|Group theory → Lie groups
In differential geometry, representation theory and harmonic analysis, a symmetric space is a pseudo-Riemannian manifold whose group of symmetries contains an inversion symmetry about every point. This can be made more precise, in either the language of Riemannian geometry or of Lie theory. The Riemannian definition is more geometric, and plays a deep role in the theory of holonomy. The Lie-theoretic definition is more algebraic.
In Riemannian geometry, a complete, simply connected Riemannian manifold is a symmetric space if and only if its curvature tensor is invariant under parallel transport. More generally, a Riemannian manifold (M,g) is said to be symmetric if and only if, for each point p of M, there exists an isometry of M fixing p and acting on the tangent space of M at p by minus the identity. Any symmetric space is complete, and has a finite cover which is a simply connected symmetric space; thus these two characterizations in fact coincide up to finite covers. Both descriptions can also naturally be extended to the setting of pseudo-Riemannian manifolds.
From the point of view of Lie theory, a symmetric space is the quotient G/H of Lie group G by a Lie subgroup H, where the Lie algebra of H is also required to be the -eigenspace of an involution of the Lie algebra of G. As stated, this characterization includes pseudo-Riemannian spaces as well as a Riemannian ones; extra algebraic conditions are needed to restrict to the Riemannian case.
Riemannian symmetric spaces arise in a wide variety of situations in both mathematics and physics. They were first classified by Élie Cartan. Their central role in the theory of holonomy was discovered by Marcel Berger. They are important objects of study in representation theory and harmonic analysis as well as in differential geometry.
- 1 Definition using geodesic symmetries
- 2 General definition
- 3 Riemannian symmetric spaces satisfy the Lie-theoretic characterization
- 4 Classification of Riemannian symmetric spaces
- 5 Symmetric spaces in general
- 6 Weakly symmetric Riemannian spaces
- 7 Applications and special cases
- 8 See also
- 9 References
Definition using geodesic symmetries
Let M be a connected Riemannian manifold and p a point of M. A map f defined on a neighborhood of p is said to be a geodesic symmetry, if it fixes the point p and reverses geodesics through that point, i.e. if γ is a geodesic and then It follows that the derivative of the map at p is minus the identity map on the tangent space of p. On a general Riemannian manifold, f need not be isometric, nor can it be extended, in general, from a neighbourhood of p to all of M.
M is said to be locally Riemannian symmetric if its geodesic symmetries are in fact isometric. This is equivalent to the vanishing of the covariant derivative of the curvature tensor. A locally symmetric space is said to be a (globally) symmetric space if, in addition, its geodesic symmetries are defined on all of M.
The Cartan–Ambrose–Hicks theorem implies that M is locally Riemannian symmetric if and only if its curvature tensor is covariantly constant, and furthermore that any simply connected, complete locally Riemannian symmetric space is actually Riemannian symmetric.
Any Riemannian symmetric space M is complete and Riemannian homogeneous (meaning that the isometry group of M acts transitively on M). In fact, already the identity component of the isometry group acts transitively on M (because M is connected).
Locally Riemannian symmetric spaces that are not Riemannian symmetric may be constructed as quotients of Riemannian symmetric spaces by discrete groups of isometries with no fixed points, and as open subsets of (locally) Riemannian symmetric spaces.
Basic examples of Riemannian symmetric spaces are Euclidean space, spheres, projective spaces, and hyperbolic spaces, each with their standard Riemannian metrics. More examples are provided by compact, semi-simple Lie groups equipped with a bi-invariant Riemannian metric. An example of a non-Riemannian symmetric space is anti-de Sitter space.
Any compact Riemann surface of genus greater than 1 (with its usual metric of constant curvature −1) is a locally symmetric space but not a symmetric space.
