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Symmetric space

From Wikipedia, the free encyclopedia

(pseudo-)Riemannian manifold whose geodesics are reversible
For other uses, seeSymmetric space (disambiguation).
Lie groups andLie algebras

Inmathematics, asymmetric space is aRiemannian manifold (or more generally, apseudo-Riemannian manifold) whose group of isometries contains aninversion symmetry about every point. This can be studied with the tools ofRiemannian geometry, leading to consequences in the theory ofholonomy; or algebraically throughLie theory, which allowedCartan to give a complete classification. Symmetric spaces commonly occur indifferential geometry,representation theory andharmonic analysis.

In geometric terms, 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 pointp ofM, there exists an isometry ofM fixingp and acting on the tangent spaceTpM{\displaystyle T_{p}M} as minus the identity (every symmetric space iscomplete, since any geodesic can be extended indefinitely via symmetries about the endpoints). Both descriptions can also naturally be extended to the setting ofpseudo-Riemannian manifolds.

From the point of view of Lie theory, a symmetric space is the quotientG / H of a connectedLie groupG by a Lie subgroupH that is (a connected component of) the invariant group of aninvolution ofG. This definition includes more than the Riemannian definition, and reduces to it whenH is compact.

Riemannian symmetric spaces arise in a wide variety of situations in both mathematics and physics. Their central role in the theory of holonomy was discovered byMarcel Berger. They are important objects of study in representation theory and harmonic analysis as well as in differential geometry.

Geometric definition

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LetM be a connected Riemannian manifold andp a point ofM. A diffeomorphismf of a neighborhood ofp is said to be ageodesic symmetry if it fixes the pointp and reverses geodesics through that point, i.e. ifγ is a geodesic withγ(0)=p{\displaystyle \gamma (0)=p} thenf(γ(t))=γ(t).{\displaystyle f(\gamma (t))=\gamma (-t).} It follows that the derivative of the mapf atp is minus the identity map on thetangent space ofp. On a general Riemannian manifold,f need not be isometric, nor can it be extended, in general, from a neighbourhood ofp to all ofM.

M is said to belocally 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 can be extended to isometries on all ofM.

Basic properties

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TheCartan–Ambrose–Hicks theorem implies thatM is locally Riemannian symmetricif and only if its curvature tensor iscovariantly constant, and furthermore that everysimply connected,complete locally Riemannian symmetric space is actually Riemannian symmetric.

Every Riemannian symmetric spaceM is complete and Riemannianhomogeneous (meaning that the isometry group ofM acts transitively onM). In fact, already the identity component of the isometry group acts transitively onM (becauseM 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.

Examples

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Basic examples of Riemannian symmetric spaces areEuclidean space,spheres,projective spaces, andhyperbolic spaces, each with their standard Riemannian metrics. More examples are provided by compact, semi-simpleLie groups equipped with a bi-invariant Riemannian metric.

Every compactRiemann surface of genus greater than 1 (with its usual metric of constant curvature −1) is a locally symmetric space but not a symmetric space.

Everylens space is locally symmetric but not symmetric, with the exception ofL(2,1){\displaystyle L(2,1)}, which is symmetric. The lens spaces are quotients of the 3-sphere by a discrete isometry that has no fixed points.

An example of a non-Riemannian symmetric space isanti-de Sitter space.

Algebraic definition

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LetG be a connectedLie group. Then asymmetric space forG is a homogeneous spaceG / H where the stabilizerH of a typical point is an open subgroup of the fixed point set of aninvolutionσ in Aut(G). Thusσ is an automorphism ofG withσ2 = idG andH is an open subgroup of the invariant set

Gσ={gG:σ(g)=g}.{\displaystyle G^{\sigma }=\{g\in G:\sigma (g)=g\}.}

BecauseH is open, it is a union of components ofGσ (including, of course, the identity component).

