We study local variations of causal curves in a space-time with respec
t to b-length (or generalized affine parameter length). In a convex no
rmal neighbourhood, causal curves of maximal metric length are geodesi
cs. Using variational arguments, we show that causal curves of minimal
b-length insufficiently small globally hyper belie sets are geodesics
. As an application we obtain a generalization of a theorem by Schmidt
, showing that the cluster curve of a partially future imprisoned, fut
ure inextendible and future b-incomplete curve must be a null geodesic
. We give examples which illustrate that the cluster curve does not ha
ve to be closed or incomplete. The theory of variations developed in t
his work provides a starting point for a Morse theory of b-length. (C)
1997 American Institute of Physics.