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SYMPLECTIC QUOTIENTS: MOMENT MAPS, SYMPLECTIC REDUCTION AND THE MARSDEN-WEINSTEIN-MEYER THEOREM

VICTORIA HOSKINS

1. Construction of group quotients in differential geometry Let X be a smooth manifold and K be a ; then an action of K on X is an action σ : K × X → X which is smooth map of manifolds such that σk : X → X is a diffeomorphism for all k ∈ K. Let K · x denote the orbit of x ∈ X and Kx denote the stabiliser of x. The topological quotient is the orbit space X/K = {K · x : x ∈ X}, which is given the quotient topology, so that the morphism π : X → X/K is continuous. In general, this topological quotient need not be a manifold. Example 1.1. (1) Let S1 act on S2 by rotation so that the North and South pole are the only fixed points of this action; then the topological quotient is homeomorphic to the closed interval [0, 1], which is not a manifold, as it has corners. In this example, the boundary points arise as the action is not free. 2 1 1 (2) Let R act on T = S × S by translation by an irrational slope ω1/ω2. More precisely, if we consider T 2 as obtained from the square [0, 1]2 by gluing opposite edges, then the lift of this action to [0, 1]2 is given by

t · (a, b) = (a + ω1t, b + ω2t). In this example, the orbit space is not Hausdorff due to the presence of dense orbits. This is a phenomena of non-proper actions. Remark 1.2. (1) If K acts properly on X (that is, the graph of the action K × X → X × X given by (k, x) 7→ (k · x, x) is proper), then all orbits are closed and the quotient X/K is Hausdorff. (2) If K is compact, then any action of K on X is proper. Theorem 1.3. Let K be a Lie group acting freely and properly on a smooth manifold X; then there is a unique structure of a smooth manifold on X/K such that π : X → X/K is a submersion. Furthermore, π : X → X/K is a principal K-bundle. Proof. We give an outline of the main steps in the proof. Step 1: each orbit K · x is a closed embedded submanifold diffeomorphic to K. Consider the action map σx : K → X given by k 7→ k · x; this is a smooth (as σ is smooth), proper (as K is compact), injective (as the action is free) morphism with image K · x. We claim that σx is an immersion. Up to the action of K, it suffices to check that deσx : k → TxX is injective, where k denotes the of K. We see that deσx(A) = 0 for A ∈ k if and only if the infinitesimal action of A on x is trivial, but, as the action is free, this holds if and only if A = 0. Step 2: the Slice theorem. For a free action of K on X, a slice of the action at x ∈ X is an open neighbourhood S ⊂ X of x such that the action K × S → K · S gives a K-equivariant diffeomorphism. In our set up of a free and proper action, we can use the Slice theorem of Palais to construct slices of the action at every point in X and, in Step 3, we use these slice to provide charts on X/K. 1 2 VICTORIA HOSKINS

To construct a slice of the action at x ∈ X, we choose a decomposition

TxX = Tx(K · x) ⊕ W such that W is normal to the orbit. Following Step 1, we produce a transverse section S to the orbit K · x by taking a sufficiently small ball D ⊂ W such S is the image of D under the diffeomorphism

Φ: {neighbourhoods of 0 ∈ TxX} −→ {neighbourhoods of x ∈ X}.

For  > 0, we let S := S ∩ Φ(B(0)). The Slice theorem states that for  sufficiently small, the map η : K × S → X given by (k, s) 7→ k · s is a diffeomorphism onto a K-invariant neighbourhood of K · x. For any  > 0, one verifies that d(e,x)η is bijective; that is, η is a local diffeomorphism at (e, x) and, using the K-action, we deduce that dη is a local diffeomorphism at (k, x) for all k ∈ K. We claim that for  sufficiently small, η is injective. To prove this we 0 argue by contradiction: otherwise there are sequences xn → x and xn → x in X and gn, hn ∈ K 0 such that (gn, xn) 6= (hn, xn) and 0 gn · xn = hn · xn. −1 0 Let kn := hn gn; then kn · xn = xn → x. Consider the graph of the action Γ : K × X → X × X; 0 then Γ(kn, xn) = (kn · xn, xn) = (xn, xn), which converges to (x, x). As the action is proper, there is a convergent subsequence knj → k. However, such a convergent subsequence contradicts the fact that η is a local diffeomorphism at (k, x). Hence, for  sufficiently small, η is injective, and provides a diffeomorphism from a neighbourhood K × S of K × {x} in K × X onto a neighbourhood U of η(K × {x}) = K · x in X. This completes the proof of the Slice theorem. Step 3: The construction of charts via the slice theorem. Let π : X → X/K and p = π(x) for some x ∈ X. We use the slice theorem to provide a chart at p ∈ X/K. Let S be a slice at x ∈ X; then S is a smooth open neighbourhood of x ∈ X and we have a diffeomorphism K × S =∼ U := K · S. Hence, π(U) = U/K =∼ (K × S)/K =∼ S is an open neighbourhood of p = π(x) ∈ X/K and we can use the smooth structure on S to define a smooth structure locally on X/K. We leave it as an exercise to check that the transition functions and π are smooth. By construction of these charts, we see that π : X → X/K is a principal K-bundle.  2. Actions in Let (X, ω) be a ; that is, X is a (real) smooth manifold and ω is a closed non-degenerate 2-form on X, called the symplectic form. We can think of ω as a family of skew-symmetric non-degenerate bilinear forms

ωx : TxX × TxX → R. ∼ ∗ The non-degeneracy of ω implies that dimR X is even and ω induces isomorphisms TxX = TxX , which vary smoothly with x ∈ X. In particular, the symplectic form determines an isomorphism TX =∼ T ∗X. Definition 2.1. Let K be a lie group and σ : K × X → X be a smooth action. We say the ∗ action is symplectic if K acts by ; that is, σkω = ω for all k ∈ K. Hence, for a symplectic action, the action K → Diff(X) factors through the subgroup of symplectomorphisms Sympl(X, ω). Our goal is to provide a method for constructing quotients of such actions in symplectic geometry; in the sense, that the quotient is also a symplectic manifold. Even if a symplectic K-action on (X, ω) admits a smooth quotient X/K, this quotient may not be symplectic purely for dimension reasons (for example, if K has odd dimension, then so does X/K and so the quotient cannot be symplectic). Instead, we will construct a quotient with expected dimension dim X − 2 dim K, by using a for the action to construct a symplectic reduction. The moment map for the action can be thought of as a lift of an infinitesimal version of the action. SYMPLECTIC QUOTIENTS 3