As an automorphism ofG,σ fixes the identity element, and hence, by differentiating at the identity, it induces an automorphism of the Lie algebrag{\displaystyle {\mathfrak {g}}} ofG, also denoted byσ, whose square is the identity. It follows that the eigenvalues ofσ are ±1. The +1 eigenspace is the Lie algebrah{\displaystyle {\mathfrak {h}}} ofH (since this is the Lie algebra ofGσ), and the −1 eigenspace will be denotedm{\displaystyle {\mathfrak {m}}}. Sinceσ is an automorphism ofg{\displaystyle {\mathfrak {g}}}, this gives adirect sum decomposition

g=hm{\displaystyle {\mathfrak {g}}={\mathfrak {h}}\oplus {\mathfrak {m}}}

with

[h,h]h,[h,m]m,[m,m]h.{\displaystyle [{\mathfrak {h}},{\mathfrak {h}}]\subset {\mathfrak {h}},\;[{\mathfrak {h}},{\mathfrak {m}}]\subset {\mathfrak {m}},\;[{\mathfrak {m}},{\mathfrak {m}}]\subset {\mathfrak {h}}.}

The first condition is automatic for any homogeneous space: it just says the infinitesimal stabilizerh{\displaystyle {\mathfrak {h}}} is a Lie subalgebra ofg{\displaystyle {\mathfrak {g}}}. The second condition means thatm{\displaystyle {\mathfrak {m}}} is anh{\displaystyle {\mathfrak {h}}}-invariant complement toh{\displaystyle {\mathfrak {h}}} ing{\displaystyle {\mathfrak {g}}}. Thus any symmetric space is areductive homogeneous space, but there are many reductive homogeneous spaces which are not symmetric spaces. The key feature of symmetric spaces is the third condition thatm{\displaystyle {\mathfrak {m}}} brackets intoh{\displaystyle {\mathfrak {h}}}.

Conversely, given any Lie algebrag{\displaystyle {\mathfrak {g}}} with a direct sum decomposition satisfying these three conditions, the linear mapσ, equal to the identity onh{\displaystyle {\mathfrak {h}}} and minus the identity onm{\displaystyle {\mathfrak {m}}}, is an involutive automorphism.

Riemannian symmetric spaces satisfy the Lie-theoretic characterization

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IfM is a Riemannian symmetric space, the identity componentG of the isometry group ofM is aLie group acting transitively onM (that is,M is Riemannian homogeneous). Therefore, if we fix some pointp ofM,M is diffeomorphic to the quotientG/K, whereK denotes theisotropy group of the action ofG onM atp. By differentiating the action atp we obtain an isometric action ofK on TpM. This action is faithful (e.g., by a theorem of Kostant, any isometry in the identity component is determined by its1-jet at any point) and soK is a subgroup of the orthogonal group of TpM, hence compact. Moreover, if we denote bysp: M → M the geodesic symmetry ofM atp, the map

σ:GG,hsphsp{\displaystyle \sigma :G\to G,h\mapsto s_{p}\circ h\circ s_{p}}

is aninvolutive Lie groupautomorphism such that the isotropy groupK is contained between the fixed point groupGσ{\displaystyle G^{\sigma }} and its identity component (hence an open subgroup)(Gσ)o,{\displaystyle (G^{\sigma })_{o}\,,} see the definition and following proposition on page 209, chapter IV, section 3 in Helgason's Differential Geometry, Lie Groups, and Symmetric Spaces for further information.

To summarize,M is a symmetric spaceG / K with a compact isotropy groupK. 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 aK-invariant inner product on the tangent space toG / K at the identity coseteK: such an inner product always exists by averaging, sinceK is compact, and by acting withG, we obtain aG-invariant Riemannian metricg onG / K.

To show thatG / K is Riemannian symmetric, consider any pointp =hK (a coset ofK, wherehG) and define

sp:MM,hKhσ(h1h)K{\displaystyle s_{p}:M\to M,\quad h'K\mapsto h\sigma (h^{-1}h')K}

whereσ is the involution ofG fixingK. Then one can check thatsp is an isometry with (clearly)sp(p) =p and (by differentiating) dsp equal to minus the identity on TpM. Thussp is a geodesic symmetry and, sincep was arbitrary,M is a Riemannian symmetric space.

If one starts with a Riemannian symmetric spaceM, 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 ofM.

