In this note we study the structure of diffeomorphism anomalies in 3 1 canonical gravity coupled to a chiral massless fermion. We find tha
t when the spatial manifold Sigma is S-3 or a Lens space L(p, q), the
first homotopy group of the related diffeomorphism group can be non-tr
ivial and hence the question of global anomalies becomes relevant. Her
e we show that for gravity coupled to SU(2) chiral fermions, assuming
the strong form of the Hatcher conjecture, SU(2)-induced diffeomorphis
m anomalies do not occur whenever Sigma is S-3 or a Lens space. (C) 19
98 Elsevier Science B.V.