5 The Mukai-Umemura manifold and its deformations [02AK]
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5 The Mukai-Umemura manifold and its deformations
The first part of this section gives an account, not aimed at algebraic geometry specialists, of a very interesting family of Fano -folds, following Mukai. The basic references are [22], [23], but there are also many other relevant papers in the algebraic geometry literature. Then we go on to discuss the existence of Kahler-Einstein metrics on some manifolds in this family.
5.1 Mukai’s construction
We start with a -dimensional complex vector space and write for the Grassmann manifold of 3-dimensional subspaces of . So has dimension . A form defines a subset consisting of the -planes such that vanishes. In other language we consider the tautological rank 3 vector bundle ; the form defines a section of with zero set . For generic this zero set is a smooth subvariety of codimension . Now let be three such forms and consider
Of course this only depends on the -plane in spanned by the , so we may sometimes write . Obviously there is a Zariski-open subset in the Grassmannian of -planes such that is a smooth subvariety of dimension . This set is non-empty, as we will see later. The group acts on the whole construction and obviously different subspaces which lie in the same orbit define isomorphic manifolds , so we get a set of equivalence classes of manifolds constructed in this way, parametrised by the quotient . (Mukai shows further that this parametrisation is effective: i.e. is isomorphic to if and only if lie in the same orbit. Moreover, he shows that all “prime Fano -folds of genus 12” arise in this way.)
We compute the canonical bundle of the variety for some . We have
where is the ample line bundle . So, writing for the the top exterior power of a vector bundle, we have
The tangent bundle of the Grassmannian at a -plane can be identified with . So
Now since the tangent bundle of is the kernel of a surjective map from to we have
Thus is a Fano manifold. The sections of over give the Plucker embedding
For any -form we get a hyperplane section which just consists of the -planes such . By definition this occurs if is in and is in the image of the wedge product map . We expect this map to have an image of dimension in which case the image of the composite
lies in a linear subspace . Certainly this map is defined by sections of , we will see later that has dimension and that this embedding is that given by the anticanonical system.
To make this more concrete we show now that is a rational variety; that is, we construct an explicit parametrisation of a dense open set in . Suppose we have a pair of -dimensional subspaces with . We ask what -planes in the -dimensional subspace lie in . In matrix notation, we can write the restriction of a form to as
Now consider the -dimensional subspaces which arise as the graphs of linear maps . The condition becomes
| (33) |
So our three forms give us three triples and we have three equations of the form (33) to solve to find a point of . We have unknowns: the entries of the matrix . The left hand side of (33) takes values in the -dimensional space of skew symmetric matrices so we obtain a total of equations in these unknowns and we expect a finite number of solutions. These equations are quadratic and one can solve them explicitly, to see that there are generically two solutions. However it is easier to suppose that we are in the case when itself lies in . This means that all the are zero, so the equations (33) become linear. Generically this system of linear equations in unknowns is nondegerate and there is a unique solution. Now suppose we have found one point in and consider the space of -planes in which contain . This is a copy of projective -space . Given a point in , that is to say a 6 dimensional subspace of , we choose a complementary subspace to write is as . Then we can proceed as above and, by solving linear equations, find the points of . Generically there is just one, say, different from the original . Conversely for any the sum lies in a -dimensional subspace. Of course there will be various exceptional cases, but the upshot is that we get a birational map from to which takes a subspace containing to .
We now consider a special manifold in this family. Take the vector space to be the sixth symmetric power of the fundamental representation of . Then decomposes into distinct irreducible representations
The summand is a -plane invariant under , so there is a natural action on the corresponding variety, the Mukai-Umemura manifold, . We will see below that admits a Kahler-Einstein metric. The representation has a standard invariant symmetric form and the inclusion is just the map from the Lie algebra of given by the action on . This comes down to saying that a -plane is in if and only if
| (34) |
for all and . Notice that the action of on all the spaces involved actually factors through .
