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I recently learned from Jim Carlson’s blog of the passing of Harsh Pittie on January 16 this year. I never met Harsh, but he is very familiar to me through his work, in particular for his classic book Characteristic classes of foliations. I first encountered this book as a graduate student, late last millenium. The book has several features which make it very attractive. First of all, it is short — only 105 pages. My strong instinct is always to read books cover-to-cover from start to finish, and the motivated reader can go through Harsh’s book in its entirety in maybe 4 hours. Second of all, the exposition is quite lovely: an excellent balance is struck between providing enough details to meet the demands of rigor, and sustaining the arc of an idea so that the reader can get the point. Third of all, the book achieves a difficult synthesis of two “opposing” points of view, namely the (differential-)geometric and the algebraic. In fact, this achievement is noted and praised in the MathSciNet review of the book (linked above) by Dmitri Fuks.
The purpose of this blog post is to try to give some insight into the “meaning” of the Hall-Witt identity in group theory. This identity can look quite mysterious in its algebraic form, but there are several ways of describing it geometrically which are more natural and easier to understand.
If is a group, and
are elements of
, the commutator of
and
(denoted
) is the expression
(note: algebraists tend to use the convention that
instead). Commutators (as their name suggests) measure the failure of a pair of elements to commute, in the sense that
. Since
, the property of being a commutator is invariant under conjugation (here the superscript
means conjugation by
; i.e.
; again, the algebraists use the opposite convention).
I am (update: was) currently (update: but am no longer) in Brisbane for the “New directions in geometric group theory” conference, which has been an entirely enjoyable and educational experience. I got to eat fish and chips, to watch Australia make 520 for 7 (declared) against the West Indies at the WACA, and to hear Masato Mimura give a very nice talk about his recent results on rigidity of the “universal lattice”.
His talk included a quick and beautiful survey of some geometric aspects of the theory of rigidity for infinite groups, which I will attempt to partially reproduce (despite the limitations of the wordpress format). In this context, rigidity is expressed in terms of isometric affine actions of groups on Banach spaces. This means the following. Suppose is a Banach space (i.e. a complete, normed vector space) and
is a group. A linear isometric action is a representation
from
to the group of linear isometries of
— i.e. linear norm-preserving automorphisms. An affine action is a representation from
to the group of affine isometries of
— i.e. isometries as a metric space that do not necessarily fix the zero element. The group of isometries of a Banach space
is a semi-direct product
where
is the group of linear isometries, and
is the Banach space, thought of as an Abelian group, acting on itself by (isometric) translations. Such an action is usually encoded by a pair
which records the “linear” part of the action, and a 1-cocycle with coefficients in
, i.e. a function
satisfying
for every
. This formula might look strange if you don’t know where it comes from: it is just the way that factors transform in semi-direct products. The affine action is given by sending
to the transformation that sends each
to
. Consequently,
is sent to the transformation that sends
to
and the fact that this is a group action becomes the formula
Equating the left and right hand sides gives the cocycle condition. Given one affine isometric action, one can obtain another in a silly way by conjugating by an isometry for some
. Under conjugation by such an isometry, a cocycle
transforms by
. A function of the form
is called a 1-coboundary, and the quotient of the space of 1-cocycles by the space of 1-coboundaries is the 1 dimensional cohomology of
with coefficients in
. This is usually denoted
, where
is suppressed in the notation. In particular, an affine isometric action of
on
with linear part
has a global fixed point iff it represents
in
. Contrapositively,
admits an affine isometric action on
without a global fixed point iff
for some
.
A group is said to satisfy Serre’s Property (FH) if every affine isometric action of
on a Hilbert space has a global fixed point. In 2007, Bader-Furman-Gelander-Monod introduced a property (FB) for a group
to mean that every affine isometric action of
on some (out of a class of) Banach space(s)
has a global fixed point. Mimura used the notation property (FL_p) for the case that
is allowed to range over the class of
spaces (for some fixed
).
Intimately related is Kazhdan’s Property (T), introduced by Kazhdan in this paper. Let be a locally compact topological group (for example, a discrete group). The set of irreducible unitary representations of
is called its dual, and denoted
. This dual is topologized in the following way. Associated to a representation
, a unit vector
, a positive number
and a compact subset
there is an open neighborhood of
consisting of representations
for which there is a unit vector
such that
whenever
. With this topology (called the Fell topology), one says that a group
has property (T) if the trivial representation is isolated in
. Note that this topology is very far from being Hausdorff: the trivial representation fails to be isolated exactly when there are a sequence of representations
, unit vectors
, numbers
and compact sets
exhausting
so that
for any
. The vectors
are said to be (a sequence of) almost invariant vectors. Hence (informally) a group has property (T) if some compact subset must move some unit vector a definite amount in every irreducible nontrivial unitary representation. If a group fails to have property (T), one can rescale a sequence of irreducible actions near a sequence of almost invariant vectors in such a way that one obtains in the geometric limit a nontrivial isometric action on
without a global fixed point. A famous theorem of Delorme-Guichardet says that property (T) and property (FH) are equivalent for (locally compact second countable) groups. Property (T) passes to quotients, and to lattices (i.e. finite covolume discrete subgroups of a topological group). Kazhdan already showed in his paper that
has property (T) for
at least
, and therefore the same is true for lattices in this groups, such as
, a fact which is not easy to see directly from the definition. One beautiful application, already pointed out by Kazhdan, is that this means that all lattices in
, for instance the groups
(and in fact, all discrete groups with property (T)) are finitely generated. Kazhdan’s proof of this is incredibly short: let
be a discrete group and
and sequence of elements. For each
, let
be the subgroup of
generated by
. Notice that
is finitely generated iff
for all sufficiently large
. On the other hand, consider the unitary representations of
induced by the trivial representations on the
. Every compact subset of
is finite, and therefore eventually fixes a vector in every one of these representations; thus there is a sequence of almost fixed vectors. If
has property (T), this sequence eventually contains a fixed vector, which can only happen if
is finite, in which case
is finitely generated, as claimed.
