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Remarks on initial conditions for scalar field driven inflationary models

We consider the use of scalar fields in driving both an early and late, quintessence dark energy, inflationary phase. Due to finite causal length constraints the homogeneity of the dark energy field has to be imposed prior to any early universe inflationary phase: so introducing an initial uniformity problem. Neither is quantum cosmological reasoning well suited to justifying numerous initially displaced scalar fields with vastly differing energy scales. Some further difficulties with multiple assisted, kinetic and phantom inflationary models are outlined. We review the use of the canon-ical measure in predicting a single phase of inflation and find the negative conclusions of Gibbons and Turok can be allayed. We briefly remark upon some attempts to incorporate inflationary schemes into cyclic models.