Let G be a connected Lie group. Then a symmetric space for G is a homogeneous space G/H where the stabilizer H of a typical point is an open subgroup of the fixed point set of an involution σ in Aut(G). Thus σ is an automorphism of G with σ2 = idG and H is an open subgroup of the set
Because H is open, it is a union of components of Gσ (including, of course, the identity component).
As an automorphism of G, σ fixes the identity element, and hence, by differentiating at the identity, it induces an automorphism of the Lie algebra of G, also denoted by σ, whose square is the identity. It follows that the eigenvalues of σ are ±1. The +1 eigenspace is the Lie algebra of H (since this is the Lie algebra of Gσ), and the −1 eigenspace will be denoted . Since σ is an automorphism of , this gives a direct sum decomposition
The first condition is automatic for any homogeneous space: it just says the infinitesimal stabilizer is a Lie subalgebra of . The second condition means that is an -invariant complement to in . Thus any symmetric space is a reductive homogeneous space, but there are many reductive homogeneous spaces which are not symmetric spaces. The key feature of symmetric spaces is the third condition that brackets into .
Conversely, given any Lie algebra with a direct sum decomposition satisfying these three conditions, the linear map σ, equal to the identity on and minus the identity on , is an involutive automorphism.
Riemannian symmetric spaces satisfy the Lie-theoretic characterization
If M is a Riemannian symmetric space, the identity component G of the isometry group of M is a Lie group acting transitively on M (M is Riemannian homogeneous). Therefore, if we fix some point p of M, M is diffeomorphic to the quotient G/K, where K denotes the isotropy group of the action of G on M at p. By differentiating the action at p we obtain an isometric action of K on TpM. This action is faithful (e.g., by a theorem of Kostant, any isometry in the identity component is determined by its 1-jet at any point) and so K is a subgroup of the orthogonal group of TpM, hence compact. Moreover, if we denote by sp: M → M the geodesic symmetry of M at p, the map
To summarize, M is a symmetric space G/K with a compact isotropy group K. Conversely, symmetric spaces with compact isotropy group are Riemannian symmetric spaces, although not necessarily in a unique way. To obtain a Riemannian symmetric space structure we need to fix a K-invariant inner product on the tangent space to G/K at the identity coset eK: such an inner product always exists by averaging, since K is compact, and by acting with G, we obtain a G-invariant Riemannian metric g on G/K.
To show that G/K is Riemannian symmetric, consider any point p = hK (a coset of K, where h ∈ G) and define
where σ is the involution of G fixing K. Then one can check that sp is an isometry with (clearly) sp(p) = p and (by differentiating) dsp equal to minus the identity on TpM. Thus sp is a geodesic symmetry and, since p was arbitrary, M is a Riemannian symmetric space.
If one starts with a Riemannian symmetric space M, and then performs these two constructions in sequence, then the Riemannian symmetric space yielded is isometric to the original one. This shows that the "algebraic data" (G,K,σ,g) completely describe the structure of M.
Classification of Riemannian symmetric spaces
The algebraic description of Riemannian symmetric spaces enabled Élie Cartan to obtain a complete classification of them in 1926.
For a given Riemannian symmetric space M let (G,K,σ,g) be the algebraic data associated to it. To classify possibly isometry classes of M, first note that the universal cover of a Riemannian symmetric space is again Riemannian symmetric, and the covering map is described by dividing the connected isometry group G of the covering by a subgroup of its center. Therefore, we may suppose without loss of generality that M is simply connected. (This implies K is connected by the long exact sequence of a fibration, because G is connected by assumption.)
A simply connected Riemannian symmetric space is said to be irreducible if it is not the product of two or more Riemannian symmetric spaces. It can then be shown that any simply connected Riemannian symmetric space is a Riemannian product of irreducible ones. Therefore, we may further restrict ourselves to classifying the irreducible, simply connected Riemannian symmetric spaces.
