The Baksan Neutrino Observatory (BNO; Baksan is sometimes spelled Baxan) is a scientific laboratory of INR RAS located in the Baksan River gorge in the Caucasus mountains in Russia.[1] Cleared for building in 1967, it started operations in 1977, becoming the first such neutrino observatory in the USSR.[2] It consists of the Baksan Underground Scintillation Telescope (BUST), located 300 m (980 ft) below the surface,[3] the gallium–germanium neutrino telescope (Soviet–American Gallium Experiment, SAGE) located 4,700 m.w.e. deep[3] (2100 meters) as well as a number of ground facilities. The Baksan Experiment on Sterile Transitions (BEST) is currently (2019) being conducted at Baksan with aims of understanding sterile neutrinos. [1]
The laboratory itself is located in a 4000 meter long horizontal tunnel mined specifically for this purpose; this is in contrast to most underground physics laboratories which are placed in abandoned or still in-use mines. The entrance of the tunnel is at a valley at 1700 meters high from sea level and the tunnel itself is located under the 4000 meters tall mountain Mount Andyrchi. A small town of Neutrino was constructed in the valley in conjunction with the construction of the laboratory to house the scientists and their families.
The first experiment undertaken at BNO was not underground; it was the Carpet air-shower cosmic ray experiment in 1973. Carpet relied on liquid scintillator detectors to study cosmic ray air-showers. Carpet also made discoveries of astrophysical importance, such as detecting a giant flare in the Crab Nebula in 1989. The Carpet cosmic ray experiment continues as of 2017, and it is being upgraded in to gamma ray telescope. Further upgrades are also planned.
The first underground experiment, the BUST started operations in 1977. It is located 550 meters from the tunnel entrance. It detected neutrinos from the SN1987A supernova. It continues to operate (as of 2017).
The next experiment at BNO was the Gallium-Germanium Neutrino Telescope (GGNT) as part of the SAGE experiment. It started operation 1986. It is located 3500 meters from the tunnel entrance. It continues to operate (as of 2017).
In addition to the big experiments BUST and SAGE, a number of smaller experiments that benefit from the low-background location have taken place at BNO; for example, the isotopic composition of the lunar samples brought by Luna-16, Luna-20 and Luna-24 spacecraft was measured in BNO.
BNO is also home to the Andyrchi air-shower array, located on the surface above BUST in the mountain slope. The array and BUST work in coincidence. BNO hosts also a small gravitational-wave detector, OGRAN. OGRAN would be capable of registering a galactic supernova, should one occur in the Milky Way.
The BNO-observatory is planning (as of 2017) a new major detector, the Baksan Large Underground Neutrino Telescope (BLUNT). This detector would consist of huge (10-20 kilotonnes) amounts of liquid scintillator. It would be located at the end of the laboratory tunnel. It would mainly detect neutrinos.
As of 2017, the director of the observatory is Valery Kuzminov.[4]
See also
Baikal Deep Underwater Neutrino Telescope
IceCube Neutrino Observatory
References
Overbye, Dennis (16 July 2018). "The Neutrino Trappers - Deep in a mountain in southern Russia, scientists are tracking one of the universe's most elusive particles". The New York Times. Archived from the original on 17 July 2018. Retrieved 17 July 2018.
"Archived copy" Подземная охота за нейтрино: Уеные ловят призраков, которые запросто проходят сквозь земной шар, Trud (in Russian) (211), 23 November 2002, archived from the original on 16 September 2018, retrieved 17 July 2018
"Baksan Neutrino Observatory". Institute for Nuclear Research. 2001. Archived from the original on 25 September 2006. Retrieved 25 July 2006.
"Baksan scales new neutrino heights – CERN Courier". 19 May 2017. Archived from the original on 16 December 2018. Retrieved 31 January 2019.
External links
Photographs of the Baskan Observatory via englishrussia.com
Photographs of the Baskan Observatory via nytimes.com
vte
Underground physics laboratories (m of water equiv. shielding)
ArgentinaChile ANDES (↔ 4800) South Korea ARF (↕⤡ 2800) Russia Baksan (↔ 4800) United Kingdom Boulby (↕ 2800) Finland CallioLab (↕⤡ 4000) Spain Canfranc (↔ 2500) China CJPL (↔ 6720) India INO (↔ 4000) Japan Kamioka (↔ 2700) United States Kimballton aka KURF (↔ 1450) Italy LNGS (↔ 3400) France LSBB (↔ 1500) France LSM/Fréjus (↔ 4800) Japan Oto (↔ 1400) Canada SNOLAB (↕ 6000) UkraineSoledar (↕ 570) United States Soudan (↕ 2100) Australia Stawell aka SUPL (⤡ 2900) United States SURF (↕ 4300) United States WIPP (↕ 1600) South Korea Yangyang aka Y2L (↔ 2100)
vte
Neutrino detectors, experiments, and facilities
Discoveries
Cowan–Reines ( νe ) Lederman–Schwartz–Steinberger ( νμ) DONUT ( ντ) Neutrino oscillation SN 1987 neutrino burst
Operating
(divided by primary neutrino source)
Astronomical
ANITA ANTARES ASD BDUNT Borexino BUST HALO IceCube LVD NEVOD SAGE Super-Kamiokande SNEWS
Reactor
Daya Bay Double Chooz KamLAND RENO STEREO
Accelerator
ANNIE ICARUS (Fermilab) MicroBooNE MINERνA MiniBooNE NA61/SHINE NOνA NuMI T2K
AMoRE COBRA CUORE EXO GERDA KamLAND-Zen MAJORANA NEXT PandaX SNO+ XMASS
Other
Construction
ARA ARIANNA Baikal-GVD BEST DUNE Hyper-Kamiokande JUNO KM3NeT SuperNEMO FASERν
Retired
AMANDA CDHS Chooz CNGS Cuoricino DONUT ERPM GALLEX Gargamelle GNO Heidelberg-Moscow Homestake ICARUS IGEX IMB K2K Kamiokande KARMEN KGF LSND MACRO MINOS MINOS+ NARC NEMO OPERA RICE SciBooNE SNO Soudan 2 Utah
Proposed
CUPID GRAND INO LAGUNA LEGEND LENA Neutrino Factory nEXO Nucifer SBND UNO JEM-EUSO WATCHMAN
Cancelled
DUMAND Project Long Baseline Neutrino Experiment NEMO Project NESTOR Project SOX BOREX
See also
BNO (Baksan or Baxan Neutrino Observatory) Kamioka Observatory LNGS SNOLAB List of neutrino experiments
Hellenica World - Scientific Library
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