Property (FL_p) generalizes (FH) (equivalently (T)) in many significant ways, with interesting applications to dynamics. For example, Navas showed that if is a group with property (T) then every action of
on a circle which is at least
factors through a finite group. Navas’s argument can be generalized straightforwardly to show that if
has (FL_p) for some
then every action of
on a circle which is at least
factors through a finite group. The proof rests on a beautiful construction due to Reznikov (although a similar construction can be found in Pressley-Segal) of certain functions on a configuration space of the circle which are not in
but have coboundaries which are; this gives rise to nontrivial cohomology with
coefficients for groups acting on the circle in a sufficiently interesting way.
(Update: Nicolas Monod points out in an email that the “function on a configuration space” is morally just the derivative. In fact, he made the nice remark that if is any elliptic operator on an
-manifold, then the commutator
is of Schatten class
whenever
is a sufficiently smooth function; morally this should give rise to nontrivial cohomology with suitable coefficients for groups acting with enough regularity on any given
-manifold, and one would like to use this e.g. to approach Zimmer’s conjecture, but nobody seems to know how to make this work as yet; in fact the work of Monod et. al. on (FL_p) is at least partly motivated by this general picture.)
Mimura discussed a spectrum of rigid behaviour for infinite groups, ranging from most rigid (property (FL_p) for every ) to least rigid (amenable) (note: every finite group is both amenable and has property (T), so this only really makes sense for infinite groups; moreover, every reasonable measure of rigidity for infinite groups is usually invariant under passing to subgroups of finite index). Free groups,
and so on are very non-rigid. However, it is well-known that certain infinite families of (word) hyperbolic groups, including lattices in groups of isometries of quaternion-hyperbolic symmetric spaces, and “random” groups with relations having density parameter
(see Zuk or Ollivier) are both hyperbolic and have property (T). Nevertheless, these groups are not as rigid as higher rank lattices like
for
. The latter have property (FL_p) for every
, whereas Yu showed that every hyperbolic group admits a proper affine isometric action on
for some
(the existence of a proper affine isometric action on a Hilbert space is called “a-T-menability” by Gromov, and the “Haagerup property” by some. Groups satisfying this property, or even Yu’s weaker property, are known to satisfy some version of the Baum-Connes conjecture, the subject of a very nice minicourse by Graham Niblo at the same conference).
It is in this context that one can appreciate Mimura’s results. His first main result is that the group (i.e. the “universal lattice”) has property (FL_p) for every
provided
is at least 4. Since property (FL_p) (like (T)) passes to quotients, this implies that
has (FL_p) for every unital, commutative, finitely generated ring
.
His second main result concerns a “quasification” of FL_p, to a property called (FFL_p). Without getting too technical, this property concerns “quasi-actions” of a group on a Banach space by affine isometries; algebraically these are encoded by 1-cochains for which there is a universal constant
so that
as measured in the Banach norm on
. Any bounded map
defines a 1-cochain; such (bounded) 1-cochains corresponds to quasi-action with a bounded orbit. Associated to
one defines in a similar way a complex of bounded cochains; quasi-actions modulo bounded quasi-actions are parameterized by the kernel of the comparison map
from bounded to ordinary cohomology. Mimura’s second main result is that when
is the universal lattice as above, and
has no invariant vectors, the comparison map from bounded to ordinary cohomology in dimension 2 is injective.
The fact that as above is required to have no invariant vectors is a technical necessity of Mimura’s proof. When
is trivial, one is studying “ordinary” bounded cohomology, and there is an exact sequence
with real coefficients for any (here
denotes the vector space of homogeneous quasimorphisms on
). In this context, one knows by Bavard duality that
is injective if and only if the stable commutator length is identically zero on
. By quite a different method, Mimura shows that for
at least
, and for any Euclidean ring
(i.e. a ring for which one has a Euclidean algorithm; for example,
) the group
has vanishing stable commutator length, and therefore one has injectivity of bounded to ordinary cohomology in dimension
.
(Update 1/9/2010): Nicholas Monod sent me a nice email commenting on a couple of points in this blog entry, and I have consequently modified the language a bit in a few places. Ta much!
