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\begin{document}
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{center}
{\Large\bf K\"ahler manifolds and holonomy \\[15mm]
\small lecture 1}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\\[14mm]

{\small Misha Verbitsky } 
\\[20mm]

{\tiny\bf Tel-Aviv University
\\[2mm]  December 13, 2010, 
}
\end{center}

\newpage

{\bf \blue Complex action on vector spaces}


Let $V$ be a vector space over $\R$, and $I:\; V \arrow V$
an automorphism which satisfies $I^2 = - \Id_V$. {\bf \blue We extend the
action of $I$ on the tensor spaces 
$V\otimes V \otimes ... \otimes V \otimes 
V^*\otimes V^* \otimes ... \otimes V^*$ by multiplicativity:}
$I(v_1 \otimes ... \otimes w_1 \otimes ... \otimes w_n)=
I(v_1) \otimes ... \otimes I(w_1)\otimes ... \otimes I(w_n)$.


{\bf \green Trivial observations:}

1. {\bf \purple The eigenvalues of $I$ are $\pm \1$.}

2. {\bf \purple $V$ admits an $I$-invariant metric $g$.}
Take any metric $g_0$, and let $g:= g_0 + I(g_0)$.

3. {\bf \purple $I$ diagonalizable over $\C$.} Indeed,  any orthogonal matrix
is diagonalizable.

4. {\bf \purple All eigenvalues of $I$ are equal to $\pm \1$}.
Indeed, $I^2=-1$.

5. {\bf \purple There are as many $\1$-eigenvalues as there are
$-\1$-eigenvalues.} Indeed, $I$ is real.


\newpage

{\bf \blue The Hodge decomposition in linear algebra}

\definition
{\bf \blue The Hodge decomposition} 
$V\otimes_\R \C:= V^{1,0}\oplus V^{0,1}$ is defined in such a way that
$V^{1,0}$ is a $\1$-eigenspace of $I$, and $V^{0,1}$ a $-\1$-eigenspace.

\remark 
Let $V_\C:= V \otimes_\R \C$.
The Grassmann algebra of skew-symmetric forms
$\Lambda^n V_\C:=\Lambda^n_\R V \otimes _\R C$
admits a decomposition
\[ 
  \Lambda^n V_\C= \bigoplus_{p+q=n} \Lambda^p V^{1,0} 
  \otimes \Lambda^q V^{0,1}
\]
We denote $\Lambda^p V^{1,0} \otimes \Lambda^q V^{0,1}$ by $\Lambda^{p,q}V$.
The resulting decomposition $\Lambda^n V_\C= \bigoplus_{p+q=n}\Lambda^{p,q}V$
is called {\bf \blue the Hodge decomposition of the Grassmann algebra}.

\remark The operator $I$ induces $U(1)$-action on $V$ by the formula
$\rho(t)(v) = \cos t\cdot v + \sin t \cdot I(v)$. We extend this
action on the tensor spaces by muptiplicativity.

\newpage

{\bf \blue $U(1)$-representations and the weight decomposition }

\remark {\bf \red Any complex representation $W$ of $U(1)$ is written
as a sum of 1-dimensional representations $W_i(p)$}, with $U(1)$
acting on each $W_i(p)$ as $\rho(t)(v) = e^{\1 pt}(v)$. The 1-dimensional
representations are called {\bf \blue weight $p$ 
representations of $U(1)$.}

\definition 
A {\bf \blue weight decomposition} of a $U(1)$-representation
$W$ is a decomposition $W= \oplus W^p$, where each $W^p=\oplus_i W_i(p)$ is
a sum of  1-dimensional representations of weight $p$.

\remark {\bf \red The Hodge decomposition 
$\Lambda^n V_\C= \bigoplus_{p+q=n}\Lambda^{p,q}V$
is a weight decomposition}, with $\Lambda^{p,q}V$
being a weight $p-q$-component of $\Lambda^n V_\C$.

\remark $V^{p,p}$ is the space of $U(1)$-invariant 
vectors in $\Lambda^{2p}V$.