The next step is to show that any irreducible, simply connected Riemannian symmetric space M is of one of the following three types:
1. Euclidean type: M has vanishing curvature, and is therefore isometric to a Euclidean space.
2. Compact type: M has nonnegative (but not identically zero) sectional curvature.
3. Non-compact type: M has nonpositive (but not identically zero) sectional curvature.
A more refined invariant is the rank, which is the maximum dimension of a subspace of the tangent space (to any point) on which the curvature is identically zero. The rank is always at least one, with equality if the sectional curvature is positive or negative. If the curvature is positive, the space is of compact type, and if negative, it is of noncompact type. The spaces of Euclidean type have rank equal to their dimension and are isometric to a Euclidean space of that dimension. Therefore, it remains to classify the irreducible, simply connected Riemannian symmetric spaces of compact and non-compact type. In both cases there are two classes.
A. G is a (real) simple Lie group;
B. G is either the product of a compact simple Lie group with itself (compact type), or a complexification of such a Lie group (non-compact type).
The examples in class B are completely described by the classification of simple Lie groups. For compact type, M is a compact simply connected simple Lie group, G is M×M and K is the diagonal subgroup. For non-compact type, G is a simply connected complex simple Lie group and K is its maximal compact subgroup. In both cases, the rank is the rank of G.
The compact simply connected Lie groups are the universal covers of the classical Lie groups , , and the five exceptional Lie groups E6, E7, E8, F4, G2.
The examples of class A are completely described by the classification of noncompact simply connected real simple Lie groups. For non-compact type, G is such a group and K is its maximal compact subgroup. Each such example has a corresponding example of compact type, by considering a maximal compact subgroup of the complexification of G which contains K. More directly, the examples of compact type are classified by involutive automorphisms of compact simply connected simple Lie groups G (up to conjugation). Such involutions extend to involutions of the complexification of G, and these in turn classify non-compact real forms of G.
In both class A and class B there is thus a correspondence between symmetric spaces of compact type and non-compact type. This is known as duality for Riemannian symmetric spaces.
Specializing to the Riemannian symmetric spaces of class A and compact type, Cartan found that there are the following seven infinite series and twelve exceptional Riemannian symmetric spaces G/K. They are here given in terms of G and K, together with a geometric interpretation, if readily available. The labelling of these spaces is the one given by Cartan.
|AI||n − 1||Space of real structures on which leave the complex determinant invariant|
|AII||n − 1||Space of quaternionic structures on compatible with the Hermitian metric|
|AIII||min(p,q)||Grassmannian of complex p-dimensional subspaces of|
|BDI||min(p,q)||Grassmannian of oriented real p-dimensional subspaces of|
|DIII||[n/2]||Space of orthogonal complex structures on|
|CI||n||Space of complex structures on compatible with the inner product|
|CII||min(p,q)||Grassmannian of quaternionic p-dimensional subspaces of|
|EII||40||4||Space of symmetric subspaces of isometric to|
|EIII||32||2||Complexified Cayley projective plane|
|EIV||26||2||Space of symmetric subspaces of isometric to|
|EVI||64||4||Rosenfeld projective plane over|
|EVII||54||3||Space of symmetric subspaces of isomorphic to|
|EVIII||128||8||Rosenfeld projective plane|
|EIX||112||4||Space of symmetric subspaces of isomorphic to|
|FI||28||4||Space of symmetric subspaces of isomorphic to|
|FII||16||1||Cayley projective plane|
|G||8||2||Space of subalgebras of the octonion algebra which are isomorphic to the quaternion algebra|
A more modern classification (Huang & Leung 2011) uniformly classifies the Riemannian symmetric spaces, both compact and non-compact, via a Freudenthal magic square construction. The irreducible compact Riemannian symmetric spaces are, up to finite covers, either a compact simple Lie group, a Grassmannian, a Lagrangian Grassmannian, or a double Lagrangian Grassmannian of subspaces of for normed division algebras A and B. A similar construction produces the irreducible non-compact Riemannian symmetric spaces.
