If the geometry of space-time is \nc, i.e. [xμ,xν]=iθμν, then \nc\cpviolng effects may be manifest at low energies. For a
\nc scale Λ≡θ−1/2≤2TeV, \cpviol from \ncg is
comparable to that from the Standard Model (SM) alone: the \nc contributions
to ϵ and ϵ′/ϵ in the K-system, may actually dominate
over the Standard Model contributions. Present data permit \ncg to be the
only source of \cpviol. Furthermore the most recent findings for g-2 of the
muon are consistent with predictions from \ncg. If the geometry of space-time
is \nc, i.e.[xμ,xν]=iθμν, then \nc\cpviolng
effects may be manifest at low energies. For a \nc scale Λ≡θ−1/2≤2TeV, \cpviol from \ncg is comparable to that from the
Standard Model (SM) alone: the \nc contributions to ϵ and
ϵ′/ϵ in the K-system, may actually dominate over the Standard
Model contributions. Present data permit \ncg to be the only source of
\cpviol. Furthermore the most recent findings for g-2 of the muon are
consistent with predictions from \ncg.Comment: fixed notation, corrected some typo