Рейтинг (ПРНД) сотруднков ИЯИ РАН сезона 23 [309]

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ФИОГРПРНДПРНД
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Ткачёв Игорь ИвановичТ412,6433,213.01.2023С
Ткачев Игорь Иванович
Заведующий отделом, доктор физ-мат наук, академик РАН

Публикации
2021

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

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*6,379*0,018 = 3.445

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*4.991*0.047 = 7,037

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*5.407*0.38 = 61,64
The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS,
A. Abusleme, et al. [JUNO],
Eur. Phys. J. C 81 (2021) no.11, 973
doi:10.1140/epjc/s10052-021-09544-4
ПРНД = 30*4.991*0.018 = 2.695

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*4.991*0.018 = 2.695

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*1.121*0.047 = 1.58

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*1.335*0.047 = 1,882

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*1.335*0.018 = 0.721

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*5.407*0.047 = 7.624

!!! 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*5.521*0.047 = 7,785

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*6,379*0.018 = 3.445

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*9.185*0.047 = 12.95

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*6,3791*0.047 = 8.994

Observations of the Origin of Downward Terrestrial Gamma-Ray Flashes,
T. Abu-Zayyad, et al. [Telescope Array],
JGR Atmospheres 125 (2021) 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*1.335*0.018 = 0.721

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*2.944*0.018 = 1.59

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*3.519*0.07 = 7,39

ИТОГО 2021 = 147.125

2022

JUNO Physics and Detector,
A. Abusleme, et al. [JUNO],
Prog. Part. Nucl. Phys. 123 (2022), 103927
doi:10.1016/j.ppnp.2021.103927
ПРНД = 30*12.425*0.018 = 6.71

First direct neutrino-mass measurement with sub-eV sensitivity,
M. Aker, et al. [KATRIN],
Nature Phys. 18 (2022) no.2, 160-166
doi:10.1038/s41567-021-01463-1
ПРНД = 30*19.684*0.047 = 27.754

Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for
Large-Scale Electric Field Changes,
R. U. Abbasi, et al.
Phys. Rev. D 105 (2022) no.6, 062002
doi:10.1103/PhysRevD.105.062002
ПРНД = 30*5.407*0.047 = 7.624

Damping signatures at JUNO, a medium-baseline reactor neutrino oscillation experiment,
J. Wang, et al. [JUNO],
JHEP 06 (2022), 062
doi:10.1007/JHEP06(2022)062
ПРНД = 30*6.379*0.018 = 3.445

Propagation effects in the FRB 20121102A spectra,
D. G. Levkov, A. G. Panin and I. I. Tkachev,
[arXiv:2010.15145 [astro-ph.HE]].
Astrophys.J. 925 (2022) 2, 109
ПРНД = 30*5.521*0.51 = 84.471

JUNO Sensitivity on Proton Decay $p\to \bar\nu K^+$ Searches,'
A. Abusleme et al. [JUNO],
[arXiv:2212.08502 [hep-ex]].
ПРНД = 3*0.018 = 0.054

Caustic-like Structures in UHECR Flux after Propagation in Turbulent Intergalactic Magnetic Fields,
K .Dolgikh, A. Korochkin, G. Rubtsov, D. Semikoz and I. Tkachev,
[arXiv:2212.01494 [astro-ph.HE]].
ПРНД = 3*0.38 = 1.14

Model Independent Approach of the JUNO $^8$B Solar Neutrino Program,
J. Zhao et al. [JUNO],
[arXiv:2210.08437 [hep-ex]].
ПРНД = 3*0.018 = 0.054

Entanglement of annihilation photons,
A. Ivashkin, D. Abdurashitov, A. Baranov, F. Guber, S. Morozov, S. Musin, A. Strizhak and I. Tkachev,
[arXiv:2210.07623 [quant-ph]].
ПРНД = 3*0.3*2 = 1.8


Search for Lorentz-Invariance Violation with the first KATRIN data,
M. Aker et al. [KATRIN],
[arXiv:2207.06326 [nucl-ex]].
ПРНД = 3*0.047 = 0.141