Symmetric spaces in general
An important class of symmetric spaces generalizing the Riemannian symmetric spaces are pseudo-Riemannian symmetric spaces, in which the Riemannian metric is replaced by a pseudo-Riemannian metric (nondegenerate instead of positive definite on each tangent space). In particular, Lorentzian symmetric spaces, i.e., n dimensional pseudo-Riemannian symmetric spaces of signature (n − 1,1), are important in general relativity, the most notable examples being Minkowski space, De Sitter space and anti-de Sitter space (with zero, positive and negative curvature respectively). De Sitter space of dimension n may be identified with the 1-sheeted hyperboloid in a Minkowski space of dimension n + 1.
Symmetric and locally symmetric spaces in general can be regarded as affine symmetric spaces. If M = G/H is a symmetric space, then Nomizu showed that there is a G-invariant torsion-free affine connection (i.e. an affine connection whose torsion tensor vanishes) on M whose curvature is parallel. Conversely a manifold with such a connection is locally symmetric (i.e., its universal cover is a symmetric space). Such manifolds can also be described as those affine manifolds whose geodesic symmetries are all globally defined affine diffeomorphisms, generalizing the Riemannian and pseudo-Riemannian case.
The classification of Riemannian symmetric spaces does not extend readily to the general case for the simple reason that there is no general splitting of a symmetric space into a product of irreducibles. Here a symmetric space G/H with Lie algebra
However, the irreducible symmetric spaces can be classified. As shown by Katsumi Nomizu, there is a dichotomy: an irreducible symmetric space G/H is either flat (i.e., an affine space) or is semisimple. This is the analogue of the Riemannian dichotomy between Euclidean spaces and those of compact or noncompact type, and it motivated M. Berger to classify semisimple symmetric spaces (i.e., those with semisimple) and determine which of these are irreducible. The latter question is more subtle than in the Riemannian case: even if is simple, G/H might not be irreducible.
As in the Riemannian case there are semisimple symmetric spaces with G = H × H. Any semisimple symmetric space is a product of symmetric spaces of this form with symmetric spaces such that is simple. It remains to describe the latter case. For this, one needs to classify involutions σ of a (real) simple Lie algebra . If is not simple, then is a complex simple Lie algebra, and the corresponding symmetric spaces have the form G/H, where H is a real form of G: these are the analogues of the Riemannian symmetric spaces G/K with G a complex simple Lie group, and K a maximal compact subgroup.
Thus we may assume is simple. The real subalgebra may be viewed as the fixed point set of a complex antilinear involution τ of , while σ extends to a complex antilinear involution of commuting with τ and hence also a complex linear involution σ∘τ.
The classification therefore reduces to the classification of commuting pairs of antilinear involutions of a complex Lie algebra. The composite σ∘τ determines a complex symmetric space, while τ determines a real form. From this it is easy to construct tables of symmetric spaces for any given , and furthermore, there is an obvious duality given by exchanging σ and τ. This extends the compact/non-compact duality from the Riemannian case, where either σ or τ is a Cartan involution, i.e., its fixed point set is a maximal compact subalgebra.
The following table indexes the real symmetric spaces by complex symmetric spaces and real forms, for each classical and exceptional complex simple Lie group.