On page 10 of Besse’s famous book on Einstein manifolds one finds the following quote:
It would seem that Riemannian and Lorentzian geometry have much in common: canonical connections, geodesics, curvature tensor, etc. . . . But in fact this common part is only a common disposition at the onset: one soon enters different realms.
I will not dispute this. But it is not clear to me whether this divergence is a necessary consequence of the nature of the objects of study (in either case), or an artefact of the schism between mathematics and physics during much of the 20th century. In any case, in this blog post I have the narrow aim of describing some points of contact between Lorentzian (and more generally, causal) geometry and other geometries (hyperbolic, symplectic), which plays a significant role in some of my research.
The first point of contact is the well-known duality between geodesics in the hyperbolic plane and points in the (projectivized) “anti de-Sitter plane”. Let denote a
-dimensional vector space equipped with a quadratic form
If we think of the set of rays through the origin as a copy of the real projective plane , the hyperbolic plane is the set of projective classes of vectors
with
, the (projectivized) anti de-Sitter plane is the set of projective classes of vectors
with
, and their common boundary is the set of projective classes of (nonzero) vectors
with
. Topologically, the hyperbolic plane is an open disk, the anti de-Sitter plane is an open Möbius band, and their boundary is the “ideal circle” (note: what people usually call the anti de-Sitter plane is actually the annulus double-covering this Möbius band; this is like the distinction between spherical geometry and elliptic geometry). Geometrically, the hyperbolic plane is a complete Riemannian surface of constant curvature
, whereas the anti de-Sitter plane is a complete Lorentzian surface of constant curvature
.
In this projective model, a hyperbolic geodesic is an open straight line segment which is compactified by adding an unordered pair of points in the ideal circle. The straight lines in the anti de-Sitter plane tangent to the ideal circle at these two points intersect at a point
. Moreover, the set of geodesics
in the hyperbolic plane passing through a point
are dual to the set of points
in the anti de-Sitter plane that lie on a line which does not intersect the ideal circle. In the figure, three concurrent hyperbolic geodesics are dual to three colinear anti de-Sitter points.

The anti de-Sitter geometry has a natural causal structure. There is a cone field whose extremal vectors at every point are tangent to the straight lines through
that are also tangent to the ideal circle. A smooth curve is timelike if its tangent at every point is supported by this cone field, and spacelike if its tangent is everywhere not supported by the cone field. A timelike curve corresponds to a family of hyperbolic geodesics which locally intersect each other; a spacelike curve corresponds to a family of disjoint hyperbolic geodesics that foliate some region.
One can distinguish (locally) between future and past along a timelike trajectory, by (arbitrarily) identifying the “future” direction with a curve which winds positively around the ideal circle. The fact that one can distinguish in a consistent way between the positive and negative direction is equivalent to the existence of a nonzero section of timelike vectors. On the other hand, there does not exist a nonzero section of spacelike vectors, so one cannot distinguish in a consistent way between left and right (this is a manifestation of the non-orientability of the Möbius band).
The duality between the hyperbolic plane and the anti de-Sitter plane is a manifestation of the fact that (at least at the level of Lie algebras) they have the same (infinitesimal) symmetries. Let denote the group of real
matrices which preserve
; i.e. matrices
for which
for all vectors
. This contains a subgroup
of index
which preserves the “positive sheet” of the hyperboloid
, and acts on it in an orientation-preserving way. The hyperbolic plane is the homogeneous space for this group whose point stabilizers are a copy of
(which acts as an elliptic “rotation” of the tangent space to their common fixed point). The anti de-Sitter plane is the homogeneous space for this group whose point stabilizers are a copy of
(which acts as a hyperbolic “translation” of the geodesic in hyperbolic space dual to the given point in anti de-Sitter space). The ideal circle is the homogeneous space whose point stabilizers are a copy of the affine group of the line. The hyperbolic plane admits a natural Riemannian metric, and the anti de-Sitter plane a Lorentz metric, which are invariant under these group actions. The causal structure on the anti de-Sitter plane limits to a causal structure on the ideal circle.
Now consider the -dimensional vector space
and the quadratic form
. The (
-dimensional) sheets
and
both admit homogeneous Lorentz metrics whose point stabilizers are copies of
and
(which are isomorphic but sit in
in different ways). These
-manifolds are compactified by adding the projectivization of the cone
. Topologically, this is a Clifford torus in
dividing this space into two open solid tori which can be thought of as two Lorentz
-manifolds. The causal structure on the pair of Lorentz manifolds limits to a pair of complementary causal structures on the Clifford torus. (edited 12/10)
Let’s go one dimension higher, to the -dimensional vector space
and the quadratic form
. Now only the sheet
is a Lorentz manifold, whose point stabilizers are copies of
, with an associated causal structure. The projectivized cone
is a non-orientable twisted
bundle over the circle, and it inherits a causal structure in which the sphere factors are spacelike, and the circle direction is timelike. This ideal boundary can be thought of in quite a different way, because of the exceptional isomorphism at the level of (real) Lie algebras
, where
denotes the Lie algebra of the symplectic group in dimension
. In this manifestation, the ideal boundary is usually denoted
, and can be thought of as the space of Lagrangian planes in
with its usual symplectic form. One way to see this is as follows. The wedge product is a symmetric bilinear form on
with values in
. The associated quadratic form vanishes precisely on the “pure”
-forms — i.e. those associated to planes. The condition that the wedge of a given
-form with the symplectic form vanishes imposes a further linear condition. So the space of Lagrangian
-planes is a quadric in
, and one may verify that the signature of the underlying quadratic form is
. The causal structure manifests in symplectic geometry in the following way. A choice of a Lagrangian plane
lets us identify symplectic
with the cotangent bundle
. To each symmetric homogeneous quadratic form
on
(thought of as a smooth function) is associated a linear Lagrangian subspace of
, namely the (linear) section
. Every Lagrangian subspace transverse to the fiber over
is of this form, so this gives a parameterization of an open, dense subset of
containing the point
. The set of positive definite quadratic forms is tangent to an open cone in
; the field of such cones as
varies defines a causal structure on
which agrees with the causal structure defined above.
