Рейтинг (ПРНД) сотрудников ИЯИ РАН сезона 2022 [312]

по группам: Теоретическая физика, Ядерная физика, Нейтринная физика и КЛ, физика Частиц, Ускорительная физика, Междисциплинарные исследования
по должностям и регионам: Москва, научные Сотрудники (по Указу), научные Работники (вне Указа), Аспиранты, стуДенты, внешние совМестители, Сб...Мб - то же для БНО
ФИОГРПРНДдатадолжн
Кузнецов Михаил ЮрьевичЧ329,218.01.2022С
Кузнецов Михаил Юрьевич
1987 г.р., к.ф.-м.н., мнс ЛГАРН ОЭФ

2020 год

Публикации:
1. R. U. Abbasi et al. (Telescope Array collaboration), Search for point sources of ultra-high-energy photons with the Telescope Array surface detector, Mon.Not.Roy.Astron.Soc. 492, 3984 (2020)
ПРНД = 30*5.287*0.047 = 7.45

2. R. U. Abbasi et al. (Telescope Array collaboration), Evidence for a Supergalactic Structure of Magnetic Deflection Multiplets of Ultra-High Energy Cosmic Rays, Astrophys. J. 899, 86 (2020)
ПРНД = 30*5.745*0.047 = 8.28

3. R. U. Abbasi et al. (Telescope Array collaboration), Measurement of the proton-air cross section with Telescope Array’s Black Rock Mesa and Long Ridge fluorescence detectors, and surface array in hybrid mode, Phys.Rev.D 102, 062004 (2020)
ПРНД = 30*5.296*0.047 = 7.47

4. R. U. Abbasi et al. (Telescope Array collaboration), Search for Large-scale Anisotropy on Arrival Directions of Ultra-high-energy Cosmic Rays Observed with the Telescope Array Experiment, Astrophys.J.Lett. 898 L28 (2020)
ПРНД = 30*7.413*0.047 = 10.45

5. J.W. Belz et al. (Telescope Array collaboration), Observations of the origin of downward terrestrial gamma-ray flashes, Journal of Geophysical Research: Atmospheres, 125, e2019JD031940 (2020)
ПРНД = 30*4.261*0.047 = 6.01

6. R. U. Abbasi et al. (Telescope Array collaboration), Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector, J.Exp.Theor.Phys. 131, 255 (2020)
ПРНД = 60*1.290*0.047 = 3.64

7. D. Ivanov, O.E. Kalashev, M.Yu. Kuznetsov, G.I. Rubtsov, T. Sako, Y. Tsunesada, Y.V. Zhezher, Using Deep Learning to Enhance Event Geometry Reconstruction for the Telescope Array Surface Detector, Mach. Learn.: Sci. Technol. 2, 015006 (2021)
ПРНД = 8*0.3 = 2.4

Итого за 2020 год: ПРНД = 45.7

2021 год

Публикации:
1. O.Kalashev, M.Kuznetsov and Y.Zhezher, Constraining superheavy decaying dark matter with directional ultra-high energy gamma-ray limits, JCAP 11, 016 (2021)
ПРНД = 30*5.839*0.51 = 89.34

2. M.Y.Kuznetsov and P.G.Tinyakov, UHECR mass composition at highest energies from anisotropy of their arrival directions, JCAP 04, 065 (2021)
ПРНД = 30*5.839*0.65 = 113.86

3. R.U.Abbasi et al. (Telescope Array collaboration), The Cosmic-Ray Composition between 2 PeV and 2 EeV Observed with the TALE Detector in Monocular Mode, Astrophys. J. 909, 178 (2021)
ПРНД = 30*5.745*0.047 = 8.28

4. R.U.Abbasi et al. (Telescope Array collaboration), Surface detectors of the TAx4 experiment, Nucl. Instrum. Meth. A 1019, 165726 (2021)
ПРНД = 30*5.745*0.047 = 2.05