2.1. Infinitesimal action. The Lie algebra k = TeK is an infinitesimal version of the Lie group K. We can construct an infinitesimal version of the action by associating to each A ∈ k, a vector field AX on X as follows: at x ∈ X, we have d A := exp(tA) · x| ∈ T X. X,x dt t=0 x We denote the (infinite dimensional) Lie algebra of smooth vector fields on X by Vect(X) := Γ(TX), where the Lie bracket [−, −] on Vect(X) is given by the commutator. The infinitesimal action σinf : k → Vect(X),A 7→ AX is a Lie algebra anti-homomorphism (the fact that this is an anti-homomorphism is explained by the sign which occurs when going between left and right actions: the Lie bracket on k is defined using left-invariant vector fields, which are generating vector fields for the right action of the group on itself, whereas the action of K on X is a left action). The symplectic form ω determines an isomorphism TX =∼ T ∗X and, on taking global sections, we obtain an isomorphism Vect(X) =∼ Ω1(X) := Γ(T ∗X). The exterior derivative d : C∞(X) → Ω1(X) together with this isomorphism determine a map ∞ 1 ∼ Φω : C (X) → Ω (X) = Vect(X), f 7→ Yf . We can define a Lie algebra structure on C∞(X) using ω by

{f, g} := ω(Yf ,Yg) where Yf = Φω(f). Then Φω is a Lie algebra anti-homomorphism; that is,

Φω({f, g}) = −[Yf ,Yg]. Definition 2.2. A vector field on a symplectic manifold (X, ω) is Hamiltonian if it lies in the image of Φω (that is, the corresponding 1-form is exact). A vector field is symplectic if the corresponding 1-form is closed. As exact forms are closed, every Hamiltonian vector field is a symplectic vector field. Definition 2.3. Let K be a Lie group acting on a symplectic manifold (X, ω). The action is

i) infinitesimally symplectic if AX is a symplectic vector field for all A ∈ k. ii) weakly Hamiltonian if AX is a Hamiltonian vector field for all A ∈ k. For a weakly Hamiltonian action, the infinitesimal action k → Vect(X) can be pointwise lifted to a map k → C∞(X), because a Hamiltonian vector field corresponds (under ω) to the exterior derivative of a smooth function on X. In general, this lift is non-unique as there may be several smooth functions with the same exterior derivative. Definition 2.4. A symplectic action of a Lie group K on (X, ω) is Hamiltonian if the infinites- ∗ ∞ imal action σinf : k → Vect(X) can be lifted to a Lie algebra homomorphism µ : k → C (X), called the comoment map, such that the following diagram commutes C∞(X) µ∗ ; Φω  k /Vect(X). σinf 2.2. Moment map. Hamiltonian actions can also be described by using a moment (or mo- mentum) map, which one should think of as dual to a comoment map. Definition 2.5. A smooth map µ : X → k∗ is called a moment map if it is K-equivariant with respect to the action of the given K on X and the coadjoint action of K on k∗, and µ satisfies the following infinitesimal lifting property:

(1) dxµ(ζ) · A = ωx(AX,x, ζ) for all x ∈ X, ζ ∈ TxX and A ∈ k. 4 VICTORIA HOSKINS

Remark 2.6. ∗ ∗ A (1) For µ : X → k and A ∈ k , if we let µ : X → R denote the function x 7→ µ(x) · A, then A ∗ the infinitesimal lifting property can be stated as dµ = ιAX ω for all A ∈ k , where ιAω denotes the 1-form obtained by contracting the 2-form ω with the vector field AX . (2) The momentum map first arose in classical mechanics; we give some simple examples of moment maps arising from physical actions in Example 2.8 below. For a detailed description of the moment map from the viewpoint of classical mechanics, see the notes of Butterfield [1]. (3) There is still no consistent sign convention for the moment map and so often a minus sign may appear in the condition (1) used to define a moment map. For K connected, we claim that there is a bijective correspondence {µ : X → k∗ moment maps} ←→ {µ∗ : k → C∞(X) comoment maps} given by µ 7→ µ∗ where µ∗(A)(x) := µ(x) · A. It is clear that the infinitesimal lifting property ∗ of µ given by (1) corresponds to the factorisation property ϕω ◦ µ = σinf . Let us explain how K-equivariance of µ corresponds to the property that µ∗ is a Lie algebra homomorphism. Suppose we have a moment map µ; then by K-equivariance of µ, we have ∗ µ(k · x) · A = (Adkµ(x)) · A = µ(x) · Adk−1 (A) for all k ∈ K, x ∈ X and A ∈ k. For A, B ∈ k, we then have d 0 = µ(exp(tB) · x) · A − µ(x) · Ad (A) | dt exp(−tB) t=0 = dxµ(BX,x) · A − µ(x) · [−B,A]

= ωx(AX,x,BX,x) − µ(x) · [A, B] = {µ∗(A), µ∗(B)}(x) − µ∗([A, B])(x), which proves that µ∗ is an Lie algebra homomorphism. Conversely, if we know that µ∗ is a Lie algebra homomorphism and we want to prove that µ is K-equivariant, it suffices to prove that ∗ for all x ∈ X and A ∈ k that the map ϕx,A : K → R given by ϕx,A(k) := µ(k · x) · Adk(A) is constant. As K is connected, it suffices to prove that the derivative of ϕx,A is trivial and, by using the K-action, we can reduce to checking only deϕx,A = 0. We see that d d ϕ (B) = µ(exp(tB) · x) · Ad (A)| e x,A dt exp(tB) t=0 = dxµ(BX,x) · A + µ(x) · [B,A] = {µ∗(A), µ∗(B)}(x) − µ∗([A, B])(x) = 0, as µ∗ is a Lie algebra homomorphism, which completes the proof. Remark 2.7. The moment map is not necessarily unique (see Example 2.9 below), although for certain groups we will see that it is unique (cf. part (1) of Example 2.10 ). The existence of a moment map can be characterised in terms of an extension of ω to a equivariant 2-form by work of Atiyah and Bott; see §2.4 below. 2.3. Examples of moment maps. We start with some examples which highlight the connec- tion between the moment map and classical mechanics. Example 2.8. 2 2 2 2 3 (1) Consider the natural action of SO(3) on the sphere S := {x +y +z = 1} ⊂ R , where 2 3 S has symplectic structure ω = dθ ∧ dz, for the cylindrical coordinates r, θ, z on R . ∼ 3 We can identify so(3) = R by sending the infinitesimal rotation at the standard basis 2 3 ∼ ∗ vector ej to ej. Then the moment map for this action is the inclusion S ,→ R = so(3) . To see this, consider the S1-action on S2 given by rotation around the z-axis. Then, if 1 ∼ we identify T1S = R, the moment map is given by the projection (x, y, z) → z, as

