Author/Authors :
Astier، نويسنده , , P and Autiero، نويسنده , , D and Baldisseri، نويسنده , , A and Baldo-Ceolin، نويسنده , , M and Banner، نويسنده , , M and Bassompierre، نويسنده , , G and Benslama، نويسنده , , K and Besson، نويسنده , , N and Bird، نويسنده , , I and Blumenfeld، نويسنده , , B and Bobisut، نويسنده , , F and Bouchez، نويسنده , , J and Boyd، نويسنده , , S and Bueno، نويسنده , , A and Bunyatov، نويسنده , , S and Camilleri، نويسنده , , L and Cardin، نويسنده ,
Abstract :
The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD are predicted with an uncertainty of about 8% for νμ and νe, 10% for ν̄μ, and 12% for ν̄e. The energy-dependent uncertainty achieved on the νe/νμ prediction needed for a νμ→νe oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%.
