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Neutrino detectors Basic features: 1) Very small cross-sections of interactions → very big volumes of detectors 2) Very effective shielding → underground.

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Presentation on theme: "Neutrino detectors Basic features: 1) Very small cross-sections of interactions → very big volumes of detectors 2) Very effective shielding → underground."— Presentation transcript:

1 Neutrino detectors Basic features: 1) Very small cross-sections of interactions → very big volumes of detectors 2) Very effective shielding → underground detectors, underwater, under ice Detector types: 1) Radiochemical detectors 2) Detectors of Cherenkov radiation 3) Scintillation detectors 4) Detectors based on neutrino scattering on electrons Underwater neutrino detector ANTARES Neutrino detector KAMLAND at Japan Kamiokande

2 Radiochemical detectors
For neutrinos with lower energy. Inverse beta decay process: Measurement cycle: 1) Taking of data 2) Radiochemical analysis Impossibility of neutrino energy determination (only threshold) For example: νe + 37Cl → 37Ar + e- νe + 71Ga → 71Ge + e- Scheme of gallium experiment – separation of produced germanium Chlorine experiment of R. Davise

3 Scintillation detector LSND
Detectors making use of scintillation or Cherenkov radiation Vessel: 1) Walls are covered by photomultipliers 2) Filled by liquid (liquid scintillator) Scintillation detector LSND Kamoikande detector – Cherenkov phenomena is used

4 Reaction of all neutrinos and antineutrinos: (liquid scintillator)
Heavy water – reaction of neutrinos with deuteron: Reaction of only electron neutrinos: Reaction of all neutrinos and antineutrinos: Detector KAMLAND (liquid scintillator) Photomultiplier of KAMLAND detector Detector KAMLAND

5 IceCube (AMANDA) – neutrino detector under ice
200 TeV e candidate Photomultipliers are sent under ice Detector set-up built up on South pole Detection of Cherenkov radiation produced by electrons, muons and tauons produced by reactions of high energy neutrinos

6 Proposal of HERON experiment
Neutrino scattering on electron Possibility to detect also neutrinos with very low energy Noise suppression → liquid helium (superfluid) → very low temperature (~ 10 mK) Low neutrino energy ~ keV → low electron energy Ionization, scintillation, phonons, rotons – are detected by sapphire or silicon wafer – absorber → control of temperature capture of „drifting electrons – „electron bubble“ in superfluid and superconductive liquid moves in controlled way in electric field Microcalorimetry of very small temperature changes Proposal of HERON experiment (high of 6 m)


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