ι ∂ ω = dz. ∂θ SYMPLECTIC QUOTIENTS 5

We note that this map is S1-equivariant, as it is S1-invariant and the coadjoint action of S1 is trivial. Similarly, one can verify that the S1-action given by rotation around the x-axis (resp. y-axis) is the projection onto the corresponding axis. 3 (2) If one considers the lift of the natural action of SO(3) on R to its ∗ 3 ∼ 3 3 T R = R × R given by the diagonal action, then this action is symplectic for the ∗ 3 ∗ 3 3 Liouville form ω on T R . Furthermore, the moment map µ : T R → R is given by the cross product µ(p, q) = p × q. If we view p as a position vector and q as a momentum vector, then the cross product p × q gives the angular momentum about the origin. The simplest example is actions on symplectic vector spaces given by representations. Example 2.9. Let K = U(n) be the unitary group of n × n matrices and consider its standard n representation on C . The infinitesimal action is given by d A = exp(tA) · x| = Ax X,x dt t=0 n n n for x ∈ C and A a skew-Hermitian matrix in u(n). Let H : C × C → C denote the standard n n Hermitian inner product on C : if we write z ∈ C as a row vector (z1, . . . zn), then H(z, v) = zvt = vzt = Tr(ztv) = Tr(vtz) t n n where v denotes the transpose of a matrix. We take the symplectic form ω : C × C → R equal given by the imaginary part of this Hermitian inner product: 1   1 ω(z, v) = H(z, v) − H(z, v) = (H(z, v) − H(v, z)) . 2i 2i The Hermitian inner product is U(n)-invariant (that is, H(Az, Av) = H(z, v) for all unitary n matrices A ∈ U(n)) and so it follows that the action of U(n) on (C , ω) is symplectic. In fact, n ∗ this action is Hamiltonian and there is a canonical choice of moment map µ : C → u(n) which is defined by 1 1 µ(z) · A = ω(Az, z) = H(Az, z) 2 2i for A ∈ u(n). The second equality follows from the fact that for A ∈ u(n): (2) H(Az, v) + H(z, Av) = Tr(ztAtv) + Tr(ztAv) = Tr(zt(At + A)v) = Tr(0) = 0 n for all z, v ∈ C and A ∈ u(n). We shall now carefully check that this is a moment map. First, µ is U(n)-equivariant: 1 1 µ(k · z) · A = ω(Ak · z, k · z) = ω(k−1Ak · z, ·z) = µ(z) · k−1Ak = Ad∗µ(x) · A 2 2 k n where A ∈ u(n), z ∈ C and k ∈ U(n). To verify the infinitesimal lifting condition (1), we may n ∼ n identify TzC = C and then this condition becomes

dzµ(v) · A = ω(Az, v) n ∼ n for v ∈ C = TzC and A ∈ u(n). We have d d µ(v) · A := µ(z + tv) · A| z dt t=0 1 d 1 = ω(A(z + tv), z + tv)| = [ω(Az, v) + ω(Av, z)] 2 dt t=0 2 1 = [H(Az, v) − H(v, Az) + H(Av, z) − H(z, Av)] 4i 1 = [H(Az, v) − H(v, Az)] =: ω(Az, v) 2i where the first equality on the final line follows from the relation given at (2). The moment map for this symplectic action is not unique; although it is unique up to addition by an element η of u(n)∗ which is fixed by the coadjoint action U(n) → GL(u(n)) (we call such η a central element). Every character of U(n) is a power of the determinant det : U(n) → S1, 1 ∼ whose derivative is given by the trace Tr : u(n) → Lie S = 2πiR. Hence, such a central element 6 VICTORIA HOSKINS

∗ ∗ η of u(n) must be equal to ciTr ∈ u(n) , for some constant c ∈ R, and we can use such an element to define a shifted moment map 1 µ (z) · A = H(Az, z) + η · A. η 2i n Example 2.10. If K is a Lie group which acts on C by a faithful representation ρ : K → U(n), n then we can write down the moment map µK for the action of K on C using ρ and the moment n ∗ n map µU(n) : C → u(n) for the U(n)-action on C constructed in Example 2.9. The moment map for the action of K is given by ∗ µK = ρ µU(n) where ρ∗ : u(n)∗ → k∗ is the dual to the inclusion ρ : k → u(n). We consider the following special cases: n (1) If K = SU(n) acts on C by the standard inclusion into U(n), then its moment map is given by 1 1 µ(z) · A = ω(Az, z) = H(Az, z) 2 2i for A ∈ su(n). However, there are no non-zero central elements of su(n) which we can use to shift the moment map by and so this moment map is unique. 1 n n (2) If K = (S ) acts on C via the representation

(t1, . . . , tn) 7→ diag(t1, . . . , tn), then the moment map is given by 1 µ(z) · (A ,...,A ) = ω(diag(A ,...,A )z, z) 1 n 2 1 n 1 ∼ n for Ak ∈ LieS = 2πiR. If we write z = (z1, . . . , zn) ∈ C and Ak = 2iak for real numbers ak then n X 2 µ(z) · (2ia1,..., 2ian) = ak|zk| . k=1 As the group K = (S1)n is commutative, every element in central and so it follows that ∼ n all elements in k = (2πiR) are central. We can shift the standard moment map by any n-tuple (c1, . . . , cn) of real numbers to get n X 2 µ(z) · (2ia1,..., 2ian) = (ak|zk| + ck). k=1 1 n n (3) We may also consider K = (S ) acting on C via the representation

r1 rn (t1, . . . , tn) 7→ diag(t1 , . . . , tn )

for integers rk. In this case the moment map (shifted by real numbers ci) is given by n X 2 µ(z) · (2ia1,..., 2ian) = (akrk|zk| + ck). k=1 Exercise 2.11. Consider the action of K = U(m) on the space of l × m-matrices over the ∼ lm −1 complex numbers Ml×m(C) = C given by k·M = Mk where we take the natural symplectic lm structure given by the imaginary part of the standard Hermitian inner product on C . Then if M ∈ Ml×m and A ∈ u(m) show i µ(M) · A = Tr(MAM ∗) 2 is a moment map for this action. SYMPLECTIC QUOTIENTS 7