Identify the projectivisation of the fundamental representation with the standard round sphere and fix an icosahedron, which can be regarded as a set of 12 vertices in in this sphere. Thus we get a symmetry group of order . There is a simple way to see that the -dimensional representation of becomes reducible when restricted to . There are pairs of antipodal vertices and for each such pair we have a -dimensional subspace consisting of polynomials which vanish to order at . The sum of these subspaces is obviously invariant under and is a proper subspace of since it has codimension at least . A little calculation shows that this invariant subspace is of dimension and satisfies the criterion (34). So this subspace gives a point in fixed by . On the other hand the stabiliser of is obviously not the whole of and, since there is no finite subgroup of strictly larger than , the stabiliser must be exactly .
Now go back to the wedge product . In terms of representations this is an -map
It is an exercise in representation theory to show that
So comparing with
we see that the embedding gives rise to an -equivariant embedding
| (35) |
In other words, by our identification of the anticanonical bundle we have
as a representation of .In particular, there is an -invariant section of . Explicitly, if we identify with then corresponds to the -form on defined as follows. We choose any orthonormal basis of and write down the -form
In this way, we get another description of the manifold . Our point cannot lie in the zero set of (since its orbit is -dimensional). So, in the embedding (35), we have
Thus is an element of whose stabiliser in is exactly .Now there is an obvious element of the projective space with stabiliser , just the configuration of vertices of the icosahedron, regarded as an element of the symmetric product. Since is a perfect group it must act trivially on the corresponding line in , so we get a vector in with stabiliser . It is easy to see that, up to a multiple, this in the only element of with stabiliser , and thus we have identified . Then we can simply define to be the closure in of the -orbit of in . (Here we are regarding the vector space as being a subset of the projective space in the familiar way.)
In this description, the intersection of with the hyperplane at infinity
is, by definition, the zero set of the invariant section of . Consider a -parameter subgroup in . Thus we have a pair of distinct point such that when is large positive the map contracts most of the sphere to a small neighbourhood of , and when is large negative to a small neighbourhood of . If is any configuration of distinct points it is not hard to see that the limit as of
in the symmetric product is either (in the generic case) or (in the case when one of the is ). Using this, Mukai and Umemura show that the divisor at infinity consists precisely of the union of points of the form or in . It is easy to identify this geometrically. The points of the form make up the rational normal curve in . Our divisor is the surface swept out by the lines in tangent to the rational normal curve. As a set we can identify with : we just map to . But the surface is singular and a more precise statement is that the map above is a holomorphic map which is the normalisation of . The singular set of is the image of the diagonal in , and it is easy to check that the singularity has the form of a cusp transverse to the diagonal. That is to say, we can choose local co-ordinates in around a singular point of such that is defined by the equation .
We now have a rather explicit description of , as the compactification of formed by adjoining the divisor . We can use this to compute the action of on all of the spaces of sections . For the pull back is isomorphic to the line bundle over . We can regard the structure sheaf of as a subsheaf of that of . From the local model of the singularity along the diagonal one sees that the quotient can be identified with sections of along the diagonal. This means that is the kernel of a map . As representations of this is a map
Now
and the map above is just the projection to the second factor. So
Then the exact cohomology sequence of
together with Kodaira vanishing on gives
and inductively we get a description of each . Thus
For we get multiplicities: contains two copies of . This illustrates the difference with the multiplicity-free case discussed above. (Although since the multiplicities are small until becomes quite large, once is tempted to think of as being “close” to multiplicity-free. )
5.2 Topological and symplectic picture
We will now get another explicit picture of , taking the point of view of symplectic geometry. Recall that all Kahler metrics in the cohomology class define equivalent symplectic structures, so we have a well-defined symplectic manifold with an -action. Thus we have an equivariant moment map
whose image is clearly a ball in . We can understand the structure of this moment map by restricting to a subgroup , say that corresponding to the -axis in . Then the Hamiltonian for this circle action on is the composite of with projection to the -axis. The critical points of are the fixed points of the circle action and we can find these explicitly. We can suppose that our circle subgroups corresponds to the standard action of
acting on with weights . We write for the basis vector belonging to the weight . This induces an action on the Grassmannian whose fixed points are just invariant -dimensional subspaces of and these are just the spans for distinct . By checking the 35 different cases, or otherwise, one finds that the only which satisfy the criterion (34) to lie in are . There is an action of the Weyl group on the whole situation which commutes, up to sign, with the circle action, takes to and takes to . So there are four fixed points of the circle action but to analyse the local structure around them it suffices to consider the two cases . Notice that, by considering as a Morse function we immediately see that has the same additive homology as . Notice also that the value of at a critical point is just given by the weight of the action on the fibre of over this point, which is just at .
