prnd 2021

Рейтинг (ПРНД) сотрудников ИЯИ РАН сезона 2021 [306]

по группам: Теоретическая физика, Ядерная физика, Нейтринная физика и КЛ, физика Частиц, Ускорительная физика, Междисциплинарные исследования

ФИО	ГР	ПРНД	дата
Ткачёв Игорь Иванович	Т	390,6	20.01.2021

Ткачев Игорь Иванович
Заведующий отделом, доктор физ-мат наук, академик РАН

Публикации
2019

An improved upper limit on the neutrino mass from a direct kinematic method by KATRIN
KATRIN Collaboration (M. Aker (KIT, Karlsruhe, IKP & KIT, Karlsruhe) et al.). Sep 13, 2019. 10 pp.
Published in Phys.Rev.Lett. 123 (2019) no.22, 221802
DOI: 10.1103/PhysRevLett.123.221802
e-Print: arXiv:1909.06048
ПРНД = 30*8.385*0.047 = 11.823
Measurements with a TRISTAN prototype detector system at the "Troitsk nu-mass" experiment in integral and differential mode
Tim Brunst (Tech. U., Munich (main) & Munich, Max Planck Inst.) et al.. (25) Sep 6, 2019. 17 pp.
Published in JINST 14 (2019) no.11, P11013
DOI: 10.1088/1748-0221/14/11/P11013
e-Print: arXiv:1909.02898
ПРНД = 30*1.454*0.125*1.5 = 8.179
TA Anisotropy Summary
Telescope Array Collaboration (K. Kawata (Tokyo U., ICRR) et al.). 2019. 7 pp.
Published in EPJ Web Conf. 210 (2019) 01004
DOI: 10.1051/epjconf/201921001004
ПРНД = 8*0.047 =0.376
Covering the celestial sphere at ultra-high energies: Full-sky cosmic-ray maps beyond the ankle and the flux suppression
Pierre Auger and Telescope Array Collaborations (J. Biteau (Orsay, IPN) et al.). May 10, 2019. 9 pp.
Published in EPJ Web Conf. 210 (2019) 01005
DOI: 10.1051/epjconf/201921001005
Conference: C18-10-08.1 Proceedings
e-Print: arXiv:1905.04188
ПРНД = 8*0.047 =0.376
Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector
Telescope Array Collaboration (R.U. Abbasi (Utah U.) et al.). May 9, 2019. 10 pp.
Published in: J.Exp.Theor.Phys. 131 (2020) 2, 255-264
e-Print: arXiv:1905.03738
ПРНД = 60*1.152*0.047 = 3.249
Physics potential of the International Axion Observatory (IAXO)
IAXO Collaboration (E. Armengaud (IRFU, Saclay) et al.). Apr 19, 2019. 82 pp.
Published in JCAP 1906 (2019) 047
DOI: 10.1088/1475-7516/2019/06/047
e-Print: arXiv:1904.09155
ПРНД = 30*5.21*0.047 = 7.346
Gamma-induced background in the KATRIN main spectrometer
KATRIN Collaboration (K. Altenmuller (Munich, Tech. U. & IRFU, Saclay) et al.). Mar 1, 2019. 11 pp.
Published in Eur.Phys.J. C79 (2019) no.9, 807
DOI: 10.1140/epjc/s10052-019-7320-4
e-Print: arXiv:1903.00563
ПРНД = 30*4.389*0.047 = 6.188
Constraints on the diffuse photon flux with energies above 10^18 eV using the surface detector of the Telescope Array experiment,
Telescope Array Collaboration, R.U. Abbasi(Utah U.) et al. (Nov 9, 2018)
Published in: Astropart.Phys. 110 (2019) 8-14
ПРНД = 30*2.61*0.047 = 3.68
Mass composition of ultrahigh-energy cosmic rays with the Telescope Array Surface Detector data
Telescope Array Collaboration, R.U. Abbasi(Utah U.) et al. (Aug 10, 2018)
Published in: Phys.Rev.D 99 (2019) 2, 022002
ПРНД = 30*4.833*0.047 = 6.815

Muon-induced background in the KATRIN main spectrometer
KATRIN Collaboration, K. Altenmuller(Munich, Tech. U.) et al. (May 30, 2018)
Published in: Astropart.Phys. 108 (2019) 40-49
ПРНД = 30*2.61*0.047 = 3.68
2020

