1. High-Energy Neutrino Astronomy and the Baikal-GVD Neutrino Telescope
- Author
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A. D. Avrorin, A. V. Avrorin, V. M. Aynutdinov, R. Bannasch, Z. Bardáčová, I. A. Belolaptikov, V. Dik, V. B. Brudanin, N. M. Budnev, G. V. Domogatsky, A. A. Doroshenko, R. Dvornický, A. N. Dyachok, Zh.-A. M. Dzhilkibaev, E. Eckerová, T. V. Elzhov, L. Fajt, S. V. Fialkovski, A. R. Gafarov, K. V. Golubkov, N. S. Gorshkov, T. I. Gress, R. A. Ivanov, M. S. Katulin, K. G. Kebkal, O. G. Kebkal, E. V. Khramov, M. M. Kolbin, K. V. Konischev, K. A. Kopański, A. V. Korobchenko, A. P. Koshechkin, V. A. Kozhin, M. V. Kruglov, M. K. Kryukov, V. F. Kulepov, M. B. Milenin, R. R. Mirgazov, D. V. Naumov, V. Nazari, W. Noga, D. P. Petukhov, E. N. Pliskovsky, M. I. Rozanov, V. D. Rushay, E. V. Ryabov, G. B. Safronov, B. A. Shaybonov, M. D. Shelepov, F. Šimkovic, A. V. Skurikhin, A. G. Solovjev, M. N. Sorokovikov, I. Štekl, E. O. Sushenok, O. V. Suvorova, V. A. Tabolenko, B. A. Tarashansky, Y. V. Yablokova, S. Yakovlev, and D. N. Zaborov
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Nuclear and High Energy Physics ,High energy ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,media_common.quotation_subject ,Neutrino telescope ,Astrophysics::Instrumentation and Methods for Astrophysics ,Northern Hemisphere ,FOS: Physical sciences ,Astronomy ,Construction plan ,Atomic and Molecular Physics, and Optics ,Universe ,Neutrino ,Neutrino astronomy ,Astrophysics - High Energy Astrophysical Phenomena ,Effective volume ,media_common - Abstract
Neutrino astronomy offers a novel view of the non-thermal Universe and is complementary to other astronomical disciplines. The field has seen rapid progress in recent years, including the first detection of astrophysical neutrinos in the TeV-PeV energy range by IceCube and the first identified extragalactic neutrino source (TXS 0506+056). Further discoveries are aimed for with new cubic-kilometer telescopes in the Northern Hemisphere: Baikal-GVD, in Lake Baikal, and KM3NeT-ARCA, in the Mediterranean sea. The construction of Baikal-GVD proceeds as planned; the detector currently includes over 2000 optical modules arranged on 56 strings, providing an effective volume of 0.35 km$^3$. We review the scientific case for Baikal-GVD, the construction plan, and first results from the partially built array., 9 pages, 5 figures, to be published in Proceedings of the 5-th International Conference on Particle Physics and Astrophysics (ICPPA-2020), October 5-9, 2020
- Published
- 2021
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