Further on, {\bf \blue $TM$ is the tangent bundle on a manifold,
and $\Lambda^iM$ the space of differential $i$-forms.}
It is a Grassman algebra on $TM$


\newpage

{\bf \blue Complex manifolds}

{\bf\green DEFINITION:} Let $M$ be a smooth manifold. 
An {\bf \blue almost complex structure} is an operator
$I:\; TM \arrow TM$ which satisfies $I^2 = - \Id_{TM}$.

{\bf \purple The eigenvalues of this operator are $\pm \1$.}
The corresponding eigenvalue 
decomposition is denoted $TM=T^{0,1}M\oplus T^{1,0}(M)$.


{\bf\green DEFINITION:}
An almost complex structure is {\bf \blue integrable}
if $\forall X,Y \in T^{1,0}M$, one has $[X,Y]\in T^{1,0}M$.
In this case $I$ is called {\bf \blue a complex structure operator}.
A manifold with an integrable almost complex structure
is called {\bf \blue a complex manifold}. 

{\bf\green THEOREM:} (Newlander-Nirenberg)\\
{\bf \red This definition is equivalent to the usual one.}

\remark The commutator defines a $\C^\infty M$-linear map\\
$N:=\Lambda^2(T^{1,0})\arrow T^{0,1}M$, called {\bf \blue 
the Nijenhuis tensor} of $I$. {\bf \purple One can represent $N$ as a section 
of $\Lambda^{2,0}(M) \otimes T^{0,1}M$.}

{\bf\green Exercise:} Prove that {\bf \blue $\C P^n$ is a complex
manifold,} in the sense of the above definition.


\newpage


{\bf \blue K\"ahler manifolds}

{\bf\green DEFINITION:} An Riemannian metric $g$ on
an almost complex manifiold $M$ is called 
{\bf \blue Hermitian} if $g(Ix, Iy)= g(x,y)$.
In this case, $g(x, Iy)= g(Ix, I^2y) = - g(y, Ix)$,
hence $\omega(x,y):= g(x, Iy)$ is skew-symmetric.

{\bf\green DEFINITION:} The differential 
form $\omega\in \Lambda^{1,1}(M)$ is called
{\bf \blue the Hermitian form} of $(M,I,g)$.

\remark It is $U(1)$-invariant, hence {\bf \purple of Hodge type (1,1)}.

{\bf\green DEFINITION:} A complex Hermitian manifold $(M,I,\omega)$
is called {\bf \blue K\"ahler} if $d\omega=0$. 
The cohomology class $[\omega]\in H^2(M)$ of a form $\omega$ 
is called {\bf \blue the K\"ahler class} of $M$, and
$\omega$ {\bf \blue the K\"ahler form}. 

\newpage

{\bf\blue Examples of K\"ahler manifolds.}

{\bf \green Definition:} Let $M=\C P^n$ be a complex projective
space, and $g$ a $U(n+1)$-invariant Riemannian form. It is called
{\bf \blue Fubini-Study form on $\C P^n$}. The Fubini-Study
form is obtained by taking arbitrary Riemannian form
and averaging with $U(n+1)$.

{\bf \green Remark:} For any $x\in \C P^n$, the stabilizer
$St(x)$ is isomorphic to $U(n)$. Fubini-Study form on
$T_x\C P^n= \C^n$ is $U(n)$-invariant, hence unique up to a constant.

{\bf \green Claim:} {\bf \red Fubini-Study form is K\"ahler.}
Indeed, $d\omega\restrict x$ is a $U(n)$-invariant 3-form
on $\C^n$, but such a form must vanish, because $-\Id\in U(n)$

\remark 
{\bf \purple The same argument works for all symmetric spaces.}

{\bf \green Corollary:} {\bf \red Every projective manifold 
(complex submanifold of $\C P^n$) is K\"ahler.}
Indeed, a restriction of a closed form is again closed.

