Рейтинг (ПРНД) сотрудников ИЯИ РАН сезона 2022 [312]
по группам: Теоретическая физика, Ядерная физика, Нейтринная физика и КЛ, физика Частиц, Ускорительная физика, Междисциплинарные исследования
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| ФИО | ГР | ПРНД | ПРНД
рук | дата | должн |
| Ткачёв Игорь Иванович | Т | 443,9 | 429,7 | 18.01.2022 | С |
Ткачев Игорь Иванович
Заведующий отделом, доктор физ-мат наук, академик РАН
Публикации
2020
Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector
Telescope Array Collaboration (R.U. Abbasi (Utah U.) et al.).
Published in: J.Exp.Theor.Phys. 131 (2020) 2, 255-264
ПРНД = 60*1.29*0.047 = 3.638
Propagation effects in the FRB 20121102A spectra,
D. G. Levkov, A. G. Panin and I. I. Tkachev,
[arXiv:2010.15145 [astro-ph.HE]].
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.
Published in: PoS ICRC2019 (2020) 310
ПРНД = 8*0.047 =0.376
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.
Published in: Phys.Rev.D 102 (2020) 6, 062004
e-Print: 2006.05012 [astro-ph.HE]
ПРНД = 30*5.296*0.047 = 7.467
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.
Published in: Astrophys.J.Lett. 898 (2020) 2, L28
e-Print: 2007.00023 [astro-ph.HE]
ПРНД = 30*7.413*0.047 = 10.452
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.
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.
Published in: Astrophys.J. 899 (2020) 1, 86
e-Print: 2005.07312 [astro-ph.HE]
ПРНД = 30*5.874*0.047 = 8.282
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.)
Published in: Phys.Rev.D 102 (2020) 2, 023501
e-Print: 2004.05179 [astro-ph.CO]
ПРНД = 30*5.296*0.51 = 81.029
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.
Published in: Mon.Not.Roy.Astron.Soc. 492 (2020) 3, 3984-3993
ПРНД = 30*5.287*0.047 = 7.455
Full-sky searches for anisotropies in UHECR arrival directions with the Pierre Auger Observatory and the Telescope Array
A. di Matteo, et al.
Published in: PoS ICRC2019 (2020) 439
doi:10.22323/1.358.0439
ПРНД = 8*0.047 = 0.376
Updated Results on the UHECR Hotspot Observed by the Telescope Array Experiment,
K. Kawata, et al. [Telescope Array]
PoS ICRC2019 (2020), 310
doi:10.22323/1.358.0310
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.)
Published in: Eur.Phys.J.C 80 (2020) 9, 821
e-Print: arXiv:1911.09633
ПРНД = 30*4.59*0.047 = 6.472
First operation of the KATRIN experiment with tritium
KATRIN Collaboration (M. Aker (KIT, Karlsruhe & KIT, Karlsruhe, IKP) et al.).
Published in: Eur.Phys.J.C 80 (2020) 3, 264
e-Print: arXiv:1909.06069
ПРНД = 30*4.59*0.047 = 6.472
High-resolution spectroscopy of gaseous Kr conversion electrons with the KATRIN experiment
K. Altenmuller (Munich, Tech. U. & IRFU, Saclay) et al..
Published in: J.Phys.G 47 (2020) 6, 065002
e-Print: arXiv:1903.06452
ПРНД = 30*3.045*0.047 = 4.293
2021
Damping signatures at JUNO, a medium-baseline reactor neutrino oscillation experiment,
J. Wang, et al. [JUNO],
[arXiv:2112.14450 [hep-ex]].
ПРНД = 3*0.018 = 0.054
The UHECR dipole and quadrupole in the latest data from the original Auger and TA surface detectors,
P. Tinyakov, et al. [Telescope Array],
PoS ICRC2021 (2021), 375
doi:10.22323/1.395.0375
[arXiv:2111.14593 [astro-ph.HE]].
ПРНД = 8*0.047 = 0.376
UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby
galaxies,
A. di Matteo, et al. [Telescope Array],
PoS ICRC2021 (2021), 308
doi:10.22323/1.395.0308
[arXiv:2111.12366 [astro-ph.HE]].
