Search for cascade events with Baikal-GVD
Baikal-GVD Collaboration: A.D. Avrorin, A.V. Avrorin, V.M. Aynutdinov,, R. Bannash, I.A Belolaptikov, V.B. Brudanin, N.M. Budnev, G.V. Domogatsky,, A.A. Doroshenko, R. Dvornicky, A.N. Dyachok, Zh.-A.M. Dzhilkibaev, L. Fajth,, S.V Fialkovsky, A.R. Gafarov, K.V. Golubkov
TL;DR
Baikal-GVD, a large-scale neutrino telescope in Lake Baikal, is designed to detect astrophysical neutrinos at very high energies, and this paper presents preliminary results from cascade mode searches.
Contribution
This work reports the first preliminary results of high-energy neutrino searches using the Baikal-GVD telescope in cascade mode.
Findings
Initial detection of high-energy neutrino candidates.
Potential sensitivity to astrophysical neutrino fluxes.
Validation of the cascade detection method.
Abstract
Baikal-GVD is a next generation, kilometer-scale neutrino telescope currently under construction in Lake Baikal. GVD is formed by multi-megaton sub-arrays (clusters) and is designed for the detection of astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. The design of the Baikal-GVD allows one to search for astrophysical neutrinos with flux values measured by IceCube already at early phases of the array construction. We present here preliminary results of the search for high-energy neutrinos via the cascade mode with the Baikal-GVD neutrino telescope.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Neutrino Physics Research