
  6. M.B. Amelchakov, A.G. Bogdanov, A. Chiavassa, D.M. Gromushkin, et al. A quasi-spherical optical module QSM-6M based on the Hamamatsu R877 PMT for the detection of Cherenkov radiation in water. Nuclear Instruments and Methods in Physics Research A 1064 (2024) 169437. https://doi.org/10.1016/j.nima.2024.169437
  7. A.G. Bogdanov, A. Chiavassa, D.M. Gromushkin, S.S. Khokhlov, et al. Energy spectrum and mass composition of the primary cosmic rays based on the intensity of muon bundles detected in the NEVOD-DECOR experiment. Physical Review D 112, 103041 (2025) DOI: 10.1103/clp6-bp28

EVENTS

The 2nd International Symposium on Cosmic Rays and Astrophysics (ISCRA-2019) https://iscra2019.mephi.ru/

The International Symposium on Cosmic Rays and Astrophysics (ISCRA-2021) https://indico.nevod.mephi.ru/event/6/

The International Symposium on Cosmic Rays and Astrophysics (ISCRA-2023) https://indico.nevod.mephi.ru/event/9/

The International Symposium on Cosmic Rays and Astrophysics (ISCRA-2023) https://indico.nevod.mephi.ru/event/13/

CONTACTS



Petrukhin Anatoly


Senior researcher National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)