ПРНД = 8*0.047 = 0.376
Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for
Large-Scale Electric Field Changes,
R. U. Abbasi, et al.
[arXiv:2111.09962 [astro-ph.HE]].
ПРНД = 3*0.047 = 0.141
Indications of a Cosmic Ray Source in the Perseus-Pisces Supercluster,
R. U. Abbasi, et al. [Telescope Array],
[arXiv:2110.14827 [astro-ph.HE]].
ПРНД = 3*0.047 = 0.141
Radioactivity control strategy for the JUNO detector,
A. Abusleme, et al. [JUNO],
JHEP 11 (2021), 102
doi:10.1007/JHEP11(2021)102
[arXiv:2107.03669 [physics.ins-det]]. 8.192
ПРНД = 30*5.81*0.018 = 3.137
First direct neutrino-mass measurement with sub-eV sensitivity,
M. Aker, et al. [KATRIN],
[arXiv:2105.08533 [hep-ex]].
ПРНД = 3*0.047 = 0.141
Precision measurement of the electron energy-loss function in tritium and deuterium gas for the KATRIN
experiment,
M. Aker, et al. [KATRIN],
Eur. Phys. J. C 81 (2021) no.7, 579
doi:10.1140/epjc/s10052-021-09325-z
[arXiv:2105.06930 [physics.ins-det]].
ПРНД = 30*4.59*0.047 = 6.472
JUNO Physics and Detector,
A. Abusleme, et al. [JUNO],
[arXiv:2104.02565 [hep-ex]].
ПРНД = 3*0.018 = 0.054
Instability of rotating Bose stars,
A. S. Dmitriev, D. G. Levkov, A. G. Panin, E. K. Pushnaya and I. I. Tkachev,
Phys. Rev. D 104 (2021) no.2, 023504
doi:10.1103/PhysRevD.104.023504
[arXiv:2104.00962 [gr-qc]].
ПРНД = 30*5.296*0.38 = 60.374
The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS,
A. Abusleme, et al. [JUNO],
[arXiv:2103.16900 [physics.ins-det]].
ПРНД = 3*0.018 = 0.054
JUNO sensitivity to low energy atmospheric neutrino spectra,
A. Abusleme, et al. [JUNO],
Eur. Phys. J. C 81 (2021), 10
doi:10.1140/epjc/s10052-021-09565-z
ПРНД = 30*4.59*0.018 = 2.478
The Design, Construction, and Commissioning of the KATRIN Experiment,
M. Aker, et al. [KATRIN],
JINST 16 (2021), T08015
doi:10.1088/1748-0221/16/08/T08015
[arXiv:2103.04755 [physics.ins-det]].
ПРНД = 30*1.415*0.047 = 1.995
Surface detectors of the TAx4 experiment,
R. U. Abbasi, et al. [Telescope Array],
Nucl. Instrum. Meth. A 1019 (2021), 165726
doi:10.1016/j.nima.2021.165726
[arXiv:2103.01086 [astro-ph.IM]].
ПРНД = 30*1.455*0.047 = 2.052
Mass production and characterization of 3-inch PMTs for the JUNO experiment,
C. Cao, et al.
Nucl. Instrum. Meth. A 1005 (2021), 165347
doi:10.1016/j.nima.2021.165347
[arXiv:2102.11538 [physics.ins-det]].
ПРНД = 30*1.455*0.018 = 0.786
Analysis methods for the first KATRIN neutrino-mass measurement,
M. Aker, et al. [KATRIN],
Phys. Rev. D 104 (2021) no.1, 012005
doi:10.1103/PhysRevD.104.012005
[arXiv:2101.05253 [hep-ex]].