Classification of Riemannian symmetric spaces

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Main article:List of simple Lie groups

The algebraic description of Riemannian symmetric spaces enabledÉlie Cartan to obtain a complete classification of them in 1926.

For a given Riemannian symmetric spaceM let (G,K,σ,g) be the algebraic data associated to it. To classify the possible isometry classes ofM, first note that theuniversal cover of a Riemannian symmetric space is again Riemannian symmetric, and the covering map is described by dividing the connected isometry groupG of the covering by a subgroup of its center. Therefore, we may suppose without loss of generality thatM is simply connected. (This impliesK is connected by thelong exact sequence of a fibration, becauseG is connected by assumption.)

Classification scheme

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A simply connected Riemannian symmetric space is said to beirreducible 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 spaceM is of one of the following three types:

  1. Euclidean type:M has vanishing curvature, and is therefore isometric to aEuclidean 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 therank, 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 ofsimple Lie groups. For compact type,M is a compact simply connected simple Lie group,G isM×M andK is the diagonal subgroup. For non-compact type,G is a simply connected complex simple Lie group andK is its maximal compact subgroup. In both cases, the rank is therank ofG.

The compact simply connected Lie groups are the universal covers of the classical Lie groups SO(n), SU(n), Sp(n) and the fiveexceptional Lie groupsE6,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 andK is its maximal compact subgroup. Each such example has a corresponding example of compact type, by considering a maximal compact subgroup of the complexification ofG that containsK. More directly, the examples of compact type are classified by involutive automorphisms of compact simply connected simple Lie groupsG (up to conjugation). Such involutions extend to involutions of the complexification ofG, and these in turn classify non-compact real forms ofG.

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.

Classification result

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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 spacesG / K. They are here given in terms ofG andK, together with a geometric interpretation, if readily available. The labelling of these spaces is the one given by Cartan.

