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Analytic continuation of Spacetime Metrics

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Compacted conformal infinity<br />

by choosing advanced and retarded null coordinates v, w defined<br />

by v = t + r, w = t — r , the second (spherical) metric becomes:<br />

Minkowski spacetime<br />

with its conformal infinity<br />

structure imbedded in the<br />

Einstein static universe<br />

with two spatial<br />

dimensions suppressed.<br />

define p and q by tan p = v and tan q = w, introduce a<br />

conformal factor and extend ds 2 to cover the whole manifold -><br />

Einstein static universe as the cylinder x 2 +y 2 = 1 imbedded in a<br />

3-d Minkowski space.<br />

conformally map Minkowski spacetime into a patch <strong>of</strong> the<br />

cylinder; the boundary = conformal structure <strong>of</strong> infinity<br />

two null surfaces<br />

any future-directed timelike geodesic will originate from i - and terminate at i +<br />

all null-like geodesics begin at past null infinity and end on future null infinity<br />

all spacelike geodesics both begin and end at spacelike infinity i 0<br />

the shaded region = conformal to the whole <strong>of</strong> Minkowski space-time

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