So far the only examples of moment maps that we have seen are for affine spaces. A more n interesting example is complex projective space P with its Fubini–Study symplectic form ωFS (or a smooth closed subvariety with the induced form). We consider a linear unitary action of n K on P (that is, K acts via a faithful representation K → U(n + 1)). In fact, the moment n ∗ n ∗ map µK : P → k for the K-action is the composition of the moment map µ : P → u(n + 1) for the U(n + 1)-action followed by the projection u(n + 1)∗ → k∗. n Example 2.12. Let U(n + 1) act on complex projective space P by acting on its affine cone n+1 n C by its standard representation. The symplectic form on P is the Fubini-Study form n+1 ωFS constructed from the standard Hermitian inner product H on C . It is easy to see this from is U(n + 1)-invariant (that is, the action is symplectic). As the Fubini-Study form is preserved by the action of U(n + 1) and the unitary group is compact and connected, the action 1 n is infinitesimally symplectic so that dιAX ωFS = 0. Moreover, as H (P ) = 0, every closed 1-form is exact and so the action is weakly Hamiltonian. It turns out that this action is Hamiltonian n+1 and we can write down a moment map explicitly as follows. For p = (p0, . . . , pn) ∈ C − {0}, we claim that Trp∗Ap µ([p]) · A = 2i||p||2 n ∗ defines a moment map where [p] ∈ P and A ∈ u(n + 1) and p denotes the complex conjugate transpose. We leave the U(n + 1)-equivariance of µ as an exercise for the reader to check. As n the action of U(n + 1) on P is transitive, we need only verify the condition (1) at a single point n n n+1 [p] = [1 : 0 : ··· : 0] ∈ P . We can identify T[p]P with the orthogonal space to p in C with n+1 respect to the standard Hermitian product on C : n 2n+1 1 ∼ n+1 ∼ n T[p]P = TpS /Tp(S · p) = {(0, z1, . . . , zn) ∈ C } = C .

With respect to the coordinates (z1, . . . , zn) 7→ [1 : z1 : ··· : zn] at [p], the Fubini-Study form can be expressed locally as n 1 X ω = dz ∧ dz ; FS,[p] 2i k k k=1 n that is, for v, w ∈ T[p]P , we have 1 ω (v, w) = ImH(v, w) = [H(v, w) − H(w, v)]. FS,[p] 2i n Let v ∈ T[p]P and A ∈ u(n + 1); then d 1 d Tr((p + tv)∗A(p + tv)) d µ(v) · A := µ(p + tv) · A| = | [p] dt t=0 2i dt ||p + tv||2 t=0 1 Tr(v∗Ap + p∗Av)||p||2 − (pv∗ + vp∗)Tr(p∗Ap) = 2i ||p||4 1 (a) [H(Ap, v) − H(v, Ap)] = 2i = ωFS,[p](Ap, v) ∗ n where (a) follows as H(p, v) = p v = 0 for v ∈ T[p]P . Exercise 2.13. Let K be a compact and connected Lie group; then a coadjoint orbit O ⊂ k∗ for the action of K on k∗ has a symplectic form ω given by the Kostant-Kirillov symplectic structure. Describe the infinitesimal action for the natural action of K on O and show that the inclusion µ : O ,→ k∗ is a moment map for this action. 2.4. Moment maps and infinitesimal linearisations. Given an action of a Lie group K on a smooth manifold X, Cartan introduced a notion of K-equivariant forms which are K-invariant polynomials on k with coefficients in Ω∗(X). More precisely, let l M i ∗ j K ΩK (X) := Sym (k ) ⊗ Ω (X) , 2i+j=l 8 VICTORIA HOSKINS where (Symi(k∗)⊗Ωj(X))K is the space of K-equivariant polynomial maps on k of homogeneous degree i with coefficients in Ωj(X). There is an equivariant derivative

l l+1 dK :Ωk(X) → ΩK (X), (dK (β))(A) := (d − ιAX )(β(A)), j j−1 where A ∈ k and ιAX :Ω (X) → Ω (X) denotes the contraction with the vector field AX given by the infinitesimal action of A. Now suppose that K acts symplectically on (X, ω). Then Atiyah and Bott characterise moment maps for the K-action on X as K-equivariantly closed extensions of the symplectic 2 form ω to ΩK (X) in the following way. Since we have 2 2 K 0 K ∼ 2 K ∗ ΩK (X) = Ω (X) ⊕ Hom(k, Ω (X)) = Ω (X) ⊕ MapK (X, k ), any extension of ω ∈ Ω2(X)K to a K-equivariant 2-form is of the form ω+µ∗ for a K-equivariant map µ : X → k∗. This extension is K-equivariantly closed if and only if ∗ A 0 = dK (ω − µ )(A) = (dω, −ιAX ω + dµ ); that is, if and only if µ is a moment map. Given an Hermitian line bundle π : L → X, the group U(1) acts on the associated unit circle bundle π1 : L1 → X. Suppose that we have a U(1)-invariant connection 1-form θ on L1 with 2 ∗ curvature 2πiω ∈ Ω (X) (that is, π1ω = −dθ to fix our sign conventions). Then any unitary automorphism of L preserving θ descends to an automorphism of X preserving ω; that is, a of (X, ω). Furthermore, there is a short exact sequence

1 → U(1) → Aut(L1, θ) → Sympl(X, ω) → 1. The K-action on X determines a morphism K → Sympl(X, ω). A linearisation of the K-action on X in the Hermitian line bundle L is a lift K → Aut(L1, θ) and an infinitesimal action is a U(1) lift k → Vect(L1) of the infinitesimal action k → Vect(X). We claim that there is a bijection ∗ U(1) {µ : X → k moment maps} ←→ {φ : k → Vect(L1) infinitesimal linearisations}, A A U(1) such that µ : X → R corresponds to φ := φ(A) ∈ Vect(L1) for A ∈ k. More precisely, if −1 A A l ∈ π1 (x), then µ and φ are related by the formula A A µ (x) = θl(φl ), ∗ A where θl ∈ Tl L1 and φl ∈ TlL1. We can verify that map µ associated to an infinitesimal linearisation φ gives an infinitesimal lift of the action: ∗ A A ∗ ∗ π1dµ = d(θ(φ )) = dιφA θ = (LφA − ιφA d)θ = LφA θ + ιφA π1ω = π1ιAX ω, ∗ ∗ where ιφA π1 = π1ιAX as φ is a lift of the infinitesimal action. Hence, we can conclude that A dµ = ιAX ω. The equivariance of µ follows from the fact that α is U(1)-invariant.

