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Gravity and Strings

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Lie groups, symmetric spaces, <strong>and</strong> Yang–Mills fields 609<br />

A.4.2 Example: round spheres<br />

The n-dimensional sphere S n (see Appendix C) is a homogeneous topological space on<br />

which the orthogonal group SO(n + 1) acts transitively. 18 Any point is invariant under<br />

rotations around the axis that crosses that point: the isotropy group is thus SO(n), <strong>and</strong> S n<br />

is therefore homeomorphic to SO(n + 1)/SO(n). Ifthe SO(n + 1) generators are { ˆM â ˆb },<br />

â, ˆb = 1,...,n + 1, the generators of SO(n) can be chosen as {Mab ≡ ˆMab} a, b = 1,...,n<br />

<strong>and</strong> those of the orthogonal complement as Pa ≡ Mn+1 a. Weimmediately see that S n is a<br />

symmetric space:<br />

[Pa, Mbc] = 2δa[c Pb] =−PdƔv(Mbc) d a, [Pa, Pb] = Mab. (A.129)<br />

To construct an SO(n + 1)-symmetric Riemannian metric, 19 we first construct a coset<br />

representative u as above <strong>and</strong> then the Maurer–Cartan 1-form V :<br />

−V = Pndx n + e −xn Pn Pn−1e xn Pn dx n−1<br />

Here we can use repeatedly the formula<br />

+ e −xn Pn e x n−1 Pn−1 Pn−2e xn Pn−1 e x n Pn dx n−2 ···. (A.130)<br />

[X, Y ] = Z, [Y, Z] = X, [Z, X] = Y, ⇒ e aX Ye −aX = cos(a) Y + sin(a) Z,<br />

(A.131)<br />

for the triplets Pa, Pb, <strong>and</strong> Mab,or, far better, the definition of the adjoint action:<br />

In both cases, the result is<br />

e −xn Pn Pn−1e xn Pn = 1<br />

2 ˆM â ˆb ƔAdj(e −xn Pn ) â ˆb n−1. (A.132)<br />

−e = Pndx n + Pn−1 cos x n dx n−1 + Pn−2 cos x n cos x n−1 dx n−2 + ···,<br />

−ϑ = sin x n<br />

a=n−1 <br />

Mnadx a + cos x n sin x n−1<br />

a=n−2 <br />

Mn−1 adx a<br />

a=1<br />

a=1<br />

a=1<br />

+ cos x n cos x n−1 sin x n−2<br />

a=n−3 <br />

Mn−2 adx a + ···.<br />

Using the SO(n)-invariant metric 20 δab,weobtain the SO(n + 1)-invariant metric<br />

(A.133)<br />

ds 2 = (dx n ) 2 + cos 2 x n (dx n−1 ) 2 + cos 2 x n−1 (dx n−2 ) 2 + ···. (A.134)<br />

On comparing this with the metric Eq. (C.4) in st<strong>and</strong>ard spherical coordinates, we see that<br />

the coset coordinates that we have used are related to them by x n = θn−1 + π/2,...,x 1 =<br />

ϕ.The spin connection is given by<br />

ω a b = 1<br />

2 ϑ cd fcd n+1b n+1a = 1<br />

2 ϑ cd Ɣv(Mcd) a b = ϑ a b, (A.135)<br />

18 SO(n + 1) rotates in the st<strong>and</strong>ard form the coordinates of the ambient space Rn+1 , respecting the defining<br />

equation (x1 ) 2 + ···+(x n+1 ) 2 = 1.<br />

19 With<br />

1<br />

2 n(n + 1) isometries, spheres with this metric (round spheres) are also maximally symmetric spaces.<br />

20 On rescaling some entries of δab, one obtains squashed spheres (see Appendix C.2) that have less symmetry.

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