2015
DOI: 10.1134/s106378421512018x
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Creation of neutrino laboratory for carrying out experiment on search for a sterile neutrino at the SM-3 reactor

Abstract: In connection with the question of possible existence of sterile neutrino the laboratory on the basis of SМ-3 reactor was created to search for oscillations of reactor antineutrino. A prototype of a neutrino detector with scintillator volume of 400 l can be moved at the distance of 6-11m from the reactor core. The measurements of background conditions have been made. It is shown that the main experimental problem is associated with cosmic radiation background. Test measurements of dependence of a reactor antin… Show more

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Cited by 12 publications
(6 citation statements)
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References 10 publications
(16 reference statements)
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“…Unfortunately, a research reactor beam hall usually has quite a large background of neutrons and gamma quanta, which makes it difficult to carry out low background experiments. Due to some peculiar characteristics of its construction, reactor SM-3 provides the most favorable conditions to search for neutrino oscillations at short distances [4,5]. However, SM-3 reactor, as well as other research reactors, is located on the Earth surface, hence, cosmic background is the major difficulty in considered experiment.…”
Section: Introductionmentioning
confidence: 99%
“…Unfortunately, a research reactor beam hall usually has quite a large background of neutrons and gamma quanta, which makes it difficult to carry out low background experiments. Due to some peculiar characteristics of its construction, reactor SM-3 provides the most favorable conditions to search for neutrino oscillations at short distances [4,5]. However, SM-3 reactor, as well as other research reactors, is located on the Earth surface, hence, cosmic background is the major difficulty in considered experiment.…”
Section: Introductionmentioning
confidence: 99%
“…We applied the method of delayed coincidences with time interval of 100 µs and managed to distinguish correlated events with rate of 1 s -1 . Most of these events are signals from muons stopped inside the detector and absorbed by nuclei with emission of 4 neutrons. Energy discrimination allows us to lower correlated event rate to 0.1s -1 [4,5].…”
Section: The Problem With Reactor Antineutrino Detection In the Presementioning
confidence: 99%
“…Advantages of SМ-3 reactor are a compact reactor core (35×42×42 сm 3 ) with high reactor power being equal to 100 MW, as well as а sufficiently short distance (5 m) from the reactor core to the wall of an experimental hall. Besides, the fact of special significance is that an 3 antineutrino beam can be measured within a sufficiently wide range from 6 to 13 meters [3,4]. However, SM-3 reactor is at the Earth surface, hence cosmic background is the main difficulty with this experiment.…”
Section: Introductionmentioning
confidence: 99%
“…It is expected that in the coming several years it will be possible to confirm or deny the existence of such anomalies and light SNs (see, for example, Refs. 23,28,[35][36][37][38]. Besides, HN with masses from several keV to several TeV are often used to explain some astrophysical data 22,39,40 .…”
Section: Introductionmentioning
confidence: 99%