Status of the Baikal-GVD Project

D., Avrorin, A.; Avrorin, A. V.; Aynutdinov, V. M.; Bannasch, R.; Belolaptikov, I. A.; Bogorodsky, D.Yu.; Brudanin, V. B.; Budnev, N. M.; Danilchenko, I. A.; Domogatsky, G. V.; Дорошенко, А. А.; Dyachok, A. N.; Dzhilkibaev, Zh-A.M.; Fialkovsky, S.V.; Gafarov, A. R.; Гапоненко, O. Н.; Golubkov, K. V.; Gress, T. I.; Z., Honz,; Kebkal, K. G.; G., Kebkal, O.; Конищев, К. В.; Konstantinov, E. N.; Коробченко, А. В.; Кошечкин, А. П.; Koshel, F. K.; Kozhin, V. A.; F., Kulepov, V.; Kuleshov, D. A.; Ljashuk, V. I.; B., Milenin, M.; Mirgazov, R. A.; Osipova, E. R.; I., Panfilov, A.; Pankov, L. V.; Perevalov, A.; Pliskovsky, E. N.; Poleshuk, V. A.; I., Rozanov, M.; Rubtsov, V. F.; Rjabov, E. V.; Shaybonov, B. A.; Sheifler, A. A.; Скурихин, А. В.; Smagina, A. A.; V., Suvorova, O.; Tarashchansky, B.; Yakovlev, S. A.; V., Zagorodnikov, A.; Zhukov, V. A.; L., Zurbanov, V.

doi:10.1142/9789814663618_0019

Cited by 4 publications

(5 citation statements)

References 7 publications

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“…The KM3NeT [38] and the BAIKAL-GVD [39] are such kind of experiments; the first will be in the Mediterranean Sea, the second one in Baikal Lake. They will be in the right geographical position to validate the presence of a diffuse galactic neutrino component, thanks to the possibility to use passing muons of relatively low energies.…”

Section: Future Km 3 -Class Telescopes In Northern Hemispherementioning

confidence: 99%

Extragalactic Plus Galactic Model for Icecube Neutrino Events

Palladino

Vissani

2016

ApJ

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The hypothesis that high-energy cosmic neutrinos are power law distributed is critically analyzed. We propose a model with two components that better explains the observations. The extragalactic component of the high-energy neutrino flux has a canonical n -E 2 spectrum while the galactic component has a n -E 2.7 spectrum; both of them are significant. This model has several implications, which can be tested by IceCube and ANTARES over the next several years. Moreover, the existence of a diffuse component, close to the Galactic plane and that yields (20-30)% of IceCube's events, is interesting for the future km 3 neutrino telescopes located in the Northern Hemisphere and for gamma-ray telescopes aiming to measure events up to a few 100 TeV from the southern sky.

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Section: Future Km 3 -Class Telescopes In Northern Hemispherementioning

confidence: 99%

Extragalactic Plus Galactic Model for Icecube Neutrino Events

Palladino

Vissani

2016

ApJ

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“…The basic structural unit of the data acquisition system of Baikal-GVD [6,7] is a section of OMs. A section is a functionally complete unit that includes systems of registration of radiation, calibration systems, and control electronics for the formation of trigger, the signal processing, and data transfer.…”

Section: Data Acquisition Systemmentioning

confidence: 99%

Gigaton Volume Detector in Lake Baikal: status of the project

Domogatsky¹,

Avrorin²,

Avrovin³

et al. 2018

Proceedings of XVII International Workshop on Neutrino Telescopes — PoS(NEUTEL2017)

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Baikal-GVD is a kilometer-scale neutrino telescope under construction in Lake Baikal, which will be formed by multi-megaton subarrays -clusters of strings. A first demonstration cluster "Dubna" has been deployed in 2015 and comprises 192 optical modules (OMs). In 2016 this cluster was upgraded to the baseline configuration which comprises 288 OMs arranged at eight strings. The second full-scale GVD-cluster was deployed and put in operation in 2017. We review the present activity towards the GVD implementation and discuss some selected results obtained with the "Dubna" cluster.

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“…The Baikal-GVD project is a logical extension of the research and development work performed on the last several years by the Baikal Collaboration [1,2,3,4,5,6]. The detection of highenergy neutrinos has been demonstrated with the NT200 telescope.…”

Section: Introductionmentioning

confidence: 99%