Calibration Strategy of the JUNO Experiment
JUNO Collaboration, Angel Abusleme (Chile U., Catolica) et al. (Nov 12, 2020)
e-Print: 2011.06405 [physics.ins-det]
ПРНД = 3*0.047 = 0.141
Bound on 3+1 active-sterile neutrino mixing from the first four-week science run of KATRIN
KATRIN Collaboration, M. Aker (KIT, Karlsruhe) et al. (Nov 10, 2020)
e-Print: 2011.05087 [hep-ex]
ПРНД = 3*0.047 = 0.141
Periodic structure in the FRB 121102 spectra
D.G. Levkov, A.G. Panin, I.I. Tkachev (Oct 28, 2020)
e-Print: 2010.15145 [astro-ph.HE]
ПРНД = 3*0.51 = 1.53
Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory
BabyIAXO Collaboration, A. Abeln (Kirchhoff Inst. Phys.) et al. (Oct 22, 2020)
e-Print: 2010.12076 [physics.ins-det]
ПРНД = 3*0.047 = 0.141
Observations of the Origin of Downward Terrestrial Gamma-Ray Flashes
Telescope Array Collaboration, T. Abu-Zayyad et al. (Sep 29, 2020)
e-Print: 2009.14327 [physics.ao-ph]
ПРНД = 3*0.047 = 0.141
Updated Results on the UHECR Hotspot Observed by the Telescope Array Experiment
Telescope Array Collaboration, Kazumasa Kawata et al. (Sep 28, 2020)
Published in: PoS ICRC2019 (2020) 310 • Contribution to: ICRC 2019, 310
ПРНД = 8*0.047 =0.376
Search for Large-scale Anisotropy on Arrival Directions of Ultra-high-energy Cosmic Rays Observed with the Telescope Array Experiment
Telescope Array Collaboration, R.U. Abbasi (Illinois U., Chicago) et al. (Jul 2, 2020)
Published in: Astrophys.J.Lett. 898 (2020) 2, L28
e-Print: 2007.00023 [astro-ph.HE]
ПРНД = 30*8.198*0.047 = 11.559
Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector
JUNO and Daya Bay Collaborations, A. Abusleme(Chile U., Catolica) et al. (Jul 1, 2020)
Published in: Nucl.Instrum.Meth.A 988 (2021) 164823
e-Print: 2007.00314 [physics.ins-det]
ПРНД = 30*1.265*0.018 = 0.6831
Feasibility and physics potential of detecting 8B solar neutrinos at JUNO
JUNO Collaboration, Angel Abusleme(Chile U., Catolica) et al. (Jun 21, 2020)
e-Print: 2006.11760 [hep-ex]
ПРНД = 3*0.018 = 0.054

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
Telescope Array Collaboration, R.U. Abbasi (Illinois U., Chicago) et al. (Jun 9, 2020)
Published in: Phys.Rev.D 102 (2020) 6, 062004
e-Print: 2006.05012 [astro-ph.HE]
ПРНД = 30*4.833*0.047 = 6.815
New high-sensitivity searches for neutrons converting into antineutrons and/or sterile neutrons at the European Spallation Source
A. Addazi et al. (Jun 8, 2020)
e-Print: 2006.04907 [physics.ins-det]
ПРНД = 3*0.07 = 0.21