LabelGKDimensionRankGeometric interpretation
AISU(n){\displaystyle \mathrm {SU} (n)\,}SO(n){\displaystyle \mathrm {SO} (n)\,}(n1)(n+2)/2{\displaystyle (n-1)(n+2)/2}n1{\displaystyle n-1}Space of real structures onCn{\displaystyle \mathbb {C} ^{n}} that leave the complex determinant invariant
AIISU(2n){\displaystyle \mathrm {SU} (2n)\,}Sp(n){\displaystyle \mathrm {Sp} (n)\,}(n1)(2n+1){\displaystyle (n-1)(2n+1)}n1{\displaystyle n-1}Space of quaternionic structures onC2n{\displaystyle \mathbb {C} ^{2n}} compatible with the Hermitian metric
AIIISU(p+q){\displaystyle \mathrm {SU} (p+q)\,}S(U(p)×U(q)){\displaystyle \mathrm {S} (\mathrm {U} (p)\times \mathrm {U} (q))\,}2pq{\displaystyle 2pq}min(p,q){\displaystyle \min(p,q)}Grassmannian of complexp-dimensional subspaces ofCp+q{\displaystyle \mathbb {C} ^{p+q}}
BDISO(p+q){\displaystyle \mathrm {SO} (p+q)\,}SO(p)×SO(q){\displaystyle \mathrm {SO} (p)\times \mathrm {SO} (q)\,}pq{\displaystyle pq}min(p,q){\displaystyle \min(p,q)}Grassmannian of oriented realp-dimensional subspaces ofRp+q{\displaystyle \mathbb {R} ^{p+q}}
DIIISO(2n){\displaystyle \mathrm {SO} (2n)\,}U(n){\displaystyle \mathrm {U} (n)\,}n(n1){\displaystyle n(n-1)}[n/2]{\displaystyle [n/2]}Space of orthogonal complex structures onR2n{\displaystyle \mathbb {R} ^{2n}}
CISp(n){\displaystyle \mathrm {Sp} (n)\,}U(n){\displaystyle \mathrm {U} (n)\,}n(n+1){\displaystyle n(n+1)}n{\displaystyle n}Space of complex structures onHn{\displaystyle \mathbb {H} ^{n}} compatible with the inner product
CIISp(p+q){\displaystyle \mathrm {Sp} (p+q)\,}Sp(p)×Sp(q){\displaystyle \mathrm {Sp} (p)\times \mathrm {Sp} (q)\,}4pq{\displaystyle 4pq}min(p,q){\displaystyle \min(p,q)}Grassmannian of quaternionicp-dimensional subspaces ofHp+q{\displaystyle \mathbb {H} ^{p+q}}
EIE6{\displaystyle E_{6}\,}Sp(4)/{±I}{\displaystyle \mathrm {Sp} (4)/\{\pm I\}\,}426
EIIE6{\displaystyle E_{6}\,}SU(6)SU(2){\displaystyle \mathrm {SU} (6)\cdot \mathrm {SU} (2)\,}404Space of symmetric subspaces of(CO)P2{\displaystyle (\mathbb {C} \otimes \mathbb {O} )P^{2}} isometric to(CH)P2{\displaystyle (\mathbb {C} \otimes \mathbb {H} )P^{2}}
EIIIE6{\displaystyle E_{6}\,}SO(10)SO(2){\displaystyle \mathrm {SO} (10)\cdot \mathrm {SO} (2)\,}322ComplexifiedCayley projective plane(CO)P2{\displaystyle (\mathbb {C} \otimes \mathbb {O} )P^{2}}
EIVE6{\displaystyle E_{6}\,}F4{\displaystyle F_{4}\,}262Space of symmetric subspaces of(CO)P2{\displaystyle (\mathbb {C} \otimes \mathbb {O} )P^{2}} isometric toOP2{\displaystyle \mathbb {OP} ^{2}}
EVE7{\displaystyle E_{7}\,}SU(8)/{±I}{\displaystyle \mathrm {SU} (8)/\{\pm I\}\,}707
EVIE7{\displaystyle E_{7}\,}SO(12)SU(2){\displaystyle \mathrm {SO} (12)\cdot \mathrm {SU} (2)\,}644Rosenfeld projective plane(HO)P2{\displaystyle (\mathbb {H} \otimes \mathbb {O} )P^{2}} overHO{\displaystyle \mathbb {H} \otimes \mathbb {O} }
EVIIE7{\displaystyle E_{7}\,}E6SO(2){\displaystyle E_{6}\cdot \mathrm {SO} (2)\,}543Space of symmetric subspaces of(HO)P2{\displaystyle (\mathbb {H} \otimes \mathbb {O} )P^{2}} isomorphic to(CO)P2{\displaystyle (\mathbb {C} \otimes \mathbb {O} )P^{2}}
EVIIIE8{\displaystyle E_{8}\,}Spin(16)/{±vol}{\displaystyle \mathrm {Spin} (16)/\{\pm \mathrm {vol} \}\,}1288Rosenfeld projective plane(OO)P2{\displaystyle (\mathbb {O} \otimes \mathbb {O} )P^{2}}
EIXE8{\displaystyle E_{8}\,}E7SU(2){\displaystyle E_{7}\cdot \mathrm {SU} (2)\,}1124Space of symmetric subspaces of(OO)P2{\displaystyle (\mathbb {O} \otimes \mathbb {O} )P^{2}} isomorphic to(HO)P2{\displaystyle (\mathbb {H} \otimes \mathbb {O} )P^{2}}
FIF4{\displaystyle F_{4}\,}Sp(3)SU(2){\displaystyle \mathrm {Sp} (3)\cdot \mathrm {SU} (2)\,}284Space of symmetric subspaces ofOP2{\displaystyle \mathbb {O} P^{2}} isomorphic toHP2{\displaystyle \mathbb {H} P^{2}}
FIIF4{\displaystyle F_{4}\,}Spin(9){\displaystyle \mathrm {Spin} (9)\,}161Cayley projective planeOP2{\displaystyle \mathbb {O} P^{2}}
GG2{\displaystyle G_{2}\,}SO(4){\displaystyle \mathrm {SO} (4)\,}82Space of subalgebras of theoctonion algebraO{\displaystyle \mathbb {O} } which are isomorphic to thequaternion algebraH{\displaystyle \mathbb {H} }

