Okuneva E., Sveshnikova L., Astapov I., Bezyazykov P., Blinov A., Borodin A., Bonvech E., Budnev N., Bulan A., Busygin P., Vaidyanatan A., Volkov N., Volchugov P., Voronin D., Gafarov A., Gres E., Gres O., Gres T., Grishin O., Garmash A., Grebenyuk V., Grinyuk A., Dyachok A., Zhurov D., Zagorodnikov A., Ivanova A., Ivanova A., Ilyushin M., Kalmykov N., Kindin V., Kiryukhin V., Kokoulin R., Kolosov N., Kompaniets K., Korosteleva E., Kozhin V., Kravchenko E., Kryukov A., Kuzmichev L., Chiavassa A., Lavrova M., Lagutin A., Lemeshev Y., Lubsandorzhiev B., Lubsandorzhiev N., Malakhov S., Mirgazov R., Monkhoev R., Osipova E., Pakhorukov A., Pan A., Panov A., Pankov L., Petrukhin A., Podgrudkov D., Poddubny I., Popova E., Postnikov E., Prosin V., Ptuskin V., Pushnin A., Razumov A., Raikin R., Rubtsov G., Ryabov E., Samoliga V., Satyshev I., Silaev A., Silaev, Jr. A., Sidorenkov A., Skurikhin A., Sokolov A., Tabolenko V., Tanaev A., Ternovoy M., Tkachev L., Ushakov N., Chernov D., Yashin I.
Abstract
In November 2020, the IceCube neutrino Observatory registered a neutrino event with an energy of 150 TeV directed at the Cygnus Cocoon gamma-ray source. In the Carpet-2 experiment, as part of the Baksan Neutrino Observatory (BNO), a sharp increase in the flow of events with an energy of more than 300 TeV was recorded from the same direction within the angular accuracy of the events. This flux is 4 orders of magnitude higher than the expected intensity of gamma quanta of this energy region according to data in the region of less than 100 TeV. It was expected that such a powerful flare could be registered by the TAIGAHiSCORE installation of the TAIGA astrophysical complex. We analyzed the events of the EAS recorded by the installation of TAIGA-HiSCORE for 18 hours in October-November 2020 fromthe Cygnus Cocoon source. The article provides the upper limit of the expected excess flow.
Âdernaâ fizika. 2024;87(3):162-169