Кузнецов Михаил Юрьевич
1987 г.р., к.ф.-м.н., мнс ЛГАРН ОЭФ
2017 год
Публикации:
1. Yu.A. Fomin, N.N. Kalmykov, I.S. Karpikov, G.V. Kulikov, M.Yu. Kuznetsov, G.I. Rubtsov, V.P. Sulakov, S.V. Troitsky, No muon excess in extensive air showers at 100-500 PeV primary energy: EAS-MSU results, Astropart.Phys. 92, 1 (2017).
ПРНД = 30*3.203*1.5*0.2 = 28.83
2. M.Yu. Kuznetsov, Hadronically decaying heavy dark matter and high-energy neutrino limits, JETP Lett. 105, 561 (2017).
ПРНД = 60*1.363 = 81.78
3. Yu.A. Fomin, N.N. Kalmykov, I.S. Karpikov, G.V. Kulikov, M.Yu. Kuznetsov, G.I. Rubtsov, V.P. Sulakov, S.V. Troitsky, Constraints on the flux of ?(1016?1017.5) eV cosmic photons from the EAS-MSU muon data, Phys.Rev. D95, 123011 (2017).
ПРНД = 30*4.394*1.5*0.2 = 39.55
4. O.E. Kalashev, M. Yu. Kuznetsov, Heavy decaying dark matter and large-scale anisotropy of high-energy cosmic rays, JETP Lett. 106, 73 (2017).
ПРНД = 60*1.363/2 = 40.89
Препринты:
1. Telescope Array Collaboration (R.U. Abbasi et al.), Search for Anisotropy in the Ultra High Energy Cosmic Ray Spectrum using the Telescope Array Surface Detector, arXiv:1707.04967.
ПРНД = 3*0.06=0.18
Доклады:
1. Устный доклад, Mikhail Kuznetsov, Multimessenger search for heavy dark mater, International Session-Conference of the Section of Nuclear Physics of the Physical Sciences Department of the Russian Academy of Sciences "Physics of fundamental interactions" dedicated to 50th anniversary of Baksan Neutrino Observatory, Nalchik, Russia, 6-8 June 2017.
http://icssnp.inr.ac.ru/en/program_en/
ПРНД = 25.0
2. Устный доклад, Mikhail Kuznetsov, Multimessenger search for heavy dark mater, The XXIII International Workshop "High Energy Physics and Quantum Field Theory" (QFTHEP-2017), Yaroslavl, Russia, 26 June - 3 July 2017.
http://qfthep.sinp.msu.ru/programme/june-28-2017
ПРНД = 25.0
3. Устный доклад, Mikhail Kuznetsov, Vladimir SULAKOV, Ivan KARPIKOV, Grigory RUBTSOV, Sergey TROITSKY, Nikolay KALMYKOV, German KULIKOV, Yuri FOMIN, No muon excess in EAS at 100 PeV: results of EAS-MSU experiment, The International Cosmic Ray Conference 2017, Busan, South Korea, 12 - 20 July 2017.
https://indico.snu.ac.kr/indico/event/15/session/5/contribution/318
ПРНД = 10.0 + 15*0.2 = 13.0
4. Устный доклад, Yana ZHEZHER, Maxim PISKUNOV, Mikhail KUZNETSOV, Grigory RUBTSOV, Sergey TROITSKY, TA SD composition results, The International Cosmic Ray Conference 2017, Busan, South Korea, 12 - 20 July 2017.
https://indico.snu.ac.kr/indico/event/15/session/5/contribution/582
ПРНД = 15/5 = 3.0
5. Устный доклад, Benjamin STOKES, Gordon THOMSON, Maxim PISKUNOV, Masaki FUKUSHIMA, Mikhail KUZNETSOV, Dmitry IVANOV, Sergey TROITSKY, Yana ZHEZHER, Grigory RUBTSOV, Telescope Array search for EeV photons and neutrinos, The International Cosmic Ray Conference 2017, Busan, South Korea, 12 - 20 July 2017.
https://indico.snu.ac.kr/indico/event/15/session/5/contribution/618
ПРНД = 15*0.2 = 3.0
6. Стендовый доклад, Mikhail Kuznetsov, Vladimir SULAKOV, Ivan KARPIKOV, Grigory RUBTSOV, Sergey TROITSKY, Nikolay KALMYKOV, German KULIKOV, Yuri FOMIN, Constraints on the flux of ? (10?300) PeV cosmic photons from the EAS-MSU muon data, The International Cosmic Ray Conference 2017, Busan, South Korea, 12 - 20 July 2017.
https://indico.snu.ac.kr/indico/event/15/session/9/contribution/1359
ПРНД = 10*0.2 = 2.0
Преподавание:
Проведение семинаров по курсу «Методы машинного обучения для обработки данных» на кафедре Физики частиц и космологии Физического факультета МГУ. Весенний семестр.