As Grassmannians

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A more modern classification (Huang & Leung 2010) uniformly classifies the Riemannian symmetric spaces, both compact and non-compact, via aFreudenthal magic square construction. The irreducible compact Riemannian symmetric spaces are, up to finite covers, either a compact simple Lie group, a Grassmannian, aLagrangian Grassmannian, or adouble Lagrangian Grassmannian of subspaces of(AB)n,{\displaystyle (\mathbf {A} \otimes \mathbf {B} )^{n},} for normed division algebrasA andB. A similar construction produces the irreducible non-compact Riemannian symmetric spaces.

General symmetric spaces

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An important class of symmetric spaces generalizing the Riemannian symmetric spaces arepseudo-Riemannian symmetric spaces, in which the Riemannian metric is replaced by apseudo-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 ingeneral relativity, the most notable examples beingMinkowski space,De Sitter space andanti-de Sitter space (with zero, positive and negative curvature respectively). De Sitter space of dimensionn may be identified with the 1-sheeted hyperboloid in a Minkowski space of dimensionn + 1.

Symmetric and locally symmetric spaces in general can be regarded as affine symmetric spaces. IfM =G / H is a symmetric space, then Nomizu showed that there is aG-invariant torsion-freeaffine connection (i.e. an affine connection whosetorsion tensor vanishes) onM whosecurvature isparallel. Conversely a manifold with such a connection is locally symmetric (i.e., itsuniversal 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.

Classification results

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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 spaceG / H with Lie algebra

g=hm{\displaystyle {\mathfrak {g}}={\mathfrak {h}}\oplus {\mathfrak {m}}}

is said to be irreducible ifm{\displaystyle {\mathfrak {m}}} is anirreducible representation ofh{\displaystyle {\mathfrak {h}}}. Sinceh{\displaystyle {\mathfrak {h}}} is not semisimple (or even reductive) in general, it can haveindecomposable representations which are not irreducible.

However, the irreducible symmetric spaces can be classified. As shown byKatsumi Nomizu, there is a dichotomy: an irreducible symmetric spaceG / H is either flat (i.e., an affine space) org{\displaystyle {\mathfrak {g}}} 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 withg{\displaystyle {\mathfrak {g}}} semisimple) and determine which of these are irreducible. The latter question is more subtle than in the Riemannian case: even ifg{\displaystyle {\mathfrak {g}}} is simple,G / H might not be irreducible.

As in the Riemannian case there are semisimple symmetric spaces withG =H ×H. Any semisimple symmetric space is a product of symmetric spaces of this form with symmetric spaces such thatg{\displaystyle {\mathfrak {g}}} is simple. It remains to describe the latter case. For this, one needs to classify involutionsσ of a (real) simple Lie algebrag{\displaystyle {\mathfrak {g}}}. Ifgc{\displaystyle {\mathfrak {g}}^{c}} is not simple, theng{\displaystyle {\mathfrak {g}}} is a complex simple Lie algebra, and the corresponding symmetric spaces have the formG / H, whereH is a real form ofG: these are the analogues of the Riemannian symmetric spacesG / K withG a complex simple Lie group, andK a maximal compact subgroup.

Thus we may assumegc{\displaystyle {\mathfrak {g}}^{c}} is simple. The real subalgebrag{\displaystyle {\mathfrak {g}}} may be viewed as the fixed point set of a complexantilinear involutionτ ofgc{\displaystyle {\mathfrak {g}}^{c}}, whileσ extends to a complex antilinear involution ofgc{\displaystyle {\mathfrak {g}}^{c}} commuting withτ and hence also a complex linear involutionστ.

The classification therefore reduces to the classification of commuting pairs of antilinear involutions of a complex Lie algebra. The compositeστ determines a complex symmetric space, whileτ determines a real form. From this it is easy to construct tables of symmetric spaces for any givengc{\displaystyle {\mathfrak {g}}^{c}}, and furthermore, there is an obvious duality given by exchangingσ andτ. This extends the compact/non-compact duality from the Riemannian case, where eitherσ orτ is aCartan involution, i.e., its fixed point set is a maximal compact subalgebra.