3. Symplectic quotients Given a symplectic action of a Lie group K on a symplectic manifold (X, ω), we can ask whether a quotient exists in the category of symplectic manifolds. The topological quotient always exists, but it may not be a manifold; for example, if the action is not free or proper. Even if the action is free and proper, the resulting quotient manifold may have odd dimension and so will not admit a symplectic form. Hence, the topological quotient X/K does not in general provide a suitable quotient in symplectic geometry. In this section we define the symplectic reduction of a Hamiltonian action as a quotient of a level set of the moment map. We explain that this symplectic reduction inherits a unique symplectic form by a result of Marsden and Weinstein [5] and Meyer [5]. Finally, we prove that the symplectic reduction satisfied a universal property amongst all symplectic quotients. For further expository reading, see [2], [5] and [9]. SYMPLECTIC QUOTIENTS 9

3.1. Properties of moment maps. Suppose K is a Lie group acting on a symplectic manifold (X, ω). For x ∈ X, we let K · x denote the orbit of x and we let Kx denote the stabiliser of x. We note that kx := {A ∈ k : AX,x = 0} is the Lie algebra of Kx. If the action is Hamiltonian, then there is an associated moment map µ : X → k∗ and one can naturally ask what other properties of the action are encoded by the moment map. Lemma 3.1. Let K be a Lie group with a Hamiltonian action on a symplectic manifold (X, ω) with associated moment map µ : X → k∗. For x ∈ X, we have ωx i) ker dxµ = (Tx(K · x)) := {ζ ∈ TxX : ωx(η, ζ) = 0 ∀ η ∈ Tx(K · x)}; ∗ ii) Im dxµ = Annkx := {η ∈ k : η · A = 0 ∀ A ∈ kx}.

Proof. We first note that the tangent space Tx(K ·x) to the orbit is the image of the infinitesimal action k → TxX given by A 7→ AX,x and the kernel of this map is kx. i) A tangent vector ζ ∈ TxX is in the kernel of dxµ if and only if for all A ∈ k we have

0 = dxµ(ζ) · A = ωx(AX,x, ζ);

ωx that is, if and only if ζ ∈ Tx(K · x) := {ζ ∈ TxX : ωx(η, ζ) = 0 ∀η ∈ Tx(K · x)}. ii) If η = dxµ(ζ) ∈ Im dxµ for some ζ ∈ TxX, then for all A ∈ k we have that

η · A = dxµ(ζ) · A = ωx(AX,x, ζ).

If A ∈ kx, then AX,x = 0 and, thus, η = dxµ(ζ) ∈ Annkx. Hence, we have an inclusion Im dxµ ⊂ Annkx. We will prove these vector spaces coincide, by checking that they have the same dimension. Let d := dim X and n := dim ker dxµ; then Im dxµ has dimension d − n. The short exact sequence ∗ ∗ 0 → Annkx → k → kx → 0 shows that dim Annkx = dim k − dim kx = dim Tx(K · X). Therefore, it suffices to prove that dim Tx(K · X) = d − n. For any subspace W ⊂ TxX, there is a short exact sequence ωx ∗ 0 → W → TxX → W → 0, ∗ ωx where the map TxX → W is given by ζ 7→ ωx(ζ, −)|W . In particular, dim W + dim W = dim TxX = d. Applying this to Tx(K · x) and using Part i), we conclude that

ωx dim Tx(K · x) = d − dim(Tx(K · x)) = d − dim ker dxµ = d − n, which completes the proof. 

We recall that the action of K on X is free if all stabilisers Kx are trivial. We say an action is locally free at x if the stabiliser group Kx is finite, which is if and only if kx = 0. Corollary 3.2. Suppose we have a Hamiltonian action of a Lie group K on a symplectic manifold (X, ω) with associated moment map µ : X → k∗. Let η be an element in k∗ which is fixed by the coadjoint action of K. Then: i) The action is locally free at x ∈ X if and only if x is a regular point of µ. ii) The K-action is locally free on µ−1(η) if and only if η is a regular value of µ. iii) If η is a regular value of µ, then µ−1(η) ⊂ X is a closed submanifold of codimension equal −1 to the dimension of k, which is preserved by the K-action. Furthermore, Txµ (η) = −1 −1 ker dxµ for all x ∈ µ (η), and the vector spaces Txµ (η) and Tx(K · x) are orthogonal with respect to the symplectic form ωx on TxX.

Proof. i) The stabiliser Kx of a point x is finite if and only if its Lie algebra kx = 0 is zero. By ∗ Lemma 3.1 ii), we have that Im dxµ = Annkx which is equal to k if and only if kx = 0. Hence, the action is locally free at x if and only if dxµ is surjective (that is, x is a regular point of µ). Then ii) follows from i) and the definition of regular value. For iii), we use the preimage theorem for smooth manifolds: if µ : X → k∗ is a smooth map of smooth manifolds, then the preimage of a regular value is a closed submanifold of dimension dimX − dimk∗. Since η ∈ k∗ is fixed by the coadjoint action, equivariance of µ implies that 10 VICTORIA HOSKINS