TAO Conceptual Design Report: A Precision Measurement of the Reactor Antineutrino Spectrum with Sub-percent Energy Resolution
JUNO Collaboration, Angel Abusleme(Chile U., Catolica) et al. (May 18, 2020)
e-Print: 2005.08745 [physics.ins-det]
ПРНД = 3*0.018 = 0.054
Evidence for a Supergalactic Structure of Magnetic Deflection Multiplets of Ultra-High Energy Cosmic Rays
Telescope Array Collaboration, R.U. Abbasi(Loyola U., Chicago) et al. (May 15, 2020)
Published in: Astrophys.J. 899 (2020) 1, 86
e-Print: 2005.07312 [astro-ph.HE]
ПРНД = 30*5.745*0.047 = 8.1
Radio-emission of axion stars
D.G. Levkov(Moscow, INR and ITMP, Moscow), A.G. Panin(Moscow, INR and Moscow, MIPT), I.I. Tkachev(Moscow, INR and Novosibirsk State U.) (Apr 10, 2020)
Published in: Phys.Rev.D 102 (2020) 2, 023501
e-Print: 2004.05179 [astro-ph.CO]
ПРНД = 30*4.833*0.51 = 73.945
Search for point sources of ultra-high-energy photons with the Telescope Array surface detector
Telescope Array Collaboration, R.U. Abbasi(Utah U.) et al. (Feb 19, 2020)
Published in: Mon.Not.Roy.Astron.Soc. 492 (2020) 3, 3984-3993
ПРНД = 30*5.536*0.047 = 7.806
Full-sky searches for anisotropies in UHECR arrival directions with the Pierre Auger Observatory and the Telescope Array
Pierre Auger and Telescope Array Collaborations, A. di Matteo(INFN, Turin) et al. (Jan 7, 2020)
Published in: PoS ICRC2019 (2020) 439 • Contribution to: ICRC 2019, 439 • e-Print: 2001.01864 [astro-ph.HE]
ПРНД = 8*0.047 =0.376
Suppression of Penning discharges between the KATRIN spectrometers
KATRIN Collaboration (M. Aker (KIT, Karlsruhe & KIT, Karlsruhe, IKP) et al.). Nov 21, 2019.
Published in: Eur.Phys.J.C 80 (2020) 9, 821
e-Print: arXiv:1911.09633
ПРНД = 30*4.389*0.047 = 6.188
First operation of the KATRIN experiment with tritium
KATRIN Collaboration (M. Aker (KIT, Karlsruhe & KIT, Karlsruhe, IKP) et al.). Sep 13, 2019. 19 pp.
Published in: Eur.Phys.J.C 80 (2020) 3, 264
e-Print: arXiv:1909.06069
ПРНД = 30*4.389*0.047 = 6.188
High-resolution spectroscopy of gaseous Kr conversion electrons with the KATRIN experiment
K. Altenmuller (Munich, Tech. U. & IRFU, Saclay) et al.. Mar 15, 2019. 9 pp.
Published in: J.Phys.G 47 (2020) 6, 065002
e-Print: arXiv:1903.06452
ПРНД = 30*2.415*0.047 = 3.405
ИТОГО = 179.565

Доклады

2019
И. Ткачев, Приглашенный доклад "Axion stars: formation and collapse" на международном Солвеевском симпозиуме "The Dark Side of Black Holes" (Брюссель, Бельгия, 3-5 апреля 2019).
http://www.solvayinstitutes.be/event/workshop/dark_2019/dark_2019.html
ПРНД=25

И. Ткачев, Приглашенный пленарный доклад "Axion stars: from birth to death" на XXIV-ой международной конференции “High Energy Physics and Quantum Field Theory” (Сочи, 22 — 29 сентября 2019 ).
https://qfthep.sinp.msu.ru/programme
ПРНД=25

2020
И. Ткачев, Приглашенный доклад “Theory and phenomenology of axion miniclusters”, на международной конференции “Axion cosmology” (17 февраля - 13 марта 2020, Мюнхен, Германия),
https://www.munich-iapp.de/activities/activities-2020/2020-1
ПРНД=25

И. Ткачев, Приглашенный доклад "Axion stars and their possible astrophysical manifestations", на международной конференции "Less travelled path of dark matter: axions and primordial black holes", 9 – 13 ноября 2020, Бенгалор, Индия
https://www.icts.res.in/program/ltpdm2020/talks
ПРНД=25

И. Ткачев, Приглашенный доклад “Аксионы как темная материя", на рабочем совещании "Темная материя: теоретические предложения и экспериментальные поиски", 22 октября 2020, Дубна, Россия
http://www.jinr.ru/posts/rabochee-soveshhanie-temnaya-materiya-teoreticheskie-predlozheniya-i-eksperimentalnye-poiski/
ПРНД=25

Курсы лекций в МГУ, «Общая теория относительности», 1 семестр в 2019 и 1 семестр в 2020
ПРНД=16

Редактор журнала IJMP D в 2019 и 2020 гг.
https://www.worldscientific.com/page/ijmpd/editorial-board
ПРНД=20

Руководитель заявок РНФ
21-12-00328 Нелинейные объекты в аксионной темной материи
Руководитель заявок РФФИ
19-52-50019 Исследование вопросов происхождения космических лучей сверхвысоких энергий на установке Telescope Array.

20-52-50017 Исследованиe вопросов происхождения космических лучей сверхвысоких энергий на установке Telescope Array.

21-52-50011 Исследованиe вопросов происхождения космических лучей сверхвысоких энергий по данным экспериментов Telescope Array и TALE.

Ответственный исполнитель заявок РНФ

19-42-02004 Космологическая тёмная материя, первичные чёрные дыры, конденсаты Бозе-Эйнштейна и зарядовая асимметрия Вселенной

20-42-09010 Открытие новых окон в раннюю Вселенную с помощью многоканальной астрономии

ПРНД = 50

Итоговый ПРНД = 390.565