Tables

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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(,C)),k + =nGc / Sp(n,C),n even
G = SL(n,R)G / SO(k,l)G / S(GL(k,R)×GL(l,R))
orG / GL(n/2,C),n even
G / Sp(n,R),n even
G = SU(p,q),p +q =nG / SO(p,q)
or SU(p,p) / Sk(p,H)
G / S(U(kp,kq)×U(lp,lq))
or SU(p,p) / GL(p,C)
G / Sp(p/2,q/2),p,q even
or SU(p,p) / Sp(2p,R)
G = SL(n/2,H),n evenG / Sk(n/2,H)G / S(GL(k/2,H)×GL(/2,H)),k, even
orG / GL(n/2,C)
G / Sp(k/2,/2),k, even,k + =n
Gc=SO(n,C)Gc / SO(k,C)×SO(,C),k + =nGc / GL(n/2,C),n even
G=SO(p,q)G / SO(kp,kq)×SO(p,lq)
or SO(n,n) / SO(n,C)
G / U(p/2,q/2),p,q even
or SO(n,n) / GL(n,R)
G = Sk(n/2,H),n evenG / Sk(k/2,/2),k, even
orG / SO(n/2,C)
G / U(k/2,/2),k, even
orG / SL(n/4,H)
Gc = Sp(2n,C)Gc / Sp(2k,C)×Sp(2,C),k +  = nGc / GL(n,C)
G = Sp(p,q),p + q = nG / Sp(kp,kq)×Sp(p,q)
or Sp(n,n) / Sp(n,C)
G / U(p,q)
or Sp(p,p) / GL(p,H)
G = Sp(2n,R)G / Sp(2k,R)×Sp(2l,R)
orG / Sp(n,C)
G / U(k,),k +  = n
orG / GL(n,R)

For exceptional simple Lie groups, the Riemannian case is included explicitly below, by allowingσ to be the identity involution (indicated by a dash). In the above tables this is implicitly covered by the casekl = 0.

G2cG2c / SL(2,C)× SL(2,C)
G2G2 / SU(2)×SU(2)
G2(2)G2(2) / SU(2)×SU(2)G2(2) / SL(2,R)× SL(2,R)
F4cF4c / Sp(6,C)×Sp(2,C)F4c / SO(9,C)
F4F4 / Sp(3)×Sp(1)F4 / SO(9)
F4(4)F4(4) / Sp(3)×Sp(1)F4(4) / Sp(6,R)×Sp(2,R)
or F4(4) / Sp(2,1)×Sp(1)
F4(4) / SO(5,4)
F4(−20)F4(−20) / SO(9)F4(−20) / Sp(2,1)×Sp(1)F4(−20) / SO(8,1)
E6cE6c / Sp(8,C)E6c / SL(6,C)×SL(2,C)E6c / SO(10,C)×SO(2,C)E6c / F4c
E6E6 / Sp(4)E6 / SU(6)×SU(2)E6 / SO(10)×SO(2)E6 / F4
E6(6)E6(6) / Sp(4)E6(6) / Sp(2,2)
or E6(6) / Sp(8,R)
E6(6) / SL(6,R)×SL(2,R)
or E6(6) / SL(3,H)×SU(2)
E6(6) / SO(5,5)×SO(1,1)E6(6) / F4(4)
E6(2)E6(2) / SU(6)×SU(2)E6(2) / Sp(3,1)
or E6(2) / Sp(8,R)
E6(2) / SU(4,2)×SU(2)
or E6(2) / SU(3,3)×SL(2,R)
E6(2) / SO(6,4)×SO(2)
or E6(2) / Sk(5,H)×SO(2)
E6(2) / F4(4)
E6(−14)E6(−14) / SO(10)×SO(2)E6(−14) / Sp(2,2)E6(−14) / SU(4,2)×SU(2)
or E6(−14) / SU(5,1)×SL(2,R)
E6(−14) / SO(8,2)×SO(2)
or Sk(5,H)×SO(2)
E6(−14) / F4(−20)
E6(−26)E6(−26) / F4E6(−26) / Sp(3,1)E6(−26) / SL(3,H)×Sp(1)E6(−26) / SO(9,1)×SO(1,1)E6(−26) / F4(−20)
E7cE7c / SL(8,C)E7c / SO(12,C)×Sp(2,C)E7c / E6c×SO(2,C)
E7E7 / SU(8)E7 / SO(12)× Sp(1)E7 / E6× SO(2)
E7(7)E7(7) / SU(8)E7(7) / SU(4,4)
or E7(7) / SL(8,R)
or E7(7) / SL(4,H)
E7(7) / SO(6,6)×SL(2,R)
or E7(7) / Sk(6,H)×Sp(1)
E7(7) / E6(6)×SO(1,1)
or E7(7) / E6(2)×SO(2)
E7(−5)E7(−5) / SO(12)× Sp(1)E7(−5) / SU(4,4)
or E7(−5) / SU(6,2)
E7(−5) / SO(8,4)×SU(2)
or E7(−5) / Sk(6,H)×SL(2,R)
E7(−5) / E6(2)×SO(2)
or E7(−5) / E6(−14)×SO(2)
E7(−25)E7(−25) / E6× SO(2)E7(−25) / SL(4,H)
or E7(−25) / SU(6,2)
E7(−25) / SO(10,2)×SL(2,R)
or E7(−25) / Sk(6,H)×Sp(1)
E7(−25) / E6(−14)×SO(2)
or E7(−25) / E6(−26)×SO(1,1)
E8cE8c / SO(16,C)E8c / E7c×Sp(2,C)
E8E8 / SO(16)E8 / E7×Sp(1)
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

