Joachim Meyer (DESY) SHORT PHYSICS SUMMARIES  :   NEUTRINO 
 
  This is http://www-h1.desy.de/~jmeyer/physics/neutrino/welcome.html
 


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 August 01 : SNO  First SNO results : sun neutrinos
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a) PRL-paper from     here 
   They measure 
    'CC'   nu_e d -->  e p p  and 
     ES    nu e   -->  nu e   (That is CC + few % NC)
 They compare nu_e flux from 'CC' with ES-flux from SuperK (more 
 precise than their own) ==> 3.3 sigma exess due to NC component 
 of nu_mu,nu_tau in ES. 

 Their Fig 3 (nu_e vs nu_mu,tau fluxes) is  here 

See also Physics Today (August 01)
Nice article, but severe error in fig. 3 (SNO and SUPER-K interchanged) ! b)Analysis of the sun neutrino oscillation with/without new SNO done by Fogli.et.al hep-ph/0106247 Their Delta_m - mixingangle figures are without SNO and with SNO ------------------------------------------------------------------------- April 2002 : SNO : Measurement of NC component in solar neutrino flux ================================================== by nu_x d --> p n nu_x neutron is captured and delayed gamma produces Cerenkov-electron signal Their paper (nucl-ex/0204008) is here The non-nu_e active neutrino-flux (which is thus the nu_mu+nu_tau flux) is 3.4 +- 0.7 (10**6 cm**-2 sec**-1) A 5.3 SIGMA effect !!! The total result (only SNO data) from CC nu_e d --> e p p and ES nu e --> nu e (That is CC + few % NC) NC nu_x d --> p n nu_x is in fig 3 of their paper and here ------------------------------------------------------------------------- December 2002 : First Results from KamLAND Evidence for Reactor Antineutrino Disappearance See webpage here see http://kamland.lbl.gov/ There is also a PRL- paper KamLAND detects antineutrinos (nue_bar) from fission in a large number of Japanese reactors ( 79 % of flux come from 26 reactors at distances 138 to 214 Km). The measurement procedes through inverse beta-decay ve_bar p --> e+ neutron The signal is a prompt one from e+ e- annihilation and a delayed one from neutron capture and subsequent gamma emission. They see 54 events compared to 86.8 +- 5.6 expected. The observed rate relative to expectation is 0.611 +- 0.085 +- 0.041 This gives a 5 * 10**-4 probability for no oscillation The oscillation pattern fits very well within the range expected from the solar neutrino data. Only the LMA solution fits. The best fit gives Sin**2(2Theta) = 1.0 , Delta m**2 = 6.9 10**-5 eV**2