−1 the preimage µ (η) is preserved by the action of K. As µ|µ−1(η) = η is constant, dxµ = 0 −1 −1 −1 on Txµ (η) for all x ∈ µ (η). Hence, Txµ (η) ⊂ kerdxµ. Since η is a regular value, dxµ is surjective and so ∗ ∗ −1 dim ker dxµ = dim TxX − dim k = dimX − dimk = dim µ (η); −1 thus Txµ (η) = kerdxµ. The final statement of iii) then follows from Lemma 3.1.  3.2. Symplectic reduction. We suppose as above that we have a Hamiltonian action of a Lie group K on a symplectic manifold (X, ω) with associated moment map µ : X → k∗. We want to construct a quotient of the K-action on X (or a submanifold of X on which the action is free) in the symplectic category. Definition 3.3. For a coadjoint fixed point η ∈ k∗, we define the symplectic reduction of the K-action on X at η to be the following topological quotient red −1 X//η K := µ (η)/K. This orbit space was considered by Marsden and Weinstein [4] and Meyer [6] as a possible symplectic quotient. At the moment, this quotient is just a topological space: its topology is the weakest topology for which the quotient map µ−1(η) → µ−1(η)/K is continuous. If η is a regular value of µ, then the preimage µ−1(η) is a submanifold of X of dimension equal to dim X − dim(K) and K acts on µ−1(η) with finite stabilisers by Corollary 3.2. However, the action of K on µ−1(η) may not be free and so the symplectic reduction will be an orbifold rather than a manifold. If η is a regular value and the action of K on µ−1(η) is free and proper, then the symplectic reduction is a manifold of dimension dim X − 2 dim K by Theorem 1.3. In this case, there is a natural symplectic form on µ−1(η)/K; this is a theorem of Marsden and Weinstein [4] and Meyer [6] which we explain in the following section. Remark 3.4. If η is a regular value of µ, but is not fixed by the coadjoint action, then we can instead consider the symplectic reduction −1 µ (η)/Kη ∗ where Kη = {k ∈ K : Adkη = η} is the stabiliser group of η for the coadjoint action. There is one point in the co-Lie algebra which is always fixed by the coadjoint action: the origin 0 ∈ k∗. We refer to the symplectic reduction at zero simply as the symplectic reduction and write X//redK := µ−1(0)/K. We will later see that it provides a universal symplectic quotient of the K-action. 3.3. Marsden-Weinstein-Meyer Theorem. Theorem 3.5. Let K be a Lie group and suppose we have a Hamiltonian action of K on a symplectic manifold (X, ω) with moment map µ : X → k∗. Let η ∈ k∗ be coadjoint fixed. If the action of K on µ−1(η) is free and proper, then the following statements hold. red −1 i) The symplectic reduction X//η K = µ (η)/K is a smooth manifold of dimension dim X − 2 dim K. Furthermore, the quotient map π : µ−1(η) → µ−1(η)/K is a principal K-bundle. red red ∗ red ∗ ii) There is a unique symplectic form ω on Xη such that π ω = i ω where i : µ−1(η) ,→ X denotes the inclusion and π : µ−1(η) → µ−1(η)/K is the quotient map. Remark 3.6. (1) The assumption that the action of K on µ−1(η) is free and proper is needed to prove that the symplectic reduction is a manifold. As the action of K on µ−1(η) is free, it follows that η is a regular value of the moment map. (2) If η is a regular value, then the action is locally free and so the topological quotient is at least an orbifold. If, moreover, K is compact, then the action on µ−1(η) is proper and locally free. In the case, the symplectic reduction at η inherits an orbifold symplectic structure, by an orbifold version of the above theorem. SYMPLECTIC QUOTIENTS 11

(3) More generally, there is a stratified symplectic structure on µ−1(η)/K defined by Sja- maar and Lerman [7] such that each stratum is a smooth symplectic manifold and the symplectic reduction µ−1(η)/K has a Poisson structure for which the strata are sym- plectic leaves. The stratification is obtained by stratifying µ−1(η) by the conjugacy class of the stabiliser group for the action. Before we prove the above theorem, we need a few preliminary lemmas. Lemma 3.7. With the assumptions of the above theorem, for all x ∈ µ−1(η), the subspace Tx(K · x) of TxX is an isotropic subspace.

Proof. We recall that Tx(K ·x) is an isotropic subspace of the (TxX, ωx) ωx −1 if Tx(K·x) ⊂ Tx(K·x) . The subspaces ker dxµ = Txµ (η) and Tx(K·x) of TxX are symplectic −1 orthogonal complements with respect to ωx for x ∈ µ (η) by Corollary 3.2. As η is fixed by the coadjoint action, this implies µ−1(η) is K-invariant and so K · x ⊂ µ−1(η). Therefore

−1 ωx Tx(K · x) ⊂ Txµ (η) = Tx(K · x) , which completes the proof that Tx(K · x) is an isotropic subspace of (TxX, ωx).  Lemma 3.8. Let I be an isotropic subspace of a symplectic vector space (V, ω). Then ω induces a unique symplectic form ω0 on the quotient Iω/I. Proof. We define ω0([v], [w]) := ω(v, w) and check this definition is well defined: ω0(v + i, w + j) = ω(v, w) + ω(i, w) + ω(v, j) + ω(i, j) = ω(v, w) + 0 + 0 + 0 for i, j ∈ I. The non-degeneracy of ω0 follows from that of ω: if [u] ∈ Iω/I and ω0([u], [v]) = 0 ω ω ω ω for all v ∈ I /I, then ω(u, v) = 0 for all v ∈ I and so u ∈ (I ) = I i.e. [u] = 0.  Proof. (Marsden-Weinstein-Meyer Theorem) The preimage theorem shows that µ−1(η) is a closed smooth submanifold of X of dimension dim X − dim K. Furthermore, as K acts on µ−1(η) freely and properly, the quotient Y := µ−1(η)/K is a smooth manifold of dimension dim X −2 dim K. We shall construct a non-degenerate 2-form ωred on Y such that π∗ωred = i∗ω, red −1 by constructing symmetric forms ωp on TpY for all p ∈ Y . Let p = π(x) where π : µ (η) → Y = µ−1(η)/K; then we have a short exact sequence of vector spaces −1 0 → Tx(K · x) → Txµ (η) → TpY → 0.

By Lemma 3.7, the subspace Tx(K · x) is isotropic and has symplectic orthogonal complement −1 red Tx(µ (η)). By Lemma 3.8, there is a canonical symplectic form ωp on

ωx −1 ∼ Tx(K · x) /Tx(K · x) = Txµ (η)/Tx(K · x) = TpY. By construction, this is a non-degenerate 2-form such that π∗ωred = i∗ω, and so it remains to check that this symplectic form is closed. As the exterior derivative d commutes with pullback we have that π∗dωred = dπ∗ωred = di∗ω = i∗dω = 0. ∗ 3 red 3 −1 The pullback map π :Ω (Xη ) → Ω (µ (η)) is injective, as π is surjective, and so we conclude red that dω = 0.  ∼ 1 n Example 3.9. Consider the action of U(1) = S on C by multiplication s · (a1, . . . , an) = n (sa1, . . . , san). We can take the standard symplectic form on C and use the Killing form on ∗ ∼ ∼ u(1) to identify u(1) = u(1) = R and write the moment map for this action as n X 2 µ(x1, . . . , xn) = |xk| . k=1 12 VICTORIA HOSKINS