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Main article:Weakly symmetric space

In the 1950sAtle Selberg extended Cartan's definition of symmetric space to that ofweakly symmetric Riemannian space, or in current terminologyweakly symmetric space. These are defined as Riemannian manifoldsM with a transitive connected Lie group of isometriesG and an isometryσ normalisingG such that givenx,y inM there is an isometrys inG such thatsx =σy andsy =σx. (Selberg's assumption thatσ2 should be an element ofG was later shown to be unnecessary byErnest Vinberg.) Selberg proved that weakly symmetric spaces give rise toGelfand pairs, so that in particular theunitary representation ofG onL2(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 pointx inM and tangent vectorX atx, there is an isometrys ofM, depending onx andX, such that

  • s fixesx;
  • the derivative ofs atx sendsX to −X.

Whens is independent ofX,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 complexsemisimple Lie algebras, is given inWolf (2007).

Properties

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Some properties and forms of symmetric spaces can be noted.

Lifting the metric tensor

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Themetric tensor on the Riemannian manifoldM can be lifted to a scalar product onG by combining it with theKilling form. This is done by defining

X,Yg={X,YpX,YTpMmB(X,Y)X,Yh0otherwise{\displaystyle \langle X,Y\rangle _{\mathfrak {g}}={\begin{cases}\langle X,Y\rangle _{p}\quad &X,Y\in T_{p}M\cong {\mathfrak {m}}\\-B(X,Y)\quad &X,Y\in {\mathfrak {h}}\\0&{\mbox{otherwise}}\end{cases}}}

Here,,p{\displaystyle \langle \cdot ,\cdot \rangle _{p}} is the Riemannian metric defined onTpM{\displaystyle T_{p}M}, andB(X,Y)=trace(adXadY){\displaystyle B(X,Y)=\operatorname {trace} (\operatorname {ad} X\circ \operatorname {ad} Y)} is theKilling form. The minus sign appears because the Killing form is negative-definite onh ;{\displaystyle {\mathfrak {h}}~;} this makes,g{\displaystyle \langle \cdot ,\cdot \rangle _{\mathfrak {g}}} positive-definite.

