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We start with the spheres.
Spheres
In Part 11 Proposition 1, using the inverse stereographic projection, to each oriented sphere Sρ(c) in R3 we have associated an oriented sphere Sr(m) in S3. In Part 6 to each oriented sphere Sr(m) in S3 we have associated a point in the Lie quadric Q. In Part 7 we have introduced Q+ isomorphic to the product S3 × S1. We will now combine these constructions. But first let me outline the rough idea that I have in mind while doing it.
Think of the sphere Sρ(c) as a spherical
wave propagated in space with the velocity of light. Then, assuming the
velocity of light being a constant, its radius is related to time.
Negative radius will then mean negative time. We choose the proportionality constant to be 1, which means we are choosing units in which the velocity of light is (numerically) 1. When we map our spheres to the
points of Q, we will have different points of space and time represented
by different points of Q or Q+ . Thus spacetime will be embedded in Q and Q + . That’s the rough idea. So, let us do the work now, starting with Q.
First let us recall the definitions. With R4,2 denoting the 6-dimensional space with coordinates x0 , . . . , x5 and scalar product
We have defined Q as the quadric in the real projective space P(R4,2 ):
For a point [u] in Q the coordinates (u0 , . . . , u5 ) are called homogeneous coordinates of [u]. Given an oriented sphere Sr(m) we have associated with it the point of Q with
homogeneous coordinates (cf. Eq. (6.5)):
ui= mi−1, (i = 1, . . . , 4), u4= sin(r), u5= cos(r). (13.3)
On the other hand we have the following relation (cf. Part 9 ) between signed spheres Sρ(c) with signed radius ρ and center c ∈ R3 and oriented spheres Sr(m) not containing the origin of the stereographic projection:
where m'= (m1 , m2 , m3 ). Combining these two maps we obtain the following Proposition:
Proposition 13.1. With c = c1e1 + c2e2 + c3e3 ∈ R3 , ρ ∈ R, and
is given by:
τs(c, ρ) = [ ½(1 − q(c, ρ)) e0 + c + ρ e4+ ½(1 + q(c, ρ)) e5 ]. (13.7)
Proof. See Notes Ch. 13. But try to prove it all by yourself. It is really straightforward.
13.2 Planes
Representing oriented planes will be much simpler than spheres. We recall from Proposition 1 in Part 12 that oriented planes Πh(n)
Πh(n) = {y ∈ R3: y · n = h} (13.11)
corresponds to oriented spheres Sr(m), so that:
From these formulas we obtain the following:
Proposition 13.2. With n = n1e1 + n2e2 + n3e3 ∈ R3 , h ∈ R, the correspondence,
denoted by τp between oriented planes Πh(n) in R3 and points of Q is given by:
τp (n, h) = [−he0 + n + e4 + he5 ]. (13.15)
Proof. See Notes Ch. 13. But try to prove it all by yourself. It is really straightforward.
13.3 Vectors e+ and e−
The terms in Eq. (13.7) can be collected in a different way:
τs (c, ρ) = [(e5 + e0)/2 + q(c, ρ)(e5 − e0)/2 + c + ρ e4 ]. (13.19)
This suggest introducing, instead of e0 and e5 another basis vectors
e+ = ( e5 + e0)/2, e− = (e5 − e0)/2. (13.20)
Vectors e+ and e− are null vectors (Why?):
(e+ , e+ ) = (e− , e− ) = 0, (13.21)
and satisfy (Why?):
(e+ , e− ) = −1/2. (13.22)
Eqs. (13.19) and (13.15) read now:
We have obtained the formulas in Propositions 13.1 and 13.2 using the intermediary tool of the stereographic projection. But once we have them, we can use them simple as definitions of embeddings. As such they make a perfect sense also in Q+ if we interpret the equivalence classes [·] within Q+ . The same concerns (13.23) and (13.24), both being well defined in Q+ .
Exercise 1. Take a plane, any n, and move to infinity. Which particular element of Q would correspond to such a "plane at infinity"?







