TheoremComplete

Ambrose-Singer Holonomy Theorem

The Ambrose-Singer theorem describes the holonomy group of a connection in terms of its curvature, providing the fundamental link between the infinitesimal (curvature) and global (holonomy) aspects of a connection.


Holonomy Groups

Definition7.13Holonomy group

Let βˆ‡\nabla be a connection on a vector bundle Eβ†’ME \to M (or equivalently on a principal GG-bundle Pβ†’MP \to M). Fix a point p∈Mp \in M. The holonomy group Holp(βˆ‡)βŠ‚GL(Ep)\mathrm{Hol}_p(\nabla) \subset \mathrm{GL}(E_p) consists of all parallel transport maps around piecewise smooth loops based at pp:

Holp(βˆ‡)={PΞ³:Epβ†’Ep∣γ isΒ aΒ loopΒ atΒ p}.\mathrm{Hol}_p(\nabla) = \{P_\gamma : E_p \to E_p \mid \gamma \text{ is a loop at } p\}.

The restricted holonomy group Holp0(βˆ‡)\mathrm{Hol}^0_p(\nabla) uses only contractible loops.


The Theorem

Theorem7.4Ambrose-Singer holonomy theorem

Let Pβ†’MP \to M be a principal GG-bundle with connection Ο‰\omega and curvature Ξ©\Omega. For u∈Pu \in P with Ο€(u)=p\pi(u) = p, the Lie algebra of the holonomy group Holu(Ο‰)\mathrm{Hol}_u(\omega) is

holu(Ο‰)=span⁑{Ξ©v(X,Y):v∈P(u), X,Y∈Hv},\mathfrak{hol}_u(\omega) = \operatorname{span}\{\Omega_v(X, Y) : v \in P(u), \, X, Y \in H_v\},

where P(u)P(u) is the holonomy bundle through uu (all points reachable from uu by horizontal paths) and HvH_v is the horizontal subspace at vv.


Proof Outline

Proof

Part 1: Curvature lies in the holonomy algebra. Consider an infinitesimal parallelogram at pp. Parallel transport around it differs from the identity by F(X,Y)ϡ2+O(ϡ3)F(X,Y)\epsilon^2 + O(\epsilon^3), so F(X,Y)∈holpF(X,Y) \in \mathfrak{hol}_p.

More precisely, for tangent vectors X,YX, Y at vv, consider the loop obtained by flowing along XX, then YY, then βˆ’X-X, then βˆ’Y-Y for time Ο΅\epsilon. The holonomy of this loop is id+Ο΅2Ξ©v(X,Y)+O(Ο΅3)\mathrm{id} + \epsilon^2 \Omega_v(X,Y) + O(\epsilon^3), showing Ξ©v(X,Y)∈holu\Omega_v(X,Y) \in \mathfrak{hol}_u.

Similarly, Ξ©v(X,Y)\Omega_v(X,Y) for any vv in the holonomy bundle contributes, since parallel transporting to vv and back conjugates the infinitesimal holonomy into holu\mathfrak{hol}_u.

Part 2: Nothing else lies in the holonomy algebra. This requires showing the subbundle of PP defined by the span of curvature endomorphisms is integrable (by the Frobenius theorem applied to the distribution HβŠ•hH \oplus \mathfrak{h} where h\mathfrak{h} is the curvature span). The Bianchi identity ensures the integrability condition. β– \blacksquare

β– 

Applications

ExampleFlat connections have trivial restricted holonomy

If Ξ©=0\Omega = 0 everywhere, then hol0=0\mathfrak{hol}^0 = 0, so Hol0={e}\mathrm{Hol}^0 = \{e\}. The full holonomy group is then discrete, corresponding to the monodromy representation Ο€1(M)β†’G\pi_1(M) \to G. This recovers the classical result that flat connections correspond to representations of the fundamental group.

Theorem7.5Berger's classification

If (Mn,g)(M^n, g) is a simply connected, irreducible (not a product), non-symmetric Riemannian manifold, then Hol(g)\mathrm{Hol}(g) is one of:

| Holonomy | Dimension | Geometry | |----------|-----------|----------| | SO(n)SO(n) | nn | Generic | | U(n/2)U(n/2) | nn (even) | Kahler | | SU(n/2)SU(n/2) | nn (even) | Calabi-Yau | | Sp(n/4)Sp(n/4) | nn (4∣n4|n) | Hyperkahler | | Sp(n/4)β‹…Sp(1)Sp(n/4) \cdot Sp(1) | nn (4∣n4|n) | Quaternionic Kahler | | G2G_2 | 7 | Exceptional | | Spin(7)\mathrm{Spin}(7) | 8 | Exceptional |

RemarkHolonomy in physics

In string theory, compactifications on manifolds with special holonomy (particularly SU(3)SU(3) for Calabi-Yau threefolds and G2G_2 for MM-theory) preserve supersymmetry. Berger's classification thus constrains the possible internal geometries in string compactifications.