Factorization

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The tangent spacem{\displaystyle {\mathfrak {m}}} can be further factored into eigenspaces classified by the Killing form.[1] This is accomplished by defining an adjoint mapmm{\displaystyle {\mathfrak {m}}\to {\mathfrak {m}}} takingYY#{\displaystyle Y\mapsto Y^{\#}} as

X,Y#=B(X,Y){\displaystyle \langle X,Y^{\#}\rangle =B(X,Y)}

where,{\displaystyle \langle \cdot ,\cdot \rangle } is the Riemannian metric onm{\displaystyle {\mathfrak {m}}} andB(,){\displaystyle B(\cdot ,\cdot )} is the Killing form. This map is sometimes called thegeneralized transpose, as corresponds to the transpose for the orthogonal groups and the Hermitian conjugate for the unitary groups. It is a linear functional, and it is self-adjoint, and so one concludes that there is an orthonormal basisY1,,Yn{\displaystyle Y_{1},\ldots ,Y_{n}} ofm{\displaystyle {\mathfrak {m}}} with

Yi#=λiYi{\displaystyle Y_{i}^{\#}=\lambda _{i}Y_{i}}

These are orthogonal with respect to the metric, in that

Yi#,Yj=λiYi,Yj=B(Yi,Yj)=Yj#,Yi=λjYj,Yi{\displaystyle \langle Y_{i}^{\#},Y_{j}\rangle =\lambda _{i}\langle Y_{i},Y_{j}\rangle =B(Y_{i},Y_{j})=\langle Y_{j}^{\#},Y_{i}\rangle =\lambda _{j}\langle Y_{j},Y_{i}\rangle }

since the Killing form is symmetric. This factorizesm{\displaystyle {\mathfrak {m}}} into eigenspaces

m=m1md{\displaystyle {\mathfrak {m}}={\mathfrak {m}}_{1}\oplus \cdots \oplus {\mathfrak {m}}_{d}}

with

[mi,mj]=0{\displaystyle [{\mathfrak {m}}_{i},{\mathfrak {m}}_{j}]=0}

forij{\displaystyle i\neq j}. For the case ofg{\displaystyle {\mathfrak {g}}} semisimple, so that the Killing form is non-degenerate, the metric likewise factorizes:

,=1λ1B|m1++1λdB|md{\displaystyle \langle \cdot ,\cdot \rangle ={\frac {1}{\lambda _{1}}}\left.B\right|_{{\mathfrak {m}}_{1}}+\cdots +{\frac {1}{\lambda _{d}}}\left.B\right|_{{\mathfrak {m}}_{d}}}

In certain practical applications, this factorization can be interpreted as the spectrum of operators,e.g. the spectrum of the hydrogen atom, with the eigenvalues of the Killing form corresponding to different values of the angular momentum of an orbital (i.e. the Killing form being aCasimir operator that can classify the different representations under which different orbitals transform.)

Classification of symmetric spaces proceeds based on whether or not the Killing form is definite.

Applications and special cases

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Symmetric spaces and holonomy

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Main article:Holonomy group

If the identity component of theholonomy 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 of7 families.

Hermitian symmetric spaces

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Main article:Hermitian symmetric space

A Riemannian symmetric space that is additionally equipped with a parallel complex structure compatible with the Riemannian metric is called aHermitian 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 spaceG / K is Hermitian if and only ifK contains a central circle. A quarter turn by this circle acts as multiplication byi 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 withp = 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

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Main article:Quaternion-Kähler symmetric space

A Riemannian symmetric space that 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 calledquaternion-Kähler symmetric space.

An irreducible symmetric spaceG / K is quaternion-Kähler if and only if isotropy representation ofK contains an Sp(1) summand acting like theunit quaternions on aquaternionic 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 withp = 2 orq = 2 (these are isomorphic), BDI withp = 4 orq = 4, CII withp = 1 orq = 1, EII, EVI, EIX, FI and G.

Bott periodicity theorem

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Main article:Bott periodicity theorem

In theBott periodicity theorem, theloop spaces of the stableorthogonal group can be interpreted as reductive symmetric spaces.

See also

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References

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  1. ^Jurgen Jost, (2002) "Riemannian Geometry and Geometric Analysis", Third edition, Springer(See section 5.3, page 256)
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