These examples can be generalized to higher dimension, via the orthogonal groups or the symplectic groups
. As well as two other infinite families (which I will not discuss) there is a beautiful “sporadic” example, connected to what Freudenthal called octonion symplectic geometry associated to the noncompact real form
of the exceptional Lie group, where the ideal boundary
has an invariant causal structure whose timelike curves wind around the
factor; see e.g. Clerc-Neeb for a more thorough discussion of the theory of Shilov boundaries from the causal geometry point of view, or see here or here for a discussion of the relationship between the octonions and the exceptional Lie groups.
The causal structure on these ideal boundaries gives rise to certain natural -cocycles on their groups of automorphisms. Note in each case that the ideal boundary has the topological structure of a bundle over
with spacelike fibers. Thus each closed timelike curve has a well-defined winding number, which is just the number of times it intersects any one of these spacelike slices. Let
be an ideal boundary as above, and let
denote the cyclic cover dual to a spacelike slice. If
is a point in
, we let
denote the image of
under the
th power of the generator of the deck group of the covering. If
is a homeomorphism of
preserving the causal structure, we can lift
to a homeomorphism
of
. For any such lift, define the rotation number of
as follows: for any point
and any integer
, let
be the the smallest integer for which there is a causal curve from
to
to
, and then define
. This function is a quasimorphism on the group of causal automorphisms of
, with defect equal to the least integer
such that any two points
in
are contained in a closed causal loop with winding number
. In the case of the symplectic group
with causal boundary
, the defect is
, and the rotation number is (sometimes) called the symplectic rotation number; it is a quasimorphism on the universal central extension of
, whose coboundary descends to the Maslov class (an element of
-dimensional bounded cohomology) on the symplectic group.
Causal structures in groups of symplectomorphisms or contactomorphisms are intensely studied; see for instance this paper by Eliashberg-Polterovich.
A geometric structure on a manifold is an atlas of charts with values in some kind of “model space”, and transformation functions taken from some pseudogroup of transformations on the model space. If is the model space, and
is the pseudo-group, one talks about a
-structure on a manifold
. One usually (but not always) wants
to be homogeneous with respect to
. So, for instance, one talks about smooth structures, conformal structures, projective structures, bilipschitz structures, piecewise linear structures, symplectic structures, and so on, and so on. Riemannian geometry does not easily fit into this picture, because there are so few (germs of) isometries of a typical Riemannian metric, and so many local invariants; but Riemannian metrics modeled on a locally symmetric space, with
a Lie group of symmetries of
, are a very significant example.
Sometimes the abstract details of a theory are hard to grasp before looking at some fundamental examples. The case of geometric structures on -manifolds is a nice example, which is surprisingly rich in some ways.
One of the most important ways in which geometric structures arise is in the theory of ODE’s. Consider a first order ODE in one variable, e.g. an equation like
- Indefinite integral
. The group in this case is
, acting on
by translation. The equation is solved by integrating:
.
- Linear homogeneous ODE
. The group in this case is
, acting on
by multiplication (notice that this group action is not transitive; the point
is preserved; this corresponds to the fact that
is always a solution of a homogeneous linear ODE). The Lie algebra is
, and the ODE is “solved” by exponentiating the vector field, and integrating. Hence
is the general solution. In fact, in the previous example, the Lie algebra of the group of translations is also identified with
, and “exponentiating” is the identity map.
- Linear inhomogeneous ODE
. The group in this case is the affine group
where the first factor acts by dilations and the second by translation. The affine group is not abelian, so one cannot “integrate” a vector field directly, but it is solvable: there is a short exact sequence
. The image in the Lie algebra of the group of dilations is the term
, which can be integrated as before to give an integrating factor
. Setting
gives
which is an indefinite integral, and can be solved by a further integration. In other words, we do one integration to change the structure group from
to
(“integrating out” the group of dilations) and then what is left is an abelian structure group, in which we can do “ordinary” integration. This procedure works whenever the structure group is solvable; i.e. whenever there is a finite sequence
where each
surjects onto an abelian group, with kernel
, and after finitely many steps, the last kernel is trivial.