\newpage

{\bf \blue Connections}

{\bf \green Notation:}
Let $M$ be a smooth manifold, $TM$ its tangent bundle,
$\Lambda^iM$ the bundle of differential $i$-forms,
$C^\infty M$ the smooth functions. {\bf \purple The space of sections 
of a bundle $B$ is denoted by $B$.}

\definition
A {\bf\blue connection} on a vector bundle $B$ is
a map $B \stackrel \nabla \arrow \Lambda^1 M \otimes B$ which
satisfies \[ \nabla(fb) = df \otimes b + f \nabla b\]
for all $b\in B$, $f\in C^\infty M$.

\remark A connection $\nabla$ on $B$ gives
a connection $B^* \stackrel {\nabla^*} \arrow \Lambda^1 M \otimes B^*$
on the dual bundle, by the formula
\[
d(\langle b, \beta\rangle) = \langle \nabla b, \beta\rangle+
\langle b, \nabla^*\beta\rangle
\]
These connections are usually denoted {\bf \red by the same letter $\nabla$.}

\remark
For any tensor bundle 
${\cal B}_1:=
B^*\otimes B^* \otimes ... \otimes B^* \otimes B\otimes B \otimes ... \otimes B$
{\bf \green a connection on $B$ defines a connection on ${\cal B}_1$}
using the Leibniz formula:
\[
\nabla(b_1 \otimes b_2) = \nabla(b_1) \otimes b_2 + b_1 \otimes \nabla(b_2).
\]

\newpage

{\bf \blue Torsion}

\definition
{\bf \blue A torsion} of a connection 
$\Lambda^1 \stackrel \nabla \arrow \Lambda^1 M \otimes \Lambda^1M$
is a map $\Alt \circ \nabla - d$,
where $\Alt:\;  \Lambda^1 M \otimes \Lambda^1M\arrow \Lambda^2 M$
is exterior multiplication. It is a map 
$T_\nabla:\; \Lambda^1M \arrow \Lambda^2 M$.

{\bf \green An exercise:} 
{\bf \red Prove that torsion is a $C^\infty M$-linear.}

\definition
Let $(M, g)$ be a Riemannian manifold. A connection $\nabla$ 
is called {\bf \blue orthogonal} if $\nabla(g) =0$.
It is called {\bf \blue Levi-Civita} if it is torsion-free.

\theorem (``the main theorem of differential geometry'')\\
{\bf \red For any Riemannian manifold, the
Levi-Civita connection exists,\\ and it is unique}.

\newpage

{\bf \blue Levi-Civita connection and K\"ahler geometry}

{\bf \green THEOREM:} Let $(M,I,g)$ be an almost complex Hermitian
manifold. {\bf \purple Then the following conditions are equivalent.}

(i) {\bf \red The complex structure $I$ is integrable, and 
the Hermitian form $\omega$ is closed.}

(ii) One has {\red $\nabla(I)=0$,} where $\nabla$ is the Levi-Civita connection.

\remark {\bf \purple The implication (ii) $\Rightarrow$ (i) is clear.}
Indeed, $[X,Y]=\nabla_X Y - \nabla_Y X$, hence it is
a $(1,0)$-vector field when $X, Y$ are of type (1,0), and 
then {\bf \blue $I$ is integrable}. Also, {\bf \blue $d\omega=0$, because
$\nabla$ is torsion-free,} and $d\omega= \Alt(\nabla\omega)$.

The implication (i) $\Rightarrow$ (ii) is proven by the same argument
as used to construct the Levi-Civita connection.

\newpage


{\bf \blue Holonomy group}

\definition (Cartan, 1923)
Let $(B,\nabla)$ be a vector bundle with connection over $M$.
For each loop $\gamma$ based in $x\in M$, let 
$V_{\gamma, \nabla}:\; B\restrict x \arrow B\restrict x$
be the corresponding parallel transport along the connection.
The {\bf \blue holonomy group} of $(B,\nabla)$
is a group generated by $V_{\gamma, \nabla}$,
for all loops $\gamma$. If one takes all contractible
loops instead, $V_{\gamma, \nabla}$ generates
{\bf \blue the local holonomy}, or {\bf \blue
the restricted holonomy} group.

