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Prompt background

The contamination in the beam is the ultimate irreducible background for a oscillation search. The largest contribution to this background comes from the prompt tauonic decay of the produced from proton interactions in the neutrino target and inside the shielding.

Two new estimates of the background have recently been published [47, 48], providing adequate knowledge of this background. They include the contribution from (which is actually dominant), linear A-dependence of production cross-sections, and a value for the branching ratio as obtained in recent measurements.

For a proton energy of 450 GeV and the CHORUS detector fiducial volume, the two independent estimates of the ratio R of the number of charged-current (CC) events to CC events are from the semi-empirical parametrisation of production [47] and from the non-perturbative QCD approach [48], using the Quark-Gluon String Model (QGSM). The systematic uncertainties common to both approaches arising from the leptonic branching ratios, the production cross-section and the model parameters amount to .

This level of the prompt background, still well below one event for the total duration of the CHORUS and NOMAD experiments, becomes more relevant for a future neutrino oscillation experiment aiming at improving the sensitivity by at least one order of magnitude.

An effective way to reduce the prompt background is to lower the primary proton energy, thus exploiting the steep reduction of the production cross-section and of the acceptance of the detector for prompt . The number of CC events per proton drops faster than the number of CC events. A proton energy in the 300-350 GeV range is found to offer the best compromise. Assuming that the present WANF would operate at 350 GeV, the corresponding value of R is  [47], about 2.5 times lower than at of 450 GeV.

Additional experimental handles on the prompt background are provided by the fact that decays would result in an equal number of prompt and and that their energy spectrum is significantly harder than the one of from the oscillation.


next up previous
Next: Operation of a 350 Up: The CERN SPS neutrino Previous: The present neutrino beam