|Gc = SL(n,C)||Gc/SO(n,C)||Gc/S(GL(k,C)×GL(l,C)), k+l=n||Gc/Sp(n,C), n even|
|G = SL(n,R)||G/SO(k,l)||G/S(GL(k,R)×GL(l,R))
or G/GL(n/2,C), n even
|G/Sp(n,R), n even|
|G = SU(p,q), p + q = n||G/SO(p,q)
|G/Sp(p/2,q/2), p,q even
|G=SL(n/2,H), n even||G/Sk(n/2,H)||G/S(GL(k/2,H)×GL(l/2,H)), k,l even
|G/Sp(k/2,l/2), k,l even, k+l=n|
|Gc=SO(n,C)||Gc/SO(k,C)×SO(l,C), k+l=n||Gc/GL(n/2,C), n even|
|G/U(p/2,q/2), p,q even
|G = Sk(n/2,H), n even||G/Sk(k/2,l/2), k,l even
|G/U(k/2,l/2), k,l even
|Gc = Sp(2n,C)||Gc/Sp(2k,C)×Sp(2l,C), k + l = n||Gc/GL(n,C)|
|G = Sp(p,q), p + q = n||G/Sp(kp,kq)×Sp(lp,lq)
|G = Sp(2n,R)||G/Sp(2k,R)×Sp(2l,R)
|G/U(k,l), k + l = n
For exceptional simple Lie groups, the Riemannian case is included explicitly below, by allowing σ to be the identity involution (indicated by a dash). In the above tables this is implicitly covered by the case kl=0.
|E7||–||E7/SU(8)||E7/SO(12)× Sp(1)||E7/E6× SO(2)|
|E8(8)||E8(8)/SO(16)||E8(8)/SO(8,8) or E8(8)/Sk(8,H)||E8(8)/E7(7)×SL(2,R) or E8(8)/E7(−5)×SU(2)|
|E8(−24)||E8(−24)/E7×Sp(1)||E8(−24)/SO(12,4) or E8(−24)/Sk(8,H)||E8(−24)/E7(−5)×SU(2) or E8(−24)/E7(−25)×SL(2,R)|
Weakly symmetric Riemannian spaces
In the 1950s Atle Selberg extended Cartan's definition of symmetric space to that of weakly symmetric Riemannian space, or in current terminology weakly symmetric space. These are defined as Riemannian manifolds M with a transitive connected Lie group of isometries G and an isometry σ normalising G such that given x, y in M there is an isometry s in G such that sx = σy and sy = σx. (Selberg's assumption that s2 should be an element of G was later shown to be unnecessary by Ernest Vinberg.) Selberg proved that weakly symmetric spaces give rise to Gelfand pairs, so that in particular the unitary representation of G on L2(M) is multiplicity free.
Selberg's definition can also be phrased equivalently in terms of a generalization of geodesic symmetry. It is required that for every point x in M and tangent vector X at x, there is an isometry s of M, depending on x and X, such that
- s fixes x;
- the derivative of s at x sends X to –X.
When s is independent of X, M is a symmetric space.
An account of weakly symmetric spaces and their classification by Akhiezer and Vinberg, based on the classification of periodic automorphisms of complex semisimple Lie algebras, is given in Wolf (2007).
Applications and special cases
Symmetric spaces and holonomy
If the identity component of the holonomy group of a Riemannian manifold at a point acts irreducibly on the tangent space, then either the manifold is a locally Riemannian symmetric space, or it is in one of 7 families.
Hermitian symmetric spaces
A Riemannian symmetric space which is additionally equipped with a parallel complex structure compatible with the Riemannian metric is called a Hermitian symmetric space. Some examples are complex vector spaces and complex projective spaces, both with their usual Riemannian metric, and the complex unit balls with suitable metrics so that they become complete and Riemannian symmetric.
An irreducible symmetric space G/K is Hermitian if and only if K contains a central circle. A quarter turn by this circle acts as multiplication by i on the tangent space at the identity coset. Thus the Hermitian symmetric spaces are easily read off of the classification. In both the compact and the non-compact cases it turns out that there are four infinite series, namely AIII, BDI with p=2, DIII and CI, and two exceptional spaces, namely EIII and EVII. The non-compact Hermitian symmetric spaces can be realized as bounded symmetric domains in complex vector spaces.
Quaternion-Kähler symmetric spaces
A Riemannian symmetric space which is additionally equipped with a parallel subbundle of End(TM) isomorphic to the imaginary quaternions at each point, and compatible with the Riemannian metric, is called Quaternion-Kähler symmetric space.
