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25–29 Oct 2021
Wangjiang Hotel
Asia/Shanghai timezone

The astrophysics program of the NOvA experiment

29 Oct 2021, 15:00
20m
Wangjiang Hotel

Wangjiang Hotel

No.42 Xiashahepu Street, Jinjiang District, Chengdu City, Sichuan Province, China
oral Session 4

Speaker

Oleg Samoylov (Joint Institute for Nuclear Research)

Description

The NOvA experiment is aimed to solve the fundamental neutrino problems: precise determination of neutrino oscillation parameters, determination of neutrino mass hierarchy, search for the CP-violation in the leptonic sector. NOvA consists of the near detector on the Fermi National Laboratory site, where the muon neutrinos are produced in the NuMI accelerator complex, and the far detector located 810 km away at Ash River, detecting both survived muon and new appeared electron neutrinos. Both detectors have similar structure based on the liquid scintillator filling large volumes with detailed segmentation. The mass of the detectors target part is 14 ktons for the far detector and 220 tons for the near detector, providing to study wide astrophysical program beyond neutrino oscillation and neutrino cross-section measurements, search and detection for different signals from Space and the Earth's environment: supernova, magnetic monopole, atmospheric muons, dark matter and potential signals in coincidence with the LIGO/Virgo gravitational wave events.
Please choose the session this abstract belongs to Particle physics

Primary author

Oleg Samoylov (Joint Institute for Nuclear Research)

Presentation materials