- Ricatti equation
. In this case, it is well-known that the equation can blow up in finite time, and one does not obtain a group of transformations of
, but rather a group of transformations of the projective line
; another point of view says that one obtains a pseudogroup of transformations of subsets of
. The group in this case is the projective group
, acting by projective linear transformations. Let
be a
-parameter family of matrices in
, say
, with
. Matrices act on
by fractional linear maps; that is,
for
. Differentiating
at
one obtains
which is the general form of the Ricatti equation. Since the group
is not solvable, the Ricatti equation cannot be solved in terms of elementary functions and integrals. However, if one knows one solution
, one can find all other solutions as follows. Do a change of co-ordinates, by sending the solution
“to infinity”; i.e. define
. Then as a function of
, the Ricatti equation reduces to a linear inhomogeneous ODE. In other words, the structure group reduces to the subgroup of
fixing the point at infinity (i.e. the solution
), which is the affine group
. One can therefore solve for
, and by substituting back, for
.
The Ricatti equation is important for the solution of second order linear equations, since any second order linear equation can be transformed into a system of two first order linear equations in the variables
and
. A system of first order ODEs in
variables can be described in terms of pseudogroups of transformations of (subsets of)
. A system of linear equations corresponds to the structure group
, hence in the case of a
system, to
. The determinant map is a homomorphism from
to
with kernel
; hence, after multiplication by a suitable integrating factor, one can reduce to a system which is (equivalent to) the Ricatti equation.
Having seen these examples, one naturally wonders whether there are any other interesting families of equations and corresponding Lie groups acting on -manifolds. In fact, there are (essentially) no other examples: if one insists on (finite dimensional) simple Lie groups, then
is more or less the only example. Perhaps this is one of the reasons why the theory of ODEs tends to appear to undergraduates (and others) as an unstructured collection of rules and tricks. Nevertheless, recasting the theory in terms of geometric structures has the effect of clearing the air to some extent.
Geometric structures on
A third significant way in which geometric structures arise on circles is in the theory of conformal welding. Let
This list of examples of geometric structures on
I was in Stony Brook last week, visiting Moira Chas and Dennis Sullivan, and have been away from blogging for a while; this week I plan to write a few posts about some of the things I discussed with Moira and Dennis. This is an introductory post about the Goldman bracket, an extraordinary mathematical object made out of the combinatorics of immersed curves on surfaces. I don’t have anything original to say about this object, but for my own benefit I thought I would try to explain what it is, and why Goldman was interested in it.
In his study of symplectic structures on character varieties , where
is the fundamental group of a closed oriented surface and
is a Lie group satisfying certain (quite general) conditions, Bill Goldman discovered a remarkable Lie algebra structure on the free abelian group generated by conjugacy classes in
. Let
denote the set of homotopy classes of closed oriented curves on
, where
is itself a compact oriented surface, and let
denote the free abelian group with generating set
. If
are immersed oriented closed curves which intersect transversely (i.e. in double points), define the formal sum
In this formula, are
thought of as based loops at the point
,
represents their product in
, and
represents the resulting conjugacy class in
. Moreover,
is the oriented intersection number of
and
at
.
This operation turns out to depend only on the free homotopy classes of and
, and extends by linearity to a bilinear map
. Goldman shows that this bracket makes
into a Lie algebra over
, and that there are natural Lie algebra homomorphisms from
to the Lie algebra of functions on
with its Poisson bracket.
The connection with character varieties can be summarized as follows. Let be a (smooth) class function (i.e. a function which is constant on conjugacy classes) on a Lie group
. Define the variation function
by the formula
where is some (fixed)
-invariant orthogonal structure on the Lie algebra
(for example, if
is reductive (eg if
is semisimple), one can take
). The tangent space to the character variety
at
is the first cohomology group of
with coefficients in
, thought of as a
module with the
action, and then as a
module by the representation
. Cup product and the pairing
determine a pairing
where the last equality uses the fact that is a closed surface group; this pairing defines the symplectic structure on
.
Every element determines a function
by sending a (conjugacy class of) representation
to
. Note that
only depends on the conjugacy class of
in
. It is natural to ask: what is the Hamiltonian flow on
generated by the function
? It turns out that when
is a simple closed curve, it is very easy to describe this Hamiltonian flow. If
is nonseparating, then define a flow
by
when
is represented by a curve disjoint from
, and
if
intersects
exactly once with a positive orientation (there is a similar formula when
is separating). In other words, the representation is constant on the fundamental group of the surface “cut open” along the curve
, and only deforms in the way the two conjugacy classes of
in the cut open surface are identified in
.
In the important motivating case that , so that one component of
is the Teichmüller space of hyperbolic structures on the surface
, one can take
, and then
is just the length of the geodesic in the free homotopy class of
, in the hyperbolic structure on
associated to a representation. In this case, the symplectic structure on the character variety restricts to the Weil-Petersson symplectic structure on Teichmüller space, and the Hamiltonian flow associated to the length function
is a family of Fenchel-Nielsen twists, i.e. the deformations of the hyperbolic structure obtained by cutting along the geodesic
, rotating through some angle, and regluing. This latter observation recovers a famous theorem of Wolpert, connected in an obvious way to his formula for the symplectic form
where
is angle and
is length, and the sum is taken over a maximal system of disjoint essential simple curves
for the surface
.
