Evolving Lorentzian wormholes with the required matter satisfying the energy conditions are discussed. Several different scale factors are used and the corresponding consequences derived. The effect of extra, decaying (in time) compact dimensions present in the wormhole metric is also explored and certain interesting conclusions are derived for the cases of exponential and Kalusa-Klein inflation.PACS number(s): 04.

Ohio 44106We suggest that the reactions pp~*W yX and pp -*W yX are good candidates for measuring the magnetic moment parameter K in /% = (e/2M w ) (1 +K) . The angular distribution of the W bosons in pp-* W yX is particularly sensitive to this parameter. For the gaugetheory value of K -1, we have found a peculiar zero in d

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