We next compute the weights of the circle action on the tangent spaces at the fixed points. This is similar to the calculation of the canonical bundle. At a fixed point the tangent space , viewed as a representation of , can be written as the formal difference
Computing the weights of these two terms and subtracting we find that the weights of the action on the tangent space at are and on the tangent space at are . In either case the orbit of the fixed point is a copy of in and the weight in the action on just corresponds to the tangent space of this orbit. The weights normal to the orbit are in the case of and in the case of .
With these calculations we can get a good picture of the map . Write for the orbits of and respectively. Then restricts to an -equivariant equivalence between and the sphere of radius in and between and the sphere of radius . The image of is the ball of radius and the critical values of are precisely these two spheres. So is a fibration away from these spheres. For , write for the preimage . If the fibre is a -manifold. If also then this -manifold has a natural circle action defined by the circle subgroup of fixing . When the fibre has an action. As varies in the fibre only “changes”—in the obvious sense—when crosses the special values . Thus we understand the full topological picture if we understand the changes in the fibre as moves along the positive -axis, say. Let be the pre-image by of the positive -axis. This is a smooth -manifold, with a circle action, and the fibres , for on the axis, are the level sets of the Hamiltonian , restricted to . Then we have the usual Morse-theory description of these changes, from the Hessian of on , which is determined by the weights of the circle action. As moves across the point the situation is modelled by the level sets
for , with the circle action of weight . Thus the fibre changes from the empty set to a -sphere with an action given by these weights. As moves across the point the situation is modelled, locally, by the level sets
with the circle action of weight . The effect on the fibres is to perform a “Dehn surgery” on an -orbit. Thus the fibres for are obtained by performing this surgery on a knot . Now is a free orbit of the action so it is the “torus knot” which is just a trefoil. To nail down the Dehn surgery completely we need to specify a framing of the knot but this is determined by the fact that the linking number of a nearby orbit with is the weight , from which one concludes that the framing is . This is a well-known description of the Poincaré homology sphere (the result of -surgery on a trefoil), and ties in with our previous discussion since the fibre is the -orbit . (Another way of expressing this is that the fibres are Seifert-fibred -manifolds: for we have two multiple fibres with multiplicity and the surgery across introduces another multiple fibre with multiplicity , so for we get the Seifert manifold with multiplicities , which is another well-known description of the Poincaré manifold.)
It is interesting to match this picture up with the algebro-geometric description. This illustrates the general theory of Kirwan [19]. The -sphere at which attains its maximal value is a holomorphic sphere in : it is just the rational normal curve in our divisor . The other sphere is not holomorphic. It is a critical manifold for the function on and the divisor appears as the associated “ascending set”: the closure of the set of points which flow to under the decreasing gradient flow of . In our description of as the holomorphic curve is the diagonal and is the “anti-diagonal”consisting of pairs of antipodal points. One can also see the cusp singularity in , transverse to , from the weights of the circle action on the normal bundle.
Notice that if we write , for the -dimensional representation of , the moment map for the action gives a description of very similar to that above. In this case is where is the group of symmetries of an equilateral triangle, and we see this -manifold described as the Seifert fibration with multiple fibres .
5.3 Deformations
Here we study the deformations of Mukai’s construction about the special solution . Recall that a manifold in this family is specified by a -plane in . We start with the -plane . The tangent space of the Grassmannian at this point is given by the linear maps from to the complementary subspace , that is (using the fact that all these representations are isomorphic to their duals)
The action of the group gives a linear map
which we know has kernel the Lie algebra of the stabiliser. Now the Lie algebra of is
so the Lie algebra of is . It is clear then that the quotient of the tangent space by the tangent space to the orbit is just , as a representation of . By general theory there is an equivariant slice: a equivariant embedding from a neighbourhood of in into , mapping to our fixed subspace , such that two points in the same orbit if and only are in the same orbit. In fact, although we do not really need this, what we are describing is the versal deformation of , so , as a representation of .
