Abstract

If the geometry of space-time is \nc, i.e. [xμ,xν]=iθμν[x_{\mu},x_{\nu}]=i \theta_{\mu \nu}, then \nc \cpviolng effects may be manifest at low energies. For a \nc scale Λθ1/22TeV\Lambda \equiv \theta^{-1/2} \leq 2 TeV, \cpviol from \ncg is comparable to that from the Standard Model (SM) alone: the \nc contributions to ϵ\epsilon and ϵ/ϵ\epsilon'/\epsilon in the KK-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.i.e. [xμ,xν]=iθμν[x_{\mu},x_{\nu}]=i \theta_{\mu \nu}, then \nc \cpviolng effects may be manifest at low energies. For a \nc scale Λθ1/22TeV\Lambda \equiv \theta^{-1/2} \leq 2 TeV, \cpviol from \ncg is comparable to that from the Standard Model (SM) alone: the \nc contributions to ϵ\epsilon and ϵ/ϵ\epsilon'/\epsilon 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

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