I outline a series of results obtained in collaboration with A. Waldron on
the properties of massive higher (s>1) spin fields in cosmological, constant
curvature, backgrounds and the resulting unexpected qualitative effects on
their degrees of freedom and unitarity properties. The dimensional parameter
\L extends the flat space m-line to a (m^2,\L) "phase" plane in which these
novel phenomena unfold. In this light, I discuss a possible partial
resurrection of deSitter supergravity. I will also exhibit the well-known
causality problems of coupling these systems to gravity and, for complex
fields, to electromagnetism, systematizing some of the occasionally
misunderstood obstacles to interactions, particularly for s = 3/2 and 2.Comment: 9 pages, 1 figure. Invited talk at "Renormalization Group and
Anomalies in Gravity and Cosmology", Ouro Preto, Brazil, March 17-23, 200