One can gain a lot of insight from this simple calculation. The structure of the orbits of on (or any ) is a standard example in Geometric Invariant Theory. There are five cases
- 1.
The trivial orbit .
- 2.
The orbits of polynomials having no zero of multiplicity . These are closed in .
- 3.
The orbit of polynomials having two distinct zeros, each of multiplicity four. This orbit is closed and each point in it has stabiliser .
- 4.
The orbits of polynomials having a zero of multiplicity four and other zeros each of multiplicity less than four. These orbits are not closed but there closure contains the orbit of type (3).
- 5.
The orbits of polynomials having a zero of multiplicity . these are not closed and contain in their closure.
This is the source of the famous example of Tian of Fano manifolds without Kahler-Einstein (or Ricci soliton) metrics [31]. Tian shows that the manifolds corresponding to any orbit of type (5) cannot have such metrics. Tian’s general results also show the same for the manifolds corresponding to orbits of type (4). Tian’s results are of course deep and difficult but we note now that a weaker statement is rather obviously true. For this we need to recall some background.
In general, the linearisation of the Kahler-Einstein equations on a complex manifold at a solution is given by the self-adjoint operator and, much as we have seen in Section 3, the kernel of this can be identified with the Lie algebra of the isometry group of . Suppose we have a -equivariant deformation of : i.e. a complex manifold with a -action, an action of on a ball and a -equivariant submersion . In this situation we automatically get “local actions” of the complexified group on and , compatible with . The standard “Kuranishi method”, which depends only on the formal properties of the situation, yields the following structure (after possibly restricting to a smaller ball ).
- •
A -invariant family of Kahler metrics on the fibres such that is isometric to if and only if and are in the same -orbit.
- •
A smooth map , equivariant for the action of on and the co-adjoint action on , such that is Kahler-Einstein if and only if .
Now in this general situation we can see that, if the -action on is non-trivial the map cannot be identically zero. For if are in the same orbit of the local action on then and are isomorphic complex manifolds. But if and both vanish then and are Kahler-Einstein and, by the uniqueness of the Kahler-Einstein solution, they must be isometric and this only happens if are in the same -orbit. Thus what we see from this elementary argument is that as we deform in the smooth family we cannot deform the metric in a smooth family of Kahler-Einstein metrics, for all small . Tian’s much stronger result is that if the Futaki invariant of vanishes (say), and if lies in the closure of the the -orbit of a point then does not admit any Kahler-Einstein metric at all. This is an example of the “jumping of structures” phenomenon discussed in Section 1: there are arbitrarily small deformations of which are equivalent to a different structure .
Returning to our special case of the Mukai-Umemura manifold, we can see conversely that there are some deformations of which do admit Kahler-Einstein metrics. The general theory of these “obstruction maps” is being developed by T. Brönnle, in his Ph.D thesis, but in this special case we can make some simple deductions from symmetry arguments. Let be a point in which is fixed by a subgroup . Then acts on and if is any equivariant map from to then must fix . So if the origin is the only point in fixed by then we must have . Consider, for example,
with any . This is fixed by a dihedral group of order which has the desired property, so we see that the deformations corresponding such elements of admit Kahler-Einstein metrics, for small . For the element has a discrete stabiliser in and it follows that the corresponding metrics have discrete isometry groups. But then the deformation theory implies that all small deformations of these manifolds admit Kahler-Einstein metrics. So we conclude that there is a non-empty open set in where the manifolds admit Kahler-Einstein metrics.
Taking above we get a special family of deformations, admitting Kahler-Einstein metrics, where we can take . It follows that the corresponding manifolds have a -action. We can see this family of manifolds explicitly as follows. Fix the action on with weights as usual. Then we want to look at -dimensional subspaces of preserved by the action and we just consider those on which the action has weights . Now the weight -subspace of has a basis and our space must contain a vector
for scalars etc. Similarly must contain a vector
and a vector
The vector space is determined by these three vectors . The coefficients are not unique. We could change to . Also we could change our basis vectors to to give an equivalent -plane. This would change the coefficients, for example would change to . However the expression
is invariant under all these changes and gives a “modulus” for this family. The Mukai-Umemura manifold has . When is close to we have seen that the corresponding manifold admits a Kahler-Einstein metric. It seems likely that this true for all but, as far the author is aware, this is not known. It seems an interesting test case for future developments in the existence theory.
