English

What will the first year of SNO show?

High Energy Physics - Phenomenology 2009-10-31 v3 Astrophysics High Energy Physics - Experiment Nuclear Experiment Nuclear Theory

Abstract

The ratio of the measured to the predicted standard model CC event rates in SNO will be 0.47 if no oscillations occur. The best-fit active oscillation predictions for the CC ratio are: 0.35-39 (MSW) and 0.38-42 (vacuum) (all for a 5 MeV energy threshold), typically about 20% less than the no-oscillation expectation. We calculate the predicted ratios for six active and sterile neutrino oscillation solutions allowed at 99% CL and determine the dependence of the ratios on energy threshold. If the high-energy anomaly observed by SuperKamiokande is due to an enhanced hep flux, MSW active solutions predict that out of a total of 5000 CC events above 5 MeV in SNO between 49 and 54 events will be observed above 13 MeV whereas only 19 events are expected for no-oscillations and a nominal standard hep flux.

Keywords

Cite

@article{arxiv.hep-ph/9911248,
  title  = {What will the first year of SNO show?},
  author = {John Bahcall and Plamen Krastev and Alexei Smirnov},
  journal= {arXiv preprint arXiv:hep-ph/9911248},
  year   = {2009}
}

Comments

Phys Lett accepted. Editorial corrections. Related material and viewgraphs at http://www.sns.ias.edu/~jnb