Distance Geometry in Superspace

We can define a distance invariant under superspace transformations: R2=|xy|2+θγμ(xy)μζ For D space-time dimensions and E Grassman dimensions, does this satisfy a Cayley-Menger type equation? In 2 dimensions we know the volume of a tetrahedron is zero. Or: det[0R12R13R141R120R23R241R13R230R341R14R24R340111110]=0 What about when D=11 and E=32 ? Simplest is D=1, E=2 with (?): R2=(xy)2+(xy)(θζ+ζθ) with for example: R4=(xy)4+2(xy)3(θζ+ζθ)+2(xy)2(θθζζ) R6=(xy)6+3(xy)5(θζ+ζθ)+6(xy)4(θθζζ) Then the area of the triangle is 0 (or and polynomial with 0 constant term). We should have an identity, something like (?): R63R4(xy)2+R2(xy)4+(xy)6=0 So we would have: Δ(LAB)=0F(LAB,RAB)=0?G(RAB)=0 (Rxy)2(Rxz)2=(xy)2(xz)2+(xy)2(xz)(θζ+ζθ)+2(xz)2(xy)(θβ+βθ) +2(xy)(xz)θθ(ζβ+βζ) So (?) Δ0+(xy)(zx)(zy)(θζ+ζθ+ζβ+βζ+...) +2(xy)2(θθζζ)+(xy)(xz)θθ(ζβ+βζ)+... So very simply we can say that the distance geometry is compataible with D real and 4 grassman dimensions if (?): (ΔD)2=0

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