\remark A bundle is {\bf \blue flat} (has vanishing curvature)
{\bf\purple if and only if its restricted holonomy vanishes.}

\remark If $\nabla(\phi)=0$ for some tensor 
$\phi\in B^{\otimes i}\otimes (B^*)^{\otimes j}$,
{\bf \red the holonomy group preserves $\phi$.}

\definition {\bf \blue Holonomy of a Riemannian manifold}
is holonomy of its Levi-Civita connection.

\example Holonomy of a Riemannian manifold lies in
$O(T_x M, g\restrict x)=O(n)$.

\example  Holonomy of a K\"ahler manifold lies in
$U(T_x M, g\restrict x, I \restrict x)=U(n)$.

\remark The holonomy group {\bf \red does not depend
on the choice of a point $x\in M$.}

\newpage

{\bf \blue Curvature of a connection}

Let $M$ be a   manifold, $B$ a bundle, $\Lambda^i M$ the
differential forms, and
$\nabla:\; B \arrow B \otimes \Lambda^1M$ 
a connection. We extend $\nabla$ to 
$B \otimes \Lambda^iM\stackrel\nabla \arrow B \otimes \Lambda^{i+1}M$ 
in a natural way, using the formula
\[
\nabla(b \otimes \eta) = \nabla(b)\wedge \eta + b \otimes d\eta,
\]
and define {\bf \blue the curvature $\Theta_\nabla$} of $\nabla$ as 
$\nabla\circ \nabla:\; B \arrow B\otimes \Lambda^2M$.

\claim {\bf \red This operator is $C^\infty M$-linear.}

\remark We shall consider $\Theta_\nabla$ as an element of 
$\Lambda^2M \otimes \End B$, that is, an $\End B$-valued 2-form.


\remark
Given vector fields $X, Y\in TM$, the curvature can be written
in terms of a connection as follows
\[
\Theta_\nabla(b)= \nabla_X\nabla_Yb - \nabla_Y\nabla_X B - \nabla_{[X,Y]}b.
\]

\claim Suppose that the structure group of $B$ is reduced
to its subgroup $G$, and let $\nabla$ be a connection
which preserves this reduction. This is the same as to say
that the connection form takes values in $\Lambda^1 \otimes \goth g(B)$.
{\bf \purple Then $\Theta_\nabla$ lies in $\Lambda^2M \otimes \goth g(B)$.}

\newpage



{\bf \blue The Lasso lemma}

\definition
A {\bf \blue lasso} is a loop of the following 
form:

{\begin{center}
\epsfig{file=Lasso.png,width=0.35\linewidth}
\end{center}}

The round part is called {\bf \blue a working part}
of a loop.

\remark {\bf \blue (``The Lasso Lemma'')} Let $\{U_i\}$ be a covering
of a manifold, and $\gamma$ a loop. Then {\bf \purple
any contractible loop  $\gamma$ is a product
of several lasso, with working part of each inside some $U_i$.}

\newpage


{\bf \blue The Ambrose-Singer theorem}

\definition
Let $(B, \nabla)$ be a bundle with connection,
$\Theta\in \Lambda^2(M)\otimes \End(B)$ its curvature,
and $a,b\in T_x M$ tangent vectors. An endomorphism
$\Theta(a,b)\in \End(B)\restrict x$ is called
{\bf \blue a curvature element}.

\theorem {\bf \blue (Ambrose-Singer)}
The restricted holonomy group of $B, \nabla$ at $z\in M$ 
is a Lie group, {\bf \red with its Lie algebra generated by all 
curvature elements $\Theta(a,b)\in \End(B)\restrict x$
transported to $z$ along all paths.}

\remark Its proof follows from the Lasso lemma.

\newpage

{\bf \blue Holonomy representation}

\definition
Let $(M,g)$ be a Riemannian manifold,
$G$ its holonomy group. A {\bf\blue holonomy representation} 
is the natural action of $G$ on $TM$.

\theorem (de Rham) 
Suppose that the holonomy representation is
not irreducible: $T_xM=V_1 \oplus V_2$.
Then $M$ locally splits as $M=M_1 \times M_2$,
with $V_1= TM_1$, $V_2=TM_2$.