The combinatorial nature of the Goldman bracket suggests that it might have applications in combinatorial group theory. Turaev discovered a Lie cobracket on , and showed that together with the Goldman bracket, one obtains a Lie bialgebra. Motivated by Stallings’ reformulation of the Poincaré conjecture in terms of group theory, Turaev asked whether a free homotopy class contains a power of a simple curve if and only if the cobracket of the class is zero. The answer to this question is negative, as shown by Chas; on the other hand, Chas and Krongold showed that a class
is simple if and only if
is zero. Nevertheless, the full geometric meaning of the Goldman bracket remains mysterious, and a topic worthy of investigation.

Hyperbolic Geometry (157b) Notes #1
April 8, 2010 in Commentary, Euclidean Geometry, Groups, Hyperbolic geometry, Lie groups, Overview, Visualization | by aldenwalker | 5 comments
I am Alden, one of Danny’s students. Error/naivete that may (will) be found here is mine. In these posts, I will attempt to give notes from Danny’s class on hyperbolic geometry (157b). This first post covers some models for hyperbolic space.
1. Models
We have a very good natural geometric understanding of
, i.e. 3-space with the euclidean metric. Pretty much all of our geometric and topological intuition about manifolds (Riemannian or not) comes from finding some reasonable way to embed or immerse them (perhaps locally) in
. Let us look at some examples of 2-manifolds.
The Tractrix
The surface of revolution about the
-axis is the pseudosphere, an isometric embedding of a surface of constant curvature -1. Like the sphere, there are some isometries of the pseudosphere that we can understand as isometries of
, namely rotations about the
-axis. However, there are lots of isometries which do not extend, so this embeddeding does not serve us all that well.
That last example is the important one to consider when thinking about hypobolic spaces. Intuitively, manifolds with negative curvature have a hard time fitting in euclidean space because volume grows too fast — there is not enough room for them. The solution is to find (local, or global in the case of
) models for hyperbolic manfolds such that the geometry is distorted from the usual euclidean geometry, but the isometries of the space are clear.
2. 1-Dimensional Models for Hyperbolic Space
While studying 1-dimensional hyperbolic space might seem simplistic, there are nice models such that higher dimensions are simple generalizations of the 1-dimensional case, and we have such a dimensional advantage that our understanding is relatively easy.
2.1. Hyperboloid Model
Parameterizing
Consider the quadratic form
on
defined by
, where
. This doesn’t give a norm, since
is not positive definite, but we can still ask for the set of points
with
. This is (both sheets of) the hyperbola
. Let
be the upper sheet of the hyperbola. This will be 1-dimensional hyperbolic space.
For any
matrix
, let
. That is, matrices which preserve the form given by
. The condition is equivalent to requiring that
. Notice that if we let
be the identity matrix, we would get the regular orthogonal group. We define
, where
has
positive eigenvalues and
negative eigenvalues. Thus
. We similarly define
to be matricies of determinant 1 preserving
, and
to be the connected component of the identity.
is then the group of matrices preserving both orientation and the sheets of the hyperbolas.
We can find an explicit form for the elements of
. Consider the matrix
. Writing down the equations
and
gives us four equations, which we can solve to get the solutions
Since we are interested in the connected component of the identity, we discard the solution on the right. It is useful to do a change of variables
, so we have (recall that
).
These matrices take
to
. In other words,
acts transitively on
with trivial stabilizers, and in particular we have parmeterizing maps
The first map is actually a Lie group isomorphism (with the group action on
being
) in addition to a diffeomorphism, since
Metric
As mentioned above,
is not positive definite, but its restriction to the tangent space of
is. We can see this in the following way: tangent vectors at a point
are characterized by the form
. Specifically,
, since (by a calculation)
. Therefore,
takes tangent vectors to tangent vectors and preserves the form (and is transitive), so we only need to check that the form is positive definite on one tangent space. This is obvious on the tangent space to the point
. Thus,
is a Riemannian manifold, and
acts by isometries.
Let’s use the parameterization
. The unit (in the
metric) tangent at
is
. The distance between the points
and
is
In other words,
is an isometry from
to
.
1-dimensional hyperbollic space. The hyperboloid model is shown in blue, and the projective model is shown in red. An example of the projection map identifying
with
is shown.
2.2. Projective Model
Parameterizing
Real projective space
is the set of lines through the origin in
. We can think about
as
, where
is associated with the line (point in
) intersecting
in
, and
is the horizontal line. There is a natural projection
by projecting a point to the line it is on. Under this projection,
maps to
.
Since
acts on
preserving the lines
, it gives a projective action on
fixing the points
. Now suppose we have any projective linear isomorphism of
fixing
. The isomorphism is represented by a matrix
with eigenvectors
. Since scaling
preserves its projective class, we may assume it has determinant 1. Its eigenvalues are thus
and
. The determinant equation, plus the fact that
Implies that
is of the form of a matrix in
. Therefore, the projective linear structure on
is the “same” (has the same isometry (isomorphism) group) as the hyperbolic (Riemannian) structure on
.