5. L.A.Anchordoqui et al. (20 authors), Hunting super-heavy dark matter with ultra-high energy photons, Astropart. Phys. 132, 102614 (2021)
ПРНД = 30*2.724*0.125 = 10.22


Доклады:
1. Mikhail Kuznetsov, устный доклад, "UHECR mass composition from anisotropy of their arrival directions with the Telescope Array SD", 37th International Cosmic Ray Conference (ICRC-2021), 12-23 июля 2021, Берлин, Германия (онлайн).
https://icrc2021-venue.desy.de/video/UHECR-mass-composition-from-anisotropy-of-their-arrival-directions-with-the-Telescope-Array-SD/bc43f03e66503fbc3c31cb24a2c1c873
ПРНД = 25.0

2. Ivan Kharuk, Mikhail Kuznetsov, Yana Zhezher, Grigory Rubtsov, Oleg Kalashev, постерный доклад, "Mass composition of Telescope Array's surface detectors events using deep learning", 37th International Cosmic Ray Conference (ICRC-2021), 12-23 июля 2021, Берлин, Германия (онлайн).
https://icrc2021-venue.desy.de/video/Mass-composition-of-Telescope-Array039s-surface-detectors-events-using-deep-learning/6806b2c0907e14e53e79bb66333f977e
ПРНД = 10.0*0.38 = 3.8

3. Grigory Rubtsov, Ivan Kharuk, Mikhail Kuznetsov, постерный доклад, "Identifying mass composition of ultra high energy cosmic rays using deep learning", 20th International Workshop on Advanced Computing and Analysis Techniques in Physics Research (ACAT-2021), 29 ноября - 3 декабря 2021, Daejeon, South Korea (онлайн).
https://indico.cern.ch/event/855454/contributions/4596374/
ПРНД = 10.0*0.51 = 5.1

Материалы конференций:
1. Oleg E. Kalashev, Ivan V. Kharuk, Mikhail Yu. Kuznetsov and Grigory I. Rubtsov, Telescope Array search for EeV photons, Proceedings of Science, ICRC2021, 864 (2021)
ПРНД = 8*0.43 = 3.44

2. Mikhail Kuznetsov and Peter Tinyakov, UHECR mass composition from anisotropy of their arrival directions with the Telescope Array SD, Proceedings of Science, ICRC2021, 294 (2021)
ПРНД = 8*0.65 = 5.2

3. O.E. Kalashev, D. Ivanov, M.Yu. Kuznetsov, G.I. Rubtsov, T. Sako, Y. Tsunesada and Y.V. Zhezher, UHECR mass composition from anisotropy of their arrival directions with the Telescope Array SD, Proceedings of Science, ICRC2021, 252 (2021)
ПРНД = 8*0.30 = 2.4

4. T. Fujii et al. (14 authors), Telescope Array anisotropy summary, Proceedings of Science, ICRC2021, 392 (2021)
ПРНД = 8*0.20 = 1.6

5. Armando di Matteo et al. (16 authors), UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies, Proceedings of Science, ICRC2021, 308 (2021)
ПРНД = 8*0.20 = 1.6

6. Peter Tinyakov et al. (16 authors), The UHECR dipole and quadrupole in the latest data from the original Auger and TA surface detectors, Proceedings of Science, ICRC2021, 375 (2021)
ПРНД = 8*0.20 = 1.6

Подача заявок на гранты:
Заявка РНФ-22-22-00883 «Анализ состава и анизотропии космических лучей путем переобработки данных KASCADE-Grande с помощью машинного обучения», руководитель М.Ю. Кузнецов, на конкурс «Проведение фундаментальных научных исследований и
поисковых научных исследований малыми отдельными научными группами»
ПРНД = 10.0

Итого за 2021 год: ПРНД = 283.5

Итого за 2 года: ПРНД = 45.7 + 283.5 = 329.2