For η = 0, we have that µ−1(0) = {0} and µ−1(0)/K is just a point. The value η = 1 is more interesting: −1 2n−1 X 2 µ (1) = S = {(x1, . . . , xn): |xk| = 1} n red 1 −1 1 2n−1 1 n−1 and the symplectic reduction is C // S = µ (1)/S = S /S = P . The symplectic n form ω induced from the standard symplectic form on C is the Fubini–Study form. In fact, if n+1 one considers the construction of the Fubini–Study form using the standard form on C , then one can now see that this is just a special case of the Marsden–Weinstein–Meyer Theorem. Example 3.10. Consider the action of K = U(m) on the space of l × m-matrices over the ∼ lm complex numbers Ml×m(C) = C as in Example 2.11 where l > m. We recall that the moment map is given by i µ(M) · A = Tr(MAM ∗) 2 ∗ ∼ for M ∈ Ml×m and A ∈ u(m). By using the Killing form on u(m), we can identify u(m) = u(m) and view the moment map as a morphism µ : Ml×m → u(m) given by i µ(M) = M ∗M. 2 Let η = iIm/2 denote the skew-Hermitian matrix which is an (imaginary) scalar multiple of the identity matrix Im; then clearly η is fixed by the adjoint action of U(m) on u(m). The preimage −1 ∗ µ (η) = {M ∈ Ml×m : M M = Im} consists of l × m matrices whose m columns are linearly l −1 independent and define a length m unitary frame of C . The symplectic reduction µ (η)/U(m) l is the grassmannian Gr(m, l) of m-planes in C . There is a more general version of the Marsden-Weinstein-Meyer Theorem which allows us to take reductions at points which are not fixed by the coadjoint action: Proposition 3.11. Given a Hamiltonian action of a compact connected Lie group K on a symplectic manifold (X, ω) with moment map µ : X → k∗ and an orbit O for the coadjoint action of K on k∗. If the orbit consists of regular values of µ and the action of K on µ−1(O) is free and proper, then the symplectic reduction µ−1(O)/K is a symplectic manifold of dimension dim X + dim O − 2 dim K. Proof. The assumption that every point of O is a regular value of the moment map means that the preimage µ−1(O) is a closed submanifold of X of dimension dim X + dim O − dim K. The coadjoint orbit O has a natural symplectic form, which we denote by ωO, given by the Kostant- Kirillov symplectic structure. Consider the natural action of K on the product (X×O, −ωωO), for which the moment map µ0 : X × O → k∗ is given by µ0(x, η) = −µ(x) + η. Then the proposition follows by applying the original version of the Marsden-Weinstein-Meyer 0 −1 ∼ 0 −1 Theorem to the regular value 0 of µ and observing that µ (O) = (µ ) (0).  Remark 3.12. If η ∈ k∗ is not fixed by the coadjoint action of K on k∗, then ∗ Kη = {k ∈ K : Adkη = η} −1 −1 acts on µ (η). Then the symplectic reduction µ (Oη)/K constructed above for the coadjoint −1 orbit Oη of η is homeomorphic to the quotient µ (η)/Kη. Remark 3.13. Suppose X is a K¨ahlermanifold (i.e. it has a complex structure I and a Riemannian metric g such that ω := g(I−, −) is a symplectic form) and the action of the Lie group K preserves this structure (since the metric g, complex structure I and symplectic form ω are compatible, it suffices to check that K preserves three out of the two structures). If the action is Hamiltonian with moment map µ and K acts freely and properly on µ−1(0) where 0 is a regular value of the moment map, then the symplectic reduction µ−1(0)/X also has a K¨ahler structure (i.e. the almost complex structure induced on the symplectic reduction is integrable and and the metric also induces a compatible k¨ahler metric on the symplectic reduction). SYMPLECTIC QUOTIENTS 13

3.4. Symplectic Implosion. Let K be a compact Lie group with a Hamiltonian action on a symplectic manifold (X, ω) with moment map µ : X → k∗. The idea of a symplectic implosion for this action is to construct a stratified symplectic space with an action of a maximal torus of K, such that the symplectic reductions of K acting on X at different values η can be recovered as symplectic reductions of this maximal torus acting on the symplectic implosion. In this sense, it provides an abelianisation of the process of symplectic reduction. ∗ Definition 3.14. Fix a maximal torus T ⊂ K and positive Weyl chamber t+. The symplectic ∗ implosion Ximpl of X with respect to t+ is a stratified symplectic space with a Hamiltonian ∗ ∗ action of T on Ximpl and moment map µimpl : Ximpl → t such that for each η ∈ t+, we have a (stratified) symplectomorphism −1 ∼ −1 µimpl(η)/T = µ (η)/Kη. The construction of symplectic implosions is due to Guillemin, Jeffrey and Sjamaar [3]. The ∗ strata of Ximpl are indexed by the faces σ of t+. More precisely, we have G −1 Ximpl = µ (σ)/[Kσ,Kσ], σ ∗ where σ runs over the faces of t+, and Kσ denotes the stabiliser of the face σ. −1 ∗ Alternatively, one can construct Ximpl by gluing points in µ (t+), where x ∼ y if and only if µ(x) = µ(y) = η and x = ky for some k ∈ [Kη,Kη]. From this second description, we see there −1 ∗ −1 ∗ is a T -action on µ (t+), which descends to Ximpl = µ (t+)/ ∼, as T normalises [Kη,Kη]. ∗ ∗ The moment map µ : X → k induces the moment map µimpl : Ximpl → t , in the sense that −1 ∗ µ ◦ π = µ| −1 ∗ , where π : µ (t ) → X is the quotient map obtained by gluing. impl µ (t+) + impl

Theorem 3.15. (Guillemin, Jeffrey, Sjamaar [3]) The stratified symplectic space Ximpl is a ∗ symplectic implosion of the K-action on X with respect to t+. A third method for constructing the symplectic implosion is to use the universal symplectic implosion for K: namely consider K acting on its cotangent bundle T ∗K; then Guillemin, Jeffrey and Sjamaar [3] prove there is an isomorphism of stratified Hamiltonian T -spaces: ∼ ∗ red Ximpl = (X × (T K)impl)// K. 3.5. Lagrangian Correspondences. We recall that a symplectomorphism f :(M, ω) → (M 0, ω0) of symplectic manifolds is a diffeomorphism f : M → M 0 such that f ∗ω0 = ω. Since this definition is rather restrictive, one has a more general notion of morphisms in the symplectic category given by Lagrangian correspondences. Definition 3.16. (1) A submanifold L of a symplectic manifold X is Lagrangian if 2 dim L = dim X and i∗ω = 0 where i : L,→ X is the inclusion. Equivalently, L is Lagrangian if for all x ∈ L the vector space TxL is a Lagrangian subspace of TxX; that is, ωx (TxL) = {η ∈ TxX : ωx(η, ζ) = 0 ∀ ζ ∈ TxL} = TxL.

