Baikal_Deep_Underwater_Neutrino_Telescope

Baikal Deep Underwater Neutrino Telescope

Baikal Deep Underwater Neutrino Telescope

Observatory

The Baikal Deep Underwater Neutrino Telescope (BDUNT) (Russian: Байкальский подводный нейтринный телескоп) is a neutrino detector conducting research below the surface of Lake Baikal (Russia) since 2003.[1] The first detector was started in 1990 and completed in 1998. It was upgraded in 2005 and again starting in 2015 to build the Baikal Gigaton Volume Detector (Baikal-GVD.)[2] BDUNT has studied neutrinos coming through the Earth with results on atmospheric muon flux. BDUNT picks up many atmospheric neutrinos created by cosmic rays interacting with the atmosphere – as opposed to cosmic neutrinos which give clues to cosmic events and are therefore of greater interest to physicists.

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Detector history

The start of the Baikal neutrino experiment dates back to 1 October 1980, when a laboratory of high-energy neutrino astrophysics was established at the Institute for Nuclear Research of the former Academy of Sciences of the USSR in Moscow. This laboratory would become the core of the Baikal collaboration.

The original NT-200 design was deployed in stages 3.6 km from shore at a depth of 1.1 km.

The first part, NT-36 with 36 optical modules (OMs) at 3 short strings, was put into operation and took data up to March 1995.[3] NT-72 ran 1995–1996 then was replaced by the four-string NT-96 array.[4] Over its 700 days of operation, 320,000,000 muon events were collected with NT-36, NT-72, and NT-96. Beginning April 1997, NT-144, a six-string array took data. The full NT-200 array with 192 modules was completed April 1998.[5] In 2004–2005 it was updated to NT-200+ with three additional strings around NT-200 at distance of 100 meters, each with 12 modules.[6][7]

Baikal-GVD

Since 2016, a 1 cubic km telescope, NT-1000 or Baikal-GVD (or just GVD, Gigaton Volume Detector), is being built.[8] The first stage of 3 strings was switched on in April 2013.[9][2] During 2015 the GVD demonstration cluster (also known as Dubna) with 192 optical modules was successfully operated. This concluded the preparatory phase of the project. In 2016 the construction of the first phase of the telescope began with the demonstration cluster being upgraded to the baseline configuration for a single cluster, with 288 OMs on eight vertical strings.[10] The first phase of the telescope, when completed, is expected to contain 8 such clusters. This first phase was expected to be completed around 2020.

As of 2018, the Baikal telescope continued to operate and to be developed.[11]

On 13 March 2021, the first phase of the telescope, GVD-I, was completed. It consisted of 8 clusters of 288 OMs each, and had a volume of about half a cubic kilometre. In the years to come the telescope will be expanded to measure one cubic kilometre (the full planned size).[12] The project's cost (for the GVD-I phase) was about 2.5 billion Russian rubles (about 34 million $USD).[13]

Results

BDUNT has used its neutrino detector to study astrophysical phenomena. Searches for relic dark matter in the Sun[14] and high-energy muons[15] and neutrinos[16] have been published.

See also

References

  1. [1]
    "Icy life working with Russia's underwater 'cosmic eye'". BBC News. 24 September 2010. Retrieved 18 February 2011.
  2. [2]
    "A new neutrino telescope for Lake Baikal – CERN Courier". 22 July 2015.
  3. [3]
    Belolaptikov, I. A. (1995). "Results from the Baikal Underwater Telescope" (PDF). Nuclear Physics B: Proceedings Supplements. 43 (1–3): 241–244. Bibcode:1995NuPhS..43..241B. doi:10.1016/0920-5632(95)00481-N.
  4. [4]
    Belolaptikov, I. A.; et al. (1997). "The Baikal underwater neutrino telescope: Design, performance, and first results". Astroparticle Physics. 7 (3): 263–282. Bibcode:1997APh.....7..263B. doi:10.1016/S0927-6505(97)00022-4.
  5. [5]
    "Baikal Lake Neutrino Telescope". Baikalweb. 6 January 2005. Archived from the original on 31 August 2010. Retrieved 30 July 2008.
  6. [6]
    Aynutdinov, V.; et al. (2005). "The Baikal neutrino experiment: From NT200 to NT200+". Proceedings of the 29th International Cosmic Ray Conference. 5: 75. Bibcode:2005ICRC....5...75A.
  7. [7]
    Wischnewski, R.; et al. (Baikal Collaboration) (2005). "The Baikal Neutrino Telescope – Results and Plans". International Journal of Modern Physics A. 20 (29): 6932–6936. arXiv:astro-ph/0507698. Bibcode:2005IJMPA..20.6932W. doi:10.1142/S0217751X0503051X. S2CID 118897977.
  8. [8]
    Avrorin, A. V.; et al. (2011). "An Experimental String of the NT1000 Baikal Neutrino Telescope" (PDF). Instruments and Experimental Techniques. 54 (5): 649–659. doi:10.1134/S0020441211040178. S2CID 55191305.
  9. [9]
    Avrorin, A. V.; et al. (2014). "Data acquisition system of the NT1000 Baikal neutrino telescope". Instruments and Experimental Techniques. 57 (3): 262–273. doi:10.1134/S002044121403004X. S2CID 121619985.
  10. [10]
    Avrorin, A.D.; et al. (2017). "Baikal-GVD". EPJ Web of Conferences. 136: 04007. Bibcode:2017EPJWC.13604007A. doi:10.1051/epjconf/201713604007.
  11. [11]
    Kouchner fskbhe1.puk.ac.za
  12. [12]
    "Russia deploys giant space telescope in Lake Baikal". 13 March 2021.
  13. [13]
    "Largest neutrino telescope in the Northern hemisphere commissioned at lake Baikal".
  14. [14]
    Avrorin, A.D.; et al. (2015). "Search for neutrino emission from relic dark matter in the Sun with the Baikal NT200 detector". Astroparticle Physics. 62: 12–20. arXiv:1405.3551. Bibcode:2015APh....62...12A. doi:10.1016/j.astropartphys.2014.07.006. S2CID 108287298.
  15. [15]
    Wischnewski, R.; et al. (2005). "The Baikal Neutrino Telescope – Results and Plans". International Journal of Modern Physics A. 20 (29): 6932–6936. arXiv:astro-ph/0507698. Bibcode:2005IJMPA..20.6932W. doi:10.1142/S0217751X0503051X. S2CID 118897977.
  16. [16]
    Aynutdinov, V.; et al. (BAIKAL Collaboration) (2006). "Search for a Diffuse Flux of High-Energy Extraterrestrial Neutrinos with the NT200 Neutrino Telescope". Astroparticle Physics. 25 (2): 140–150. arXiv:astro-ph/0508675. Bibcode:2006APh....25..140A. doi:10.1016/j.astropartphys.2005.12.005. S2CID 119499665.
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