G. F. Pearce

The GENIE Neutrino Monte Carlo Generator

The exploration of the neutrino mixing matrix forms one of the major directions in science. A number of scientific opportunities lie ahead: Over the next decade searches for

The Atmospheric Neutrino Flavor Ratio from a 3.9 Fiducial Kiloton-Year Exposure of Soudan 2

{\nu}_{\mu} \rightarrow {\nu}_{e}

Measurement of the atmospheric neutrino flavour composition in Soudan 2

oscillations will dramatically improve our sensitivity to

Observation of planar three-jet events in e+e− annihilation and evidence for gluon bremsstrahlung

{\theta}_{13}

Total cross section for hadron production by e+e− annihilation at petra energies

, potentially opening a window to exploring CP violation in the lepton sector. Precision measurements of

Measurement of the L/E distributions of atmospheric neutrinos in Soudan 2 and their interpretation as neutrino oscillations

{\theta}_{23}

EXPERIMENTAL-STUDY OF JETS IN ELECTRON-POSITRON ANNIHILATION

from high statistics

Test of Quantum Electrodynamics at {PETRA}

{\nu}_{\mu}

Experimental evidence for differences in 〈p⊥〉 between quark jets and gluon jets

disappearance studies will shed more light on the neutrino mixing matrix and, possibly, elucidate its relation with the quark mixing matrix. Over a similar time-scale, exploiting matter effects, we will probe the neutrino mass hierarchy. Much of the research program will be carried out with accelerator-made neutrino beams in the few-GeV energy range, the challenging boundary between the non-perturbative and perturbative regimes where our lacking physics descriptions are now being exposed by increasingly precise neutrino data. Advancing our understanding of fundamental neutrino properties, will require building a more complete picture of neutrino interactions and reducing the corresponding systematics to the\break

BARYON PRODUCTION IN E+E(-)-ANNIHILATION AT PETRA

\sim