FLUX OF SCALAR NEUTRINO DARK-MATTER

Recently the exotic event observed at the Yunnan Cosmic Ray Station (Y CRS) is reinterpreted as a neutral supersymmetric (SUSY) particle bomb arding on proton to produce a charged SUSY particle which decays after wards. The kinematics analysis determines the lower bounds of its mass and Lifetime. Taking this bounds as inputs and following recent Liter atures to assume the scalar neutrino (sneutrino) as the main constitue nt of the cold SUSY dark matter, rye calculate the flux of sneutrino a t the earth detector in terms of the standard rate equation of cosmic matter.