(2) A Lagrangian correspondence between symplectic manifolds (X1, ω1) and (X2, ω2) is a ∗ ∗ Lagrangian submanifold L12 of (X1 × X2, −ω1  ω2) where −ω1  ω2 := −π1ω1 + π2ω.

Remark 3.17. For any symplectomorphism φ :(X1, ω1) → (X2, ω2), the graph Γ(φ) ⊂ (X1 × X2, −ω1 ω2) is a Lagrangian submanifold. Therefore, the notion of symplectic correspondence generalises that of symplectomorphisms. We want to view Lagrangian correspondences as morphisms in the symplectic category. For this, we need to define the composition of two Lagrangian correspondence. Given Lagrangian submanifolds L12 ⊂ (X1 × X2, −ω1  ω2) and L23 ⊂ (X2 × X3, −ω2  ω3), we define the composition L13 = L23 ◦ L12 to be the Lagrangian submanifold L13 := π13(L12 ×X2 L23) of (X1 × X3, −ω1  ω3) given by L13 = {(x1, x3) ∈ X1 × X3 : ∃x2 ∈ X2 such that (x1, x2) ∈ L12 and (x2, x3) ∈ L23}. 14 VICTORIA HOSKINS

Then, following [8], we define morphisms in the symplectic category to consist of chains of symplectic correspondences.

3.6. Universality of the symplectic reduction. Given a Hamiltonian action of a Lie group K on a symplectic manifold (X, ω) with moment map µ : X → k∗, the aim of this section is to show (under the assumptions of the Marsden-Weinstein-Meyer theorem) that the symplectic reduction (µ−1(0)/K, ωred) is a universal quotient of the K-action on (X, ω) in the symplectic category. We recall that the symplectic form ωred is the unique symplectic form such that π∗ωred = i∗ω where i : µ−1(0) ,→ X denotes the inclusion and π : µ−1(0) → µ−1(0)/K denotes the quotient map. First of all we need to construct a Lagrangian correspondence between (X, ω) and the symplectic reduction (µ−1(0)/K, ωred). Lemma 3.18. If the assumptions of the Marsden-Weinstein-Meyer Theorem hold for η = 0, then −1 −1  Lµ := Im i × π : µ (0) → X × µ (0)/K −1 red is a Lagrangian submanifold of (X × µ (0)/K, −ω  ω ). −1 Proof. As Lµ is diffeomorphic to µ (0) we have 1 dim L = dim X − dim K = dim X × µ−1(0)/K . µ 2 −1 ∗ red ∗ ∗ red If j : Lµ ,→ X × µ (0)/K, then j (−ω  ω ) ≡ 0 if and only if −i ω + π ω ≡ 0 which holds by the Marsden-Weinstein-Meyer theorem.  In particular, this lemma gives a morphism in the symplectic category (X, ω) and the re- duction (µ−1(0)/K, ωred). However, we want this morphism to be K-equivariant and so we should define what it means for a Lagrangian correspondence to be K-invariant (or in fact more generally K-equivariant): Definition 3.19.

(1) A K-equivariant Lagrangian correspondence between symplectic manifolds (xi, ωi) for i = 1, 2 with Hamiltonian K-actions is a Lagrangian submanifold L ⊂ (X1 × X2, −ω1  ω2) which is K-invariant and satisfies µ12(L) = 0, where µ12 denotes the moment map for the K-action on (X1 × X2, −ω1  ω2). (2) A K-invariant Lagrangian correspondence between a symplectic manifold (X1, ω1) with Hamiltonian K-action and a symplectic manifold (X2, ω2) is a K-equivariant Lagrangian correspondence, where we give (X2, ω2) the trivial K-action.

The proof of the following lemma is immediate by definition of Lµ. Lemma 3.20. If the assumptions of the Marsden-Weinstein-Meyer Theorem hold for η = 0, then the Lagrangian correspondence Lµ is K-invariant. Proposition 3.21. Let K be a Lie group with a Hamiltonian action on a symplectic manifold ∗ −1 (X, ω) with moment map µ : X → k . If K acts freely and properly on µ (0), then Lµ is a universal K-invariant symplectic correspondence from (X, ω); in the sense that every other K-invariant Lagrangian correspondence from (X, ω) to a symplectic manifold (Y, ω0) factors through Lµ. Proof. It suffices to prove the result when the morphism from (X, ω) to (Y, ω0) is given by a single 0 0 K-invariant Lagrangian correspondence i.e. a Lagrangian submanifold L ⊂ (X × Y, −ω  ω ) ∗ which is preserved by the action of K and on which µXY : X × Y → k is zero. As the K-action on Y is trivial, so is the moment map µY and so µXY is the projection X × Y → X followed ∗ 0 −1 0 by µ = µX : X → k . In particular, L ⊂ µ (0) × Y as µXY (L ) = 0, by assumption that 0 0 L is K-invariant. To show that L factors through Lµ, it suffices to produce a Lagrangian 00 −1 0 00 00 correspondence L between µ (0)/K and Y such that L = L ◦ Lµ. One checks that L := 0 −1 L /K ⊂ µ (0)/K × Y is the required Lagrangian submanifold.  SYMPLECTIC QUOTIENTS 15

References 1. J. Butterfield, On symplectic reduction in classical mechanics, Handbook of philosophy of physics, Elsevier Oxford, UK, 2007, pp. 1–132. 2. A. Cannas da Silva, Lecture on symplectic geometry, Lecture notes in Mathematics, Springer-Verlag, 2001. 3. V. Guillemin, L. Jeffrey, and R. Sjamaar, Symplectic implosion, Transform. Groups 7 (2002), no. 2, 155–184. MR 1903116 4. J. Marsden and A. Weinstein, Reduction of symplectic manifolds with symmetry, Rep. Math. Phys. 5 (1974), 121–130. 5. D. McDuff and D. Salamon, Introduction to symplectic topology, second ed., Oxford Mathematical Monographs, Oxford University Press, 1998. 6. K. Meyer, Symmetries and integrals in mechanics, Dynamical systems (M. Peixoto, ed.), Academic Press New York, 1973, pp. 259–273. 7. R. Sjamaar and E. Lerman, Stratified symplectic spaces and reduction, Ann. of Math. 134 (1991), no. 2, 375–422. 8. A. Weinstein, The symplectic “category”, Differential geometric methods in mathematical physics (Clausthal, 1980), Lecture Notes in Mathematics, vol. 905, Springer, Berlin, 1982, pp. 45–51. 9. C. Woodward, Moment maps and geometric invariant theory, Les cours du CIRM 1 (2010), no. 1, 55–98.