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Methods for the suppression of background cascades produced along atmospheric muon tracks in the Baikal-GVD

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arxiv 2107.14510 v1 pith:XMLXVOWR submitted 2021-07-30 astro-ph.IM physics.ins-det

V. A. Allakhverdyan , A. D. Avrorin , A. V. Avrorin , V. M. Aynutdinov , R. Bannasch , Z. Bardačová , I. A. Belolaptikov , I. V. Borina
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V. B. Brudanin N. M. Budnev V. Y. Dik 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 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 Pa. Malecki Y. M. Malyshkin 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. E. Sirenko A. V. Skurikhin A. G. Solovjev M. N. Sorokovikov I. Štekl A. P. Stromakov E. O. Sushenok O. V. Suvorova V. A. Tabolenko B. A. Tarashansky Y. V. Yablokova S. A. Yakovlev D. N. Zaborov
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classification astro-ph.IMphysics.ins-det
keywords backgroundbaikal-gvdcascadesneutrinoalongcascadeeventsmethods
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The Baikal-GVD (Gigaton Volume Detector) is a km$^{3}$- scale neutrino telescope located in Lake Baikal. Currently (year 2021) the Baikal-GVD is composed of 2304 optical modules divided to 8 independent detection units, called clusters. Specific neutrino interactions can cause Cherenkov light topology, referred to as a cascade. However, cascade-like events originate from discrete stochastic energy losses along muon tracks. These cascades produce the most abundant background in searching for high-energy neutrino cascade events. Several methods have been developed, optimized, and tested to suppress background cascades.

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