Metric
Clearly, we’re going to use the pushforward metric under the projection of
to
, but it turns out that this metric is a natural choice for other reasons, and it has a nice expression.
The map taking
to
is
. The hyperbolic distance between
and
in
is then
(by the fact from the previous sections that
is an isometry).
Recall the fact that
. Applying this, we get the nice form
We also recall the cross ratio, for which we fix notation as
. Then
Call the numerator of that fraction by
and the denominator by
. Then, recalling that
, we have
Therefore,
.
3. Hilbert Metric
Notice that the expression on the right above has nothing, a priori, to do with the hyperbolic projection. In fact, for any open convex body in
, we can define the Hilbert metric on
by setting
, where
and
are the intersections of the line through
and
with the boundary of
. How is it possible to take the cross ratio, since
are not numbers? The line containing all of them is projectively isomorphic to
, which we can parameterize as
. The cross ratio does not depend on the choice of parameterization, so it is well defined. Note that the Hilbert metric is not necessarily a Riemannian metric, but it does make any open convex set into a metric space.
Therefore, we see that any open convex body in
has a natural metric, and the hyperbolic metric in
agrees with this metric when
is thought of as a open convex set in
.
4. Higher-Dimensional Hyperbolic Space
4.1. Hyperboloid
The higher dimensional hyperbolic spaces are completely analogous to the 1-dimensional case. Consider
with the basis
and the 2-form
. This is the form defined by the matrix
. Define
to be the positive (positive in the
direction) sheet of the hyperbola
.
Let
be the linear transformations preserving the form, so
. This group is generated by
as symmetries of the
plane, together with
as symmetries of the span of the
(this subspace is euclidean). The group
is the set of orientation preserving elements of
which preserve the positive sheet of the hyperboloid (
). This group acts transitively on
with point stabilizers
: this is easiest to see by considering the point
. Here the stabilizer is clearly
, and because
acts transitively, any stabilizer is a conjugate of this.
As in the 1-dimensional case, the metric on
is
, which is invariant under
.
Geodesics in
can be understood by consdering the fixed point sets of isometries, which are always totally geodesic. Here, reflection in a vertical (containing
) plane restricts to an (orientation-reversing, but that’s ok) isometry of
, and the fixed point set is obviously the intersection of this plane with
. Now
is transitive on
, and it sends planes to planes in
, so we have a bijection
{Totally geodesic subspaces through
}
{linear subspaces of
through
}
By considering planes through
, we can see that these totally geodesic subspaces are isometric to lower dimensional hyperbolic spaces.
4.2. Projective
Analogously, we define the projective model as follows: consider the disk
. I.e. the points in the
plane inside the cone
. We can think of
as
, so this disk is
. There is, as before, the natural projection of
to
, and the pushforward of the hyperbolic metric agrees with the Hilbert metric on
as an open convex body in
.
Geodesics in the projective model are the intersections of planes in
with
; that is, they are geodesics in the euclidean space spanned by the
. One interesting consequence of this is that any theorem which is true in euclidean geometry which does not reply on facts about angles is still true for hyperbolic space. For example, Pappus’ hexagon theorem, the proof of which does not use angles, is true.
4.3. Projective Model in Dimension 2
In the case that
, we can understand the projective isomorphisms of
by looking at their actions on the boundary
. The set
is projectively isomorphic to
as an abstract manifold, but it should be noted that
is not a straight line in
, which would be the most natural way to find
‘s embedded in
.
In addition, any projective isomorphism of
can be extended to a real projective isomorphism of
. In other words, we can understand isometries of 2-dimensional hyperbolic space by looking at the action on the boundary. Since
is not a straight line, the extension is not trivial. We now show how to do this.
The automorphisms of
are
. We will consider
. For any Lie group
, there is an Adjoint action
defined by (the derivative of) conjugation. We can similarly define an adjoint action
by the Lie algebra on itself, as
for any path
with
. If the tangent vectors
and
are matrices, then
.
We can define the Killing form
on the Lie algebra by
. Note that
is a matrix, so this makes sense, and the Lie group acts on the tangent space (Lie algebra) preserving this form.
Now let’s look at
specifically. A basis for the tangent space (Lie algebra) is
,
, and
. We can check that
,
, and
. Using these relations plus the antisymmetry of the Lie bracket, we know
Therefore, the matrix for the Killing form in this basis is
This matrix has 2 positive eigenvalues and one negative eigenvalue, so its signature is
. Since
acts on
preserving this form, we have
, otherwise known at the group of isometries of the disk in projective space
, otherwise known as
.
Any element of
(which, recall, was acting on the boundary of projective hyperbolic space
) therefore extends to an element of
, the isometries of hyperbolic space, i.e. we can extend the action over the disk.