An irreducible symmetric space G/K is quaternion-Kähler if and only if isotropy representation of K contains an Sp(1) summand acting like the unit quaternions on a quaternionic vector space. Thus the quaternion-Kähler symmetric spaces are easily read off from the classification. In both the compact and the non-compact cases it turns out that there is exactly one for each complex simple Lie group, namely AI with p = 2 or q = 2 (these are isomorphic), BDI with p = 4 or q = 4, CII with p = 1 or q = 1, EII, EVI, EIX, FI and G.
Bott periodicity theorem
- Akhiezer, D. N.; Vinberg, E. B. (1999), "Weakly symmetric spaces and spherical varieties", Transf. Groups, 4: 3–24, doi:10.1007/BF01236659
- van den Ban, E. P.; Flensted-Jensen, M.; Schlichtkrull, H. (1997), Harmonic analysis on semisimple symmetric spaces: A survey of some general results, in Representation Theory and Automorphic Forms: Instructional Conference, International Centre for Mathematical Sciences, March 1996, Edinburgh, Scotland, American Mathematical Society, ISBN 978-0-8218-0609-8
- Berger, Marcel (1957), "Les espaces symétriques noncompacts", Annales Scientifiques de l'École Normale Supérieure, 74: 85–177
- Besse, Arthur Lancelot (1987), Einstein Manifolds, Springer-Verlag, ISBN 0-387-15279-2 Contains a compact introduction and lots of tables.
- Borel, Armand (2001), Essays in the History of Lie Groups and Algebraic Groups, American Mathematical Society, ISBN 0-8218-0288-7
- Cartan, Élie (1926), "Sur une classe remarquable d'espaces de Riemann, I", Bulletin de la Société Mathématique de France, 54: 214–216
- Cartan, Élie (1927), "Sur une classe remarquable d'espaces de Riemann, II", Bulletin de la Société Mathématique de France, 55: 114–134
- Flensted-Jensen, Mogens (1986), Analysis on Non-Riemannian Symmetric Spaces, CBMS Regional Conference, Americal Mathematical Society, ISBN 978-0-8218-0711-8
- Helgason, Sigurdur (1978), Differential geometry, Lie groups and symmetric spaces, Academic Press, ISBN 0-12-338460-5 The standard book on Riemannian symmetric spaces.
- Helgason, Sigurdur (1984), Groups and Geometric Analysis: Integral Geometry, Invariant Differential Operators, and Spherical Functions, Academic Press, ISBN 0-12-338301-3
- Huang, Yongdong; Leung, Naichung Conan (2010). "A uniform description of compact symmetric spaces as Grassmannians using the magic square" (PDF). Mathematische Annalen. 350 (1): 79–106. doi:10.1007/s00208-010-0549-8.
- Kobayashi, Shoshichi; Nomizu, Katsumi (1996), Foundations of Differential Geometry, Volume II, Wiley Classics Library edition, ISBN 0-471-15732-5 Chapter XI contains a good introduction to Riemannian symmetric spaces.
- Loos, Ottmar (1969), Symmetric spaces I: General Theory, Benjamin
- Loos, Ottmar (1969), Symmetric spaces II: Compact Spaces and Classification, Benjamin
- Nomizu, K. (1954), "Invariant affine connections on homogeneous spaces", Amer. J. Math., 76 (1): 33–65, doi:10.2307/2372398, JSTOR 2372398
- Selberg, Atle (1956), "Harmonic analysis and discontinuous groups in weakly symmetric riemannian spaces, with applications to Dirichlet series", J. Indian Math. Society, 20: 47–87
- Wolf, Joseph A. (1999), Spaces of constant curvature (5th ed.), McGraw–Hill
- Wolf, Joseph A. (2007), Harmonic Analysis on Commutative Spaces, American Mathematical Society, ISBN 0-8218-4289-7