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

Neutrino detectors

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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 detectors, underwater, - PowerPoint PPT Presentation

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Page 1: Neutrino detectors

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

Neutrino detector KAMLAND at Japan Underwater neutrino detectorANTARESKamiokande

Page 2: Neutrino detectors

Radiochemical detectors

For example: νe + 37Cl → 37Ar + e-

νe + 71Ga → 71Ge + e-

For neutrinos with lower energy. Inverse beta decay process:

Scheme of gallium experiment – separation of produced germanium

Chlorine experiment of R. Davise

Impossibility of neutrino energydetermination (only threshold)

Measurement cycle: 1) Taking of data 2) Radiochemical analysis

Page 3: Neutrino detectors

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 phenomenais used

Page 4: Neutrino detectors

Detector KAMLAND

Heavy water – reaction of neutrinos with deuteron:

Photomultiplier of KAMLAND detectorDetector KAMLAND

Reaction of all neutrinos and antineutrinos:Reaction of only electronneutrinos:

(liquid scintillator)

Page 5: Neutrino detectors

IceCube (AMANDA) – neutrino detector under ice

200 TeV e candidate

Detector set-up built up on South pole

Photomultipliers are sentunder ice

Detection of Cherenkov radiation produced by electrons, muons and tauons produced by reactions of high energy neutrinos

Page 6: Neutrino detectors

Neutrino scattering on electron

Possibility to detect also neutrinos with very low energy

Noise suppression → liquid helium (superfluid) → very low temperature (~ 10 mK)

Microcalorimetry of very small temperature changes

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 controlledway in electric field

Proposal of HERON experiment(high of 6 m)