This means that we can classify isometries of 2-dimensional hyperbolic space by what they do to the boundary, which is determined generally by their eigevectors (
acts on
by projecting the action on
, so an eigenvector of a matrix corresponds to a fixed line in
, so a fixed point in
. For a matrix
, we have the following:
5. Complex Hyperbolic Space
We can do a construction analogous to real hyperbolic space over the complexes. Define a Hermitian form
on
with coordinates
by
. We will also refer to
as
. The (complex) matrix for this form is
, where
. Complex linear isomorphisms preserving this form are matrices
such that
. This is our definition for
, and we define
to be those elements of
with determinant of norm 1.
The set of points
such that
is not quite what we are looking for: first it is a
real dimensional manifold (not
as we would like for whatever our definition of “complex hyperbolic
space” is), but more importantly,
does not restrict to a positive definite form on the tangent spaces. Call the set of points
where
by
. Consider a point
in
and
in
. As with the real case, by the fact that
is in the tangent space,
Because
is hermitian, the expression on the right does not mean that
, but it does mean that
is purely imaginary. If
, then
, i.e.
is not positive definite on the tangent spaces.
However, we can get rid of this negative definite subspace.
as the complex numbers of unit length (or
, say) acts on
by multiplying coordinates, and this action preserves
: any phase goes away when we apply the absolute value. The quotient of
by this action is
. The isometry group of this space is still
, but now there are point stabilizers because of the action of
. We can think of
inside
as the diagonal matrices, so we can write
And the projectivized matrices
is the group of isometries of
, where the middle
is all vectors in
with
(which we think of as part of complex projective space). We can also approach this group by projectivizing, since that will get rid of the unwanted point stabilizers too: we have
.
5.1. Case
In the case
, we can actually picture
. We can’t picture the original
, but we are looking at the set of
such that
. Notice that
. After projectivizing, we may divide by
, so
. The set of points
which satisfy this is the interior of the unit circle, so this is what we think of for
. The group of complex projective isometries of the disk is
. The straight horizontal line is a geodesic, and the complex isometries send circles to circles, so the geodesics in
are circles perpendicular to the boundary of
in
.
Imagine the real projective model as a disk sitting at height one, and the geodesics are the intersections of planes with the disk. Complex hyperbolic space is the upper hemisphere of a sphere of radius one with equator the boundary of real hyperbolic space. To get the geodesics in complex hyperbolic space, intersect a plane with this upper hemisphere and stereographically project it flat. This gives the familiar Poincare disk model.
5.2. Real
‘s contained in
In a similar vein, there is a symplectic structure on
such that the real
are lagrangian subspaces (the flattest), and the
are symplectic, the most negatively curved.
An important thing to mention is that complex hyperbolic space does not have constant curvature(!).
6. Poincare Disk Model and Upper Half Space Model
The projective models that we have been dealing with have many nice properties, especially the fact that geodesics in hyperbolic space are straight lines in projective space. However, the angles are wrong. There are models in which the straight lines are “curved” i.e. curved in the euclidean metric, but the angles between them are accurate. Here we are interested in a group of isometries which preserves angles, so we are looking at a conformal model. Dimension 2 is special, because complex geometry is real conformal geometry, but nevertheless, there is a model of
in which the isometries of the space are conformal.
Consider the unit disk
in
dimensions. The conformal automorphisms are the maps taking (straight) diameters and arcs of circles perpendicular to the boundary to this same set. This model is abstractly isomorphic to the Klein model in projective space. Imagine the unit disk in a flat plane of height one with an upper hemisphere over it. The geodesics in the Klein model are the intersections of this flat plane with subspaces (so they are straight lines, for example, in dimension 2). Intersecting vertical planes with the upper hemisphere and stereographically projecting it flat give geodesics in the Poincare disk model. The fact that this model is the “same” (up to scaling the metric) as the example above of
is a (nice) coincidence.
The Klein model is the flat disk inside the sphere, and the Poincare disk model is the sphere. Geodesics in the Klein model are intersections of subspaces (the angled plane) with the flat plane at height 1. Geodesics in the Poincare model are intersections of vertical planes with the upper hemisphere. The two darkened geodesics, one in the Klein model and one in the Poincare, correspond under orthogonal projection. We get the usual Poincare disk model by stereographically projecting the upper hemisphere to the disk. The projection of the geodesic is shown as the curved line inside the disk
The Poincare disk model. A few geodesics are shown.
Now we have the Poincare disk model, where the geodesics are straight diameters and arcs of circles perpendicular to the boundary and the isometries are the conformal automorphisms of the unit disk. There is a conformal map from the disk to an open half space (we typically choose to conformally identify it with the upper half space). Conveniently, the hyperbolic metric on the upper half space
can be expressed at a point
(euclidean coordinates) as
. I.e. the hyperbolic metric is just a rescaling (at each point) of the euclidean metric.
One of the important things that we wanted in our models was the ability to realize isometries of the model with isometries of the ambient space. In the case of a one-parameter family of isometries of hyperbolic space, this is possible. Suppose that we have a set of elliptic isometries. Then in the disk model, we can move that point to the origin and realize the isometries by rotations. In the upper half space model, we can move the point to infinity, and realize them by translations.