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We consider the recent limits on dark matter - nucleon elastic scatteringcross section from the analysis of CDMS II collaboration using the two signalevents observed in CDMS experiment. With these limits we try to interpret theSuper-Kamiokande (SK) bounds on the detection rates of up-going muons inducedby the neutrinos that are produced in the sun from the decay of annihilationproducts of dark matter (WIMPs) captured in the solar core. Calculated rates ofup-going muons for different annihilation channels at SK using CDMS bounds arefound to be orders below the predicted upper limits of such up-going muon ratesat SK. Thus there exists room for enhancement (boost) of the calculated ratesusing CDMS limits for interpreting SK bounds. Such a feature is expected torepresent the PAMELA data with the current CDMS limits. We also show thedependence of such a possible enhancement factor (boost) on WIMP mass fordifferent WIMP annihilation channels.

Interpreting the bounds on Solar Dark Matter induced muons at Super-Kamiokande in the light of CDMS results