c B(n + AA) could be as high as 1.0%, giving deB ~ 200 to 400 nb. c +­It is important to note that n cannot be produced by e e annihilation process c o directly. We also understand that the detection efficiency of the SPEAR for two V fS is less than a few percent. -4­ References! W.T. Kirk (eds.)ms, Proceedings of the 1975 International Sym~osium on Lepto~ and Photon Interactions at High Energies, Stanford Universitv, August 21-27,.!2Zi 2. R.J. Schnitzrk, p. 25 3. T. Appelquier, Lectures on llew Particle Spectroscopy, BNL, August 1976 4. R.M. Bennett, H. Georgi, H.D. Politzst, uCOl!mlents on the New Particles", Invited talk presented at the 2nd International Conference at Vanderbilt University on New Results in High Energy Physics, Nashville, Tennessee, March 1-3, 1976. Yale Report COO-3075-l4l 5. G.J. Blanar et al.er, Harvard Preprint, July 1976 W.T. Kirk (eds.)., Proceedings of the 1975 International Svm~osium on Lepton and Photon Interactions at High Energies, Stanford University, August 21-27, 197 6. S.C.C. Tirk, p. 195 W.T. Kirk (eds.)ng, Proceedings of the 1975 International Svm~osiu~ on Leoton and Photon Interactions at High Energies,- Stanford Cniversity, AU2ust 21-27,.ill rk, p