Qr. Ahmad et al., Measurement of the rate of nu(e)+d -> p+p+e(-) interactions produced by B-8 solar neutrinos at the sudbury neutrino observatory - art. no. 071301, PHYS REV L, 8707(7), 2001, pp. 1301
Solar neutrinos from B-8 decay have been detected at the Sudbury Neutrino O
bservatory via the charged current (CC) reaction on deuterium and the elast
ic scattering (ES) of electrons. The flux of nu (e)'s is measured by the CC
reaction rate to be phi (CC)(nu (e)) = 1.75 +/-0.07(stat)(-0.11)(+0.12)(sy
st) +/-0.05(theor) x 10(6) cm(-2) s(-1). Comparison of phi (CC)(nu (e)) to
the Super-Kamiokande Collaboration's precision value of the flux inferred f
rom the ES reaction yields a 3.3o sigma difference, assuming the systematic
uncertainties are normally distributed, providing evidence of an active no
n=nu (e) component in the solar flux. The total flux of active B-8 neutrino
s is determined to be 5.44 +/-0.99 x 10(6) cm(-2) s(-1).