Search for high-energy neutrinos from GW170817 with Baikal-GVD neutrino telescope

Collaboration, Baikal-GVD; D., Avrorin, A.; Avrorin, A. V.; Aynutdinov, V. M.; R., Bannash,; Belolaptikov, I. A.; Brudanin, V. B.; Budnev, N. M.; Дорошенко, А. А.; Domogatsky, G. V.; Dvornický, R.; Dyachok, A. N.; Dzhilkibaev, Zh. -A. M.; Fajt, L.; Fialkovsky, S.V.; Gafarov, A. R.; Golubkov, K. V.; Gres, T. I.; Z., Honz,; Kebkal, K. G.; G., Kebkal, O.; Khramov, E. V.; Kolbin, M. M.; Konischev, K. V.; Korobchenko, A.P.; Koshechkin, A. P.; Kozhin, V. A.; F., Kulepov, V.; Kuleshov, D. A.; B., Milenin, M.; Mirgazov, R. A.; Osipova, E. R.; I., Panfilov, A.; Pan'kov, L. V.; P., Petukhov, D.; Pliskovsky, E. N.; I., Rozanov, M.; Rjabov, E. V.; Rushay, V. D.; Safronov, G. B.; Simkovic, F.; Skurkhin, A. V.; Shoibonov, B.; Solovjev, A. G.; Сороковиков, М. Н.; Shelepov, M. D.; V., Suvorova, O.; Shtekl, I.; Таболенко, В. А.; Tarashansky, B.; Yakovlev, S. A.; V., Zagorodnikov, A.; L., Zurbanov, V.

doi:10.48550/arxiv.1810.10966

Cited by 2 publications

(2 citation statements)

References 6 publications

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“…This will allow one to search for PeVatrons, i.e., galactic objects in which protons are accelerated to energies ~10 14 -10 17 eV, to find the energy limits for particle acceleration in supernova remnants and PWNs, and to carry out a search for correlations with neutrino events detected by the Ice-Cube [3] and Baikal-GVD [4] neutrino observatories.…”

Section: Introductionmentioning

confidence: 99%

The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics

Vaidyanathan,

Astapov,

Bezyazeekov

et al. 2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA astrophysical complex addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV and cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west of the southern tip of lake Baikal. It includes a timing Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over an area of about 1 square kilometer and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of a triangle with side lengths of about 300m, 400m and 500m. There are three approaches to selecting gamma quanta from the hadron background in the TAIGA experiment: (1) IACT operation in standalone mode; (2) Stereo mode operation of two or more IACTs; (3) Hybrid mode operation -joint operation of TAIGA-HiSCORE and IACTs. The main advantage of the hybrid operation of the IACTs and timing is their good gamma/hadron separation, even with only a few telescopes on the large area. Present status of the project, the first experimental results and plans for the future 10-20 km 2 TAIGA are presented.

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Section: Introductionmentioning

confidence: 99%

The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics

Vaidyanathan,

Astapov,

Bezyazeekov

et al. 2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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“…At present time the operating neutrino telescopes focus on the detection of astrophysical high-energy neutrino fluxes: IceCube, a cubic kilometer detector at the South Pole [1,2,3], ANTARES [4,5] located in the Mediterranean Sea, and underwater Baikal Gigaton Volume Detector (Baikal-GVD), a cubic kilometer-scale array, which is currently under construction in lake Baikal [6,7].…”

Section: Introductionmentioning

confidence: 99%

Prompt atmospheric neutrinos in the quark–gluon string model

Sinegovsky

Сороковиков

2020

Eur. Phys. J. C

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We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the D mesons and Λ + c baryons production in pA and πA collisions are calculated in the phenomenological quark-gluon string model (QGSM) which is updated using recent measurements of cross sections of the charmed meson production in the LHC experiments. A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit from the Ice-Cube experiment, as well as with predictions of other charm production models.

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Search for high-energy neutrinos from GW170817 with Baikal-GVD neutrino telescope

Cited by 2 publications

References 6 publications

The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics

The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics

Prompt atmospheric neutrinos in the quark–gluon string model

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