TAIGA - an advanced hybrid detector complex for astroparticle physics, cosmic ray physics and gamma-ray astronomy

Буднев, Н.; Kuzmichev, L. A.; Mirzoyan, R.; Астапов, И. И.; Bezyazeekov, P. A.; Blank, Michael; Бородин, А.; Brückner, Martin; Булан, А.; Чиавасса, А.; Dyachok, A.; Gafarov, A.; Garmash, A.; Grebenyuk, V.; Gress, E.; Gress, O.; Гресс, Т.; Grinyuk, A.; Гришин, О.; Horns, D.; Igoshin, A.; Иванова, А.; Ivanova, A.D.; Калмыков, Н. Н.; Киндин, В. В.; Kiryuhin, S.; Кокоулин, Р. П.; Компаниец, К. Г.; Коростелева, Е. Е.; Kozhin, V.; Кравченко, Е. А.; Kryukov, Alexander; Lagutin, Anatoly; Lemeshev, Yu.; Лубсандоржиев, Б.; Лубсандоржиев, Н.; Lukyantsev, D.; Malakhov, S.; Миргазов, Р. Р.; Монхоев, Р.; Osipova, E.; Пахоруков, А.; Pankov, L.; Петрухин, А. А.; Poddubnyi, I.Ya.; Poleschuk, V.; Ponomareva, V. A.; Попеску, М.; Popova, E.; Порелли, А.; Постников, Е.; Prosin, V.; Птускин, В. С.; Пушнин, А.; Райкин, Р. И.; Рубцов, Г.; Ryabov, Eugene V.; Sagan, Y.; Самолига, В.; Сабиров, Б. М.; Силаев, А.; Sidorenkov, A.; Скурихин, А. В.; Slunecka, V.; Sokolov, A.; Сулаков, В. П.; Suvorkin, Y.; Свешникова, Л.; Таболенко, В. А.; Tarashchansky, B.; Ткачев, Л.; Tluczykont, M.; Tanaev, A.; Ternovoy, M.; Togoo, R.; Ушаков, Н.; Vaidyanathan, A.; Волчугов, П.; Воронин, Д.; Wischnewski, R.; Загородников, А.; Zhaglova, A.; Zhurov, D.; Yashin, I. I.

doi:10.22323/1.395.0731

Cited by 5 publications

(7 citation statements)

References 31 publications

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“…Pierre Auger Observatory: FD [53], SD [192], RD (AERA) [179]; Telescope Array: FD [74] ( X max and σ(X max ) are corrected for reconstruction and detector biases same as was done in Ref. [2] except here there is no correction of the energy scale), Cherenkov (TALE) [142]; Yakutsk: Cherenkov [178], RD [182]; Tunka: Cherenkov [177], RD [181]; LOFAR [180]. Systematic uncertainties of the FD measurements at 10 18.5 eV are indicated for the Pierre Auger (red arrows) and Telescope Array (blue arrows) data.…”

Section: Primary Composition Above 1 Eevmentioning

confidence: 99%

“…Efforts will be made to further reduce the uncertainty on the antenna calibration in the future which brings in reach a precision of individual events as well as an absolute accuracy for the energy of better than 10 %. LOFAR [180], Tunka-Rex [181], and Yakutsk-Radio [182]) and compared to world data (Auger FD [53] and SD [192], HiRes/MIA [826], TA [74], TALE [142], Tunka-133 [177], and Yakutsk [178]).…”

Section: Radio Energymentioning

confidence: 99%

“…At very high cosmic-ray energies reaching up to the presumed transition form Galactic to extragalactic cosmic rays, these are, in particular, to arrays dedicated primarily to the observation of TeV to PeV gamma rays: LHAASO [929], which recently started operation in the northern hemisphere in China, and SWGO [930], which is planned in the southern hemisphere in South America. Further progress in this lower energy range will result from new analyses of data from multi-detector experiments such as TAIGA [177] or KASCADE-Grande [931], once better hadronic interaction models will be available.…”

Section: Complementary Experimentsmentioning

confidence: 99%

“…Figure2.10: Mean logarithmic mass obtained from the experimental data on X max using various hadronic models. Pierre Auger Observatory[53], Telescope Array[74], TALE[142], Tunka-133[177], Yakutsk[178].…”

mentioning

confidence: 99%

“…Figure 6.7: Measurements of the mean of the X max distribution by radio experiments (AERA[179], LOFAR[180], Tunka-Rex[181], and Yakutsk-Radio[182]) and compared to world data (Auger FD[53] and SD[192], HiRes/MIA[826], TA[74], TALE[142], Tunka-133[177], and Yakutsk[178]). The statistical uncertainties are plotted as error bars and for radio the systematic uncertainties as bands if available.…”

mentioning

confidence: 99%

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Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Coleman,

Eser,

Mayotte

et al. 2022

Preprint

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Pin down the shower energy observable to use μ as a composition-only Reduce hadronic uncertainties interaction model E threshold (TBD) Other messengers Galactic * μ / em separation † * depending on analysis progress † depending on detector configuration• At least one next-generation experiment needs to be able to make high-precision measurements to explore new particle physics and measure particle rigidity on an event-by-event basis. Of the planned next-generation experiments, GCOS is the best positioned to meet this recommendation.• As a complementary effort, experiments with sufficient exposure ( 5 × 10 5 km 2 sr yr) are needed to search for Lorentz-invariance violation (LIV), SHDM, and other BSM physics at the Cosmic and Energy Frontiers, and to identify UHECR sources at the highest energies.• Full-sky coverage with low cross-hemisphere systematic uncertainties is critical for astrophysical studies. To this end, next generation experiments should be space-based or multi-site. Common sites between experiments are encouraged.• Based on the productive results from inter-collaboration and inter-disciplinary work, we recommend the continued progress/formation of joint analyses between experiments and with other intersecting fields of research (e.g., magnetic fields).• The UHECR community should continue its efforts to advance diversity, equity, inclusion, and accessibility. It also needs to take steps to reduce its environmental impacts and improve open access to its data to reduce the scientific gap between countries.vi

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Section: Primary Composition Above 1 Eevmentioning

confidence: 99%

Section: Radio Energymentioning

confidence: 99%

Section: Complementary Experimentsmentioning

confidence: 99%

mentioning

confidence: 99%

mentioning

confidence: 99%

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Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Coleman,

Eser,

Mayotte

et al. 2022

Preprint

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PeV proton acceleration in gamma-ray binaries

Bykov,

Petrov,

Ponomaryov

et al. 2024

Advances in Space Research

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TAIGA - An advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy

Budnev,

Astapov,

Bezyazeekov

et al. 2023

SciPost Phys. Proc.

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The physical motivations, present status, main results in study of cosmic rays and in the field of gamma-ray astronomy as well future plans of the TAIGA-1 (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA observatory addresses ground-based gamma-ray astronomy and astroparticle physics at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west from the southern tip of the lake Baikal.

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TAIGA - an advanced hybrid detector complex for astroparticle physics, cosmic ray physics and gamma-ray astronomy

Abstract: The physical motivations, present status, main results in study of cosmic rays and in the field 1

Cited by 5 publications

References 31 publications

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

PeV proton acceleration in gamma-ray binaries

TAIGA - An advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy

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