Search for keV-scale Sterile Neutrinos with first KATRIN Data,
M. Aker et al. [KATRIN],
[arXiv:2207.06337 [nucl-ex]].
ПРНД = 3*0.047 = 0.141

Prospects for detecting the diffuse supernova neutrino background with JUNO,
A. Abusleme et al. [JUNO],
JCAP 10 (2022), 033
doi:10.1088/1475-7516/2022/10/033
[arXiv:2205.08830 [hep-ex]].
ПРНД = 30*7.28*0.018 = 3.931

Mass testing and characterization of 20-inch PMTs for JUNO,
A. Abusleme et al. [JUNO],
Eur. Phys. J. C 82 (2022) no.12, 1168
doi:10.1140/epjc/s10052-022-11002-8
[arXiv:2205.08629 [physics.ins-det]].
ПРНД = 30*4.991*0.018 = 2.695

First High-speed Camera Observations of the Optical Counterpart of a Terrestrial Gamma-ray Flash,
R.U. Abbasi et al. [Telescope Array],
[arXiv:2205.05115 [physics.ao-ph]].
ПРНД = 3*0.047 = 0.141

Sub-percent precision measurement of neutrino oscillation parameters with JUNO,
A. Abusleme et al. [JUNO],
Chin. Phys. C 46 (2022) no.12, 123001
doi:10.1088/1674-1137/ac8bc9
[arXiv:2204.13249 [hep-ex]].
ПРНД = 30*2.944*0.018 = 1.59

Highlights from the Telescope Array experiment,
R.U. Abbasi et al. [Telescope Array],
PoS ICRC2021 (2022), 012
doi:10.22323/1.395.0012
ПРНД = 8*0.047 = 0.376

KATRIN: status and prospects for the neutrino mass and beyond,
M. Aker et al. [KATRIN],
J. Phys. G 49 (2022) no.10, 100501
doi:10.1088/1361-6471/ac834e
[arXiv:2203.08059 [nucl-ex]].
ПРНД = 30*3.519*0.047 = 4.962

High Energy Physics Opportunities Using Reactor Antineutrinos,
C. Awe et al. [JUNO],
[arXiv:2203.07214 [hep-ex]].
ПРНД = 3*0.018 = 0.054

Setup of Compton polarimeters for measuring entangled annihilation photons,
D. Abdurashitov, A. Baranov, D. Borisenko, F. Guber, A. Ivashkin, S. Morozov, S. Musin, A. Strizhak, I. Tkachev and V. Volkov, et al.
JINST 17 (2022) no.03, P03010
doi:10.1088/1748-0221/17/03/P03010
[arXiv:2204.04692 [physics.ins-det]].
ПРНД = 30*1.121*0.2*2 = 13.452

New Constraint on the Local Relic Neutrino Background Overdensity with the First KATRIN Data Runs,
M. Aker et al. [KATRIN],
Phys. Rev. Lett. 129 (2022) no.1, 011806
doi:10.1103/PhysRevLett.129.011806
[arXiv:2202.04587 [nucl-ex]].
ПРНД = 30*9.185*0.047 = 12.95

Improved eV-scale sterile-neutrino constraints from the second KATRIN measurement campaign,
M. Aker et al. [KATRIN],
Phys. Rev. D 105 (2022) no.7, 072004
doi:10.1103/PhysRevD.105.072004
[arXiv:2201.11593 [hep-ex]].
ПРНД = 30*5.407*0.047 = 7.624

Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays,
A. Albert et al. [IceCube, Pierre Auger, Telescope Array, Auger and ANTARES],
Astrophys. J. 934 (2022) no.2, 164
doi:10.3847/1538-4357/ac6def
[arXiv:2201.07313 [astro-ph.HE]].
ПРНД = 30*5.521*0.018 = 2.981

В поисках темной материи,
И. Ткачев, И. Харичев,
Знание-сила, 11 (2022) 4-31
ПРНД = 8*0.65*2 = 10.4

ИТОГО 2022 = 194.49
ИТОГО = 147.135 + 194.49 = 341.625

Доклады

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 2021 и 1 семестр в 2022
ПРНД=16

Редактор журнала IJMP D в 2021 и 2022 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

ПРНД = 10

Итоговый ПРНД = 412,625