We begin with a four-dimensional manifold, M, that possesses a two paramete
r family of (local) foliations by three-surfaces, with the two parameters b
eing the coordinates on the sphere of directions at each point of the manif
old expressed via homogeneous coordinates pi(A) and pi(A'). By then requiri
ng that each foliation (of the two parameter set of foliations) be a one pa
rameter family of null surfaces for some (as yet unkown) conformal Lorentzi
an metric-we derive an explicit expression, in terms of the foliation descr
iption, for this conformal metric. We then show (1) how a conformal factor
can be chosen to convert the conformal metric into a metric and (2) how to
impose on the foliation and conformal factor conditions so that the metric
satisfies the vacuum Einstein equations. The material described here is ver
y much connected to the null surface formulation (NSF) of GR developed earl
ier. The advantages of the present formulation are that one can much more e
asily see the logical structure of the NSF, one can calculate with much gre
ater ease and finally it allows [because of the use of (spinor) index calcu
lus] generalizations of the NSF so that the study of the evolutionary devel
opment of the null surface singularities (caustics, etc.) can be developed.
(C) 2000 American Institute of Physics. [S0022-2488(00)04609-0].