ПРНД = 8.0
Итого за 2017: ПРНД = 270.23
2018 год
Публикации:
1. R. U. Abbasi et al. (Telescope Array collaboration), Depth of Ultra High Energy Cosmic Ray Induced Air Shower Maxima Measured by the Telescope Array Black Rock and Long Ridge FADC Fluorescence Detectors and Surface Array in Hybrid Mode, Astrophys. J., 858(2):76, 2018.
ПРНД = 30*5.561*0.06 = 10.01
2. R. U. Abbasi et al. (Telescope Array collaboration), Evidence of Intermediate-Scale Energy Spectrum Anisotropy of Cosmic Rays E?10^19.2 eV with the Telescope Array Surface Detector, Astrophys. J., 862(2):91, 2018.
ПРНД = 30*5.561*0.06 = 10.01
3. R. U. Abbasi et al. (Telescope Array collaboration), The Cosmic-Ray Energy Spectrum between 2 PeV and 2 EeV Observed with the TALE detector in monocular mode, Astrophys. J., 865(1):74, 2018.
ПРНД = 30*5.561*0.06 = 10.01
4. R. U. Abbasi et al. (Telescope Array collaboration), Study of muons from ultrahigh energy cosmic ray air showers measured with the Telescope Array experiment, Phys. Rev., D98(2):022002, 2018.
ПРНД = 30*4.394*0.06 = 7.91
5. M. Kachelriess, O. E. Kalashev, and M. Yu. Kuznetsov, Heavy decaying dark matter and IceCube high energy neutrinos, Phys. Rev., D98:083016, 2018.
ПРНД = 30*4.394/3 = 43.94
6. R. U. Abbasi et al. (Telescope Array collaboration), Testing a reported correlation between arrival directions of ultrahigh-energy cosmic rays and a flux pattern from nearby starburst galaxies using Telescope Array data, Astrophys. J. Lett., 867:L27, 2018.
ПРНД = 30*6.634*0.06 = 11.94
7. Grigory Rubtsov, Masaki Fukushima, Dmitri Ivanov, Mikhail Kuznetsov, Maxim Piskunov, Gordon Thomson, Sergey Troitsky, and Yana Zhezher, Telescope Array search for EeV photons and neutrinos. PoS, ICRC2017:551, 2018.
ПРНД = 8/8 = 1.0
8. Mikhail Kuznetsov, Maxim Piskunov, Grigory Rubtsov, Sergey Troitsky, and Yana Zhezher, Composition Studies with the Telescope Array surface detector. PoS, ICRC2017:543, 2018.
ПРНД = 8/5 = 1.6
9. Mikhail Kuznetsov, Maxim Piskunov, Grigory Rubtsov, Sergey Troitsky, and Yana Zhezher, Composition Studies with the Telescope Array Surface Detector. JPS Conf. Proc., 19:011035, 2018.
ПРНД = 8/5 = 1.6
Препринты:
1. R. U. Abbasi et al. (Telescope Array collaboration), Evidence for Declination Dependence of Ultrahigh Energy Cosmic Ray Spectrum in the Northern Hemisphere, arXiv:1801.07820.
ПРНД = 3*0.06=0.18
2. R. U. Abbasi et al. (Telescope Array collaboration), Mass composition of ultra-high-energy cosmic rays with the Telescope Array Surface Detector Data, arXiv:1808.03680.
ПРНД = 3*0.06=0.18
3. R. U. Abbasi et al. (Telescope Array collaboration), Constraints on the diffuse photon flux with energies above 10^18 eV using the surface detector of the Telescope Array experiment, arXiv:1811.03920.
ПРНД = 3*0.06=0.18
Доклады:
1. Устный доклад, Mikhail Kuznetsov, Search for ultra high energy photons with the Telescope Array experiment. XXth International Seminar on High Energy Physics Quarks-2108, Valday, Russia, 27 May - 2 June 2018.
https://q2018.inr.ac.ru/event/1/contributions/149/
ПРНД = 25.0
2. Устный доклад, Mikhail Kuznetsov, TeV blazars and the transparency of the Universe. TeV Particle Astrophysics conference (TeVPA 2018), Berlin, Germany, 27-31 August 2018.
https://indico.desy.de/indico/event/18204/session/16/contribution/144
ПРНД = 10.0 + 15.0/2 = 17.5
3. Стендовый доклад, Mikhail Kuznetsov, Search for ultra high energy photons in Telescope Array experiment. 20th International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI-2018), Nagoya, Japan, 21-25 May 2018.
https://indico.cern.ch/event/639198/page/13503-poster-session
ПРНД = 10.0
Итого за 2018: ПРНД = 151.06
Диссертация на соискание степени кандидата физико-математических наук защищена в сентябре 2017: общий повышающий коэффициент равен 1.5.
Итого за 2 года: ПРНД = (270.23 + 151.06) * 1.5 = 631.94