5.4 The -invariant
In this subsection we establish the fact used above, that the Mukai-Umemura manifold has a Kahler-Einstein metric11 1 This material appeared in the preprint A note on the -invariant of the Mukai-Umemura 3-fold arxiv DG 07114357., which is . For this we appeal to the theory of the -invariant, developed by Tian [30]. We begin by recalling the definition. Let be a Fano manifold on which a compact group acts by holomorphic automorphisms and fix a -invariant Kahler metric in the cohomology class . Let be the set of -invariant Kahler potentials on such that and . Thus can be identified with the set of all -invariant Kahler metrics in the given Kahler class. Let be the set defined by the condition that if there exists a such that
for all . Here is the volume form defined by the fixed metric . Then Tian sets
and shows that this does not depend on the choice of . He shows that is always strictly positive and that if then has a Kahler-Einstein metric. What we really show in this subsection is that if we take the Mukai-Umemura manifold with the action of then,
Theorem 3
The -invariant is .
So, since , Tian’s theory proves the existence of a Kahler-Einstein metric. We should say straightaway that this is not really a new result. Alessio Corti has explained to the author that, given the facts above, it can be obtained from the more general theories of [13]. But our argument is extremely simple and fits well into the general framework of this article.
We will only write down the proof that , which is what is relevant to Corollary 1. The proof that is an easy extension of this.
Lemma 2
There is an such that
for all .
This is a step in Tian’s proof that and we repeat his argument. If we have
Let be the Green’s function for , so that for all functions on
where is the volume of the manifold. With our sign conventions, is bounded below and, since we can change by the addition of a constant without affecting the identity, we may suppose that . While is singular along the diagonal it is integrable in each variable. Let be the point where vanishes. Then applying the Green’s identity to we have
So we can take
For the rest of this section we work with the Mukai-Umemura manifold, which we denote by . Let be the -invariant section of the anticanonical bundle cutting out the divisor . There is a Hermitian metric on this line bundle such that the curvature of the associated unitary connection is . Set
This is a smooth function on and .
Lemma 3
For any the function is integrable.
This is also standard. The integral in question is
By what we know about the singlarities of , we can reduce to considering the integrals
where is the unit ball in and are complex co-ordinates. Let be the linear map and for set
Set
The substitution shows that
Thus is finite if and the union of the cover .
Now we give the main proof. Let be the point with stabiliser . We identify -invariant functions on with -invariant functions on as in (4.2). The function on corresponds to a convex function on which is an “admissible potential” in the language of (4.2). For any other admissible potential the difference corresponds to , restricted to . The normalisation that becomes the condition that , and in particular .
Let be the identity coset. It is the unique point fixed by the action of . Any admissible potential function on is proper and bounded below so achieves a minimum in . By the convexity and -invariance this minimum must occur at . Set . Then the inequality translates back into the statement that . So
By Lemma 1, it suffices to obtain an upper bound on . Let be the geodesic ball in centred on , of radius say, and let be the maximum value of on , so for any we have on . Convexity along geodesics emanating from implies that
for any point in . In particular, on the ball of radius about we have .
Take the inverse image in of the ball and map this to by . The image obviously contains a neighbourhood of and on we have . Then Lemma 1 implies that cannot be very large. In fact, if the minimum of on is , we have on , so
hence
where is as in Lemma 1. This completes the proof of Theorem 3.
Notice that the same argument can be applied in the toric case, when the polytope has a group of symmetries, as discussed in (4.2). We should suppose that has a unique fixed point in : then the proof proceeds exactly as before. The analogue of Lemma 1 holds with since the local models for the zeros of are where and is locally integrable for . the conclusion is that the -invariant in this case is . which is a theorem of Batyrev and Selinova [4]. Song gave another proof in [26], and showed conversely that for polytopes which do not have such a symmetry group the -invariant never exceeds . The fact that such toric manifolds nevertheless have Kahler-Einstein metrics illustrates the point that Tian’s -invariant criterion is sufficient but not necessary.