ПРНД = 30*5.296*0.047 = 7.467
Performance and simulation of the surface detector array of the TAx4 experiment,
R. U. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 355
doi:10.22323/1.395.0355
ПРНД = 8*0.047 = 0.376
Cosmic ray energy spectrum in the 2nd knee region measured by the TALE-SD array,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 362
doi:10.22323/1.395.0362
ПРНД = 8*0.047 = 0.376
Cosmic Ray Composition between 2 PeV and 2 EeV measured by the TALE Fluorescence Detector,
T. AbuZayyad, et al. [Telescope Array],
PoS ICRC2021 (2021), 346
doi:10.22323/1.395.0346
ПРНД = 8*0.047 = 0.376
The atmospheric transparency of Telescope Array observation site by the CLF,
T. Tomida, et al. [Telescope Array],
PoS ICRC2021 (2021), 217
doi:10.22323/1.395.0217
ПРНД = 8*0.047 = 0.376
A study of analysis method for the identification of UHECR source type,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 242
doi:10.22323/1.395.0242
ПРНД = 8*0.047 = 0.376
Analysis of TAx4 hybrid trigger and events,
S. Kim, et al. [Telescope Array],
PoS ICRC2021 (2021), 332
doi:10.22323/1.395.0332
ПРНД = 8*0.047 = 0.376
Cosmic Ray Energy Spectrum measured by the TALE Fluorescence Detector,
T. AbuZayyad, et al. [Telescope Array],
PoS ICRC2021 (2021), 347
doi:10.22323/1.395.0347
ПРНД = 8*0.047 = 0.376
Mass composition of Telescope Array's surface detectors events using deep learning,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 384
doi:10.22323/1.395.0384
ПРНД = 8*0.047 = 0.376
FOV direction and image size calibration of Fluorescence Detector using light source on UAV,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 196
doi:10.22323/1.395.0196
ПРНД = 8*0.047 = 0.376
UHECR mass composition from anisotropy of their arrival directions with the Telescope Array SD,
M. Kuznetsov, et al. [Telescope Array],
PoS ICRC2021 (2021), 294
doi:10.22323/1.395.0294
ПРНД = 8*0.047 = 0.376
Effects of Galactic magnetic field on the UHECR anisotropy studies,
K. Kawata, et al. [Telescope Array],
PoS ICRC2021 (2021), 358
doi:10.22323/1.395.0358
ПРНД = 8*0.047 = 0.376
Telescope Array anisotropy summary,
I. Tkachev, et al. [Telescope Array],
PoS ICRC2021 (2021), 392
doi:10.22323/1.395.0392
ПРНД = 8*0.047 = 0.376
Joint analysis of the energy spectrum of ultra-high-energy cosmic rays as measured at the Pierre Auger
Observatory and the Telescope Array,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 337
doi:10.22323/1.395.0337
ПРНД = 8*0.047 = 0.376
JUNO Physics Prospects,
A. Abusleme, et al. [JUNO],
PoS ICRC2021 (2021), 1194
doi:10.22323/1.395.1194
ПРНД = 8*0.018 = 0.144
Current status and prospects of surface detector of the TAx4 experiment,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 203
doi:10.22323/1.395.0203
ПРНД = 8*0.047 = 0.376
Cosmic Ray Composition in the Second Knee Region as Measured by the TALE Hybrid Detector,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 353
doi:10.22323/1.395.0353
ПРНД = 8*0.047 = 0.376
The status of the TALE surface detector array and TALE infill project,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 255
doi:10.22323/1.395.0255
ПРНД = 8*0.047 = 0.376
Study on the cosmic ray intensity variation using scintillation counters for air shower observation,
T. Nonaka, et al. [Telescope Array],
PoS ICRC2021 (2021), 1255
doi:10.22323/1.395.1255
ПРНД = 8*0.047 = 0.376
The measurements of the cosmic ray energy spectrum and the depth of maximum shower development
of Telescope Array Hybrid trigger events,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 305
doi:10.22323/1.395.0305
ПРНД = 8*0.047 = 0.376
Reconstruction of Air Shower Events Measured by the Surface Detectors of the TAx4 Experiment,
H. Jeong, et al. [Telescope Array],
PoS ICRC2021 (2021), 331
doi:10.22323/1.395.0331
ПРНД = 8*0.047 = 0.376
Telescope Array search for EeV photons,
R. Abbasi, et al. [Telescope Array],
PoS ICRC2021 (2021), 864
doi:10.22323/1.395.0864
ПРНД = 8*0.047 = 0.376
The Cosmic-Ray Composition between 2 PeV and 2 EeV Observed with the TALE Detector in Monoclar
Mode,
R. U. Abbasi, et al. [Telescope Array],
Astrophys. J. 909 (2021) no.2, 178
doi:10.3847/1538-4357/abdd30
[arXiv:2012.10372 [astro-ph.HE]].