{\bf\green Proof. Step 1:}
Using the parallel transform, we extend $V_1 \oplus V_2$
to a {\bf \purple splitting of vector bundles $TM = B_1 \oplus B_2$,
preserved by holonomy.}

{\bf\green Step 2:} The sub-bundles $B_1$, $B_2 \subset TM$
{\bf \purple are integrable:} $[B_1, B_1] \subset B_i$ 
(the Levi-Civita connection is torsion-free)

{\bf\green Step 3:} Taking the leaves of these
integrable distributions, {\bf \purple we obtain a local decomposition
$M=M_1 \times M_2$, with $V_1= TM_1$, $V_2=TM_2$. }


{\bf\green Step 4:} Since the splitting $TM = B_1 \oplus B_2$
is preserved by the connection, {\bf \purple the leaves $M_1, M_2$
are totally geodesic.} 

{\bf\green Step 5:} Therefore, {\bf \red locally $M$
splits (as a Riemannian manifold)}: \\
$M=M_1\times M_2$, where $M_1, M_2$ are any 
leaves of these foliations. \endproof


\newpage


{\bf \blue The de Rham splitting theorem}

\corollary 
Let $M$ be a Riemannian manifold, 
and $\Hol_0(M)\stackrel \rho \arrow \End(T_xM)$
a reduced holonomy representation. Suppose that $\rho$ is reducible:
$T_xM = V_1\oplus V_2 \oplus ...\oplus V_k$. {\bf \red Then $G=\Hol_0(M)$ also
splits: $G= G_1\times G_2 \times ...\times G_k$,}
with each $G_i$ acting trivially on all $V_j$ with $j\neq i$.

{\bf \green Proof:} Locally, this statement follows from
the local splitting of $M$ proven above. To obtain it globally
in $M$, use the Lasso Lemma. \endproof

\theorem (de Rham) A complete, simply connected  
Riemannian manifold with non-irreducible holonomy 
{\bf \red splits as a Riemannian product.}

\remark It is easy to find non-complete or non-simply
connected counterexamples to de Rham theorem.



\theorem (Simons, 1962)
Let $M$ be a manifold with irreducible holonomy.
{\bf \red Then either $M$ is locally symmetric, or $\Hol(M)$
acts transitively on the unit sphere in $T_xM$.}


\newpage

{\bf \blue Berger's theorem}

\theorem (Berger's theorem, 1955)
Let $G$ be an irreducible holonomy group of a
Riemannian manifold which is not locally symmetric. {\bf \red Then
$G$ belongs to the Berger's list:}

{
\begin{tabular}{|l|l|}
\hline
\multicolumn{2}{|c|}{\bf \color[rgb]{0,0,0.6}Berger's list}\\[1mm]
\hline
\it Holonomy  & \it Geometry\\[1mm]
\hline
$SO(n)$ acting on $\R^n$ & Riemannian manifolds\\[1mm]
\hline
$U(n)$ acting on $\R^{2n}$ & K\"ahler manifolds\\[1mm]
\hline
$SU(n)$ acting on $\R^{2n}$, $n>2$ & Calabi-Yau manifolds\\[1mm]
\hline
$Sp(n)$ acting on $\R^{4n}$ & hyperk\"ahler manifolds\\[1mm]
\hline
$Sp(n)\times Sp(1)/\{\pm 1\}$ & 
quaternionic-K\"ahler\\[1mm] acting on $\R^{4n}$, $n>1$ &  manifolds\\[1mm]
\hline
$G_2$ acting on $\R^7$ & $G_2$-manifolds \\[1mm]
\hline
$Spin(7)$ acting on $\R^8$ & $Spin(7)$-manifolds\\[1mm]
\hline
\end{tabular}
}


\remark There is one more group acting transitively on
a sphere: $Spin(9)$ acting on $S^{15}\subset \R^{16}$. In 1968, D. Alekseevsky
has shown  that {\bf \purple a manifold with holonomy $Spin(9)$ is automatically
locally symmetric.}

{\small \remark A similar list exists for non-orthogonal 
irreducible holonomy without torsion 
(Merkulov, Schwachh\"ofer, 1999).}



\end{document}