ПРНД = 30*5.874*0.047 = 8.282
Axion search with BabyIAXO in view of IAXO,
A. Abeln, K. Altenmuller, S. A. Cuendis, E. Armengaud, D. Attie, S. Aune, S. Basso, L. Berge, et al.
PoS ICHEP2020 (2021), 631
doi:10.22323/1.390.0631
[arXiv:2012.06634 [physics.ins-det]].
ПРНД = 8*0.047 = 0.376
A. Abusleme, et al. [JUNO],
Calibration Strategy of the JUNO Experiment,
A. Abusleme, et al. [JUNO],
JHEP 03 (2021), 004
doi:10.1007/JHEP03(2021)004
ПРНД = 30*5.81*0.018 = 3.137
Bound on 3+1 Active-Sterile Neutrino Mixing from the First Four-Week Science Run of KATRIN,
M. Aker, et al. [KATRIN],
Phys. Rev. Lett. 126 (2021) no.9, 091803
doi:10.1103/PhysRevLett.126.091803
ПРНД = 30*9.161*0.047 = 12.917
Conceptual design of BabyIAXO, the intermediate stage towards the International Axion Observatory,
A. Abeln, et al. [IAXO],
JHEP 05 (2021), 137
doi:10.1007/JHEP05(2021)137
[arXiv:2010.12076 [physics.ins-det]].
ПРНД = 30*5.81*0.047 = 8.192
Observations of the Origin of Downward Terrestrial Gamma-Ray Flashes,
T. Abu-Zayyad, et al. [Telescope Array],
JGR Atmospheres 125 (2020) issue 23, 31940
doi:10.1029/2019JD031940
[arXiv:2009.14327 [physics.ao-ph]].
ПРНД = 30*4.261*0.047 = 6.008
Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector,
A. Abusleme, et al. [JUNO],
Nucl. Instrum. Meth. A 988 (2021), 164823
doi:10.1016/j.nima.2020.164823
[arXiv:2007.00314 [physics.ins-det]].
ПРНД = 30*1.455*0.018 = 0.786
Feasibility and physics potential of detecting 8B solar neutrinos at JUNO,
A. Abusleme, et al. [JUNO],
Chin. Phys. C 45 (2021) no.2, 023004
doi:10.1088/1674-1137/abd92a
[arXiv:2006.11760 [hep-ex]].
ПРНД = 30*2.145*0.018 = 1.158
New high-sensitivity searches for neutrons converting into antineutrons and/or sterile neutrons at the
HIBEAM/NNBAR experiment at the European Spallation Source,
A. Addazi, K. Anderson, S. Ansellb, K. S. Babua, J. Cedercall, D. DiJulio, S. Gardiner, P. Geltenbort,
B. Golubev, A. Holley, et al.
J. Phys. G 48 (2021) no.7, 070501
doi:10.1088/1361-6471/abf429 [arXiv:2006.04907 [physics.ins-det]].
ПРНД = 30*3.045*0.07 = 6.395
ИТОГО = 137.99+141.013 = 277,9
Доклады
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
2021
И. Ткачев, Приглашенный доклад “TA anisotropy summary” на международной конференции “37th International Cosmic Ray Conference” (ICRC 2021), 12-23 июля 2021, Берлин, Германия
https://indico.desy.de/event/27991/contributions/102434/
ПРНД=25
Курсы лекций
В МГУ, «Общая теория относительности», 1 семестр в 2020 и 1 семестр в 2021
ПРНД=16
Редактор журнала IJMP D в 2020 и 2021 гг.
https://www.worldscientific.com/page/ijmpd/editorial-board
ПРНД=20
Руководитель заявок РНФ
22-12-00215 Нелинейные объекты в аксионной и аксионоподобной темной материи
21-12-00328 Нелинейные объекты в аксионной темной материи
Руководитель заявок РФФИ
21-52-50011 Исследованиe вопросов происхождения космических лучей сверхвысоких энергий по данным экспериментов Telescope Array и TALE.
ПРНД = 30
Итоговый ПРНД = 443,9