1 Introduction

A generalised complex structure on a real manifold X of dimension 2n, as defined by Hitchin [9], is a rank-2n isotropic subbundle \(E^{0,1}\subset (T_X\oplus T^*_X)^{{\mathbb {C}}}\) such that

  1. 1.

    \(E^{0,1}\oplus \overline{ E^{0,1} }= (T_X\oplus T^*_X)^{{\mathbb {C}}}\)

  2. 2.

    \(C^{\infty }(E^{0,1})\) is closed under the Courant bracket.

On a manifold with a generalized complex structure M. Gualtieri in [6] defined the notion of a generalized holomorphic bundle. More precisely, a generalized holomorphic bundle on a generalized complex manifold, is a vector bundle \({{\mathcal {E}}}\) with a differential operator \(\overline{D} : C^\infty ({{\mathcal {E}}}) \longrightarrow C^{\infty }({{\mathcal {E}}}\otimes E^{0,1})\) such that for all smooth function f and all section \(s\in C^\infty ({{\mathcal {E}}}) \) the following holds

  1. 1.

    \(\overline{D} (fs)=\overline{\partial }(fs)+f \overline{D}(s)\)

  2. 2.

    \(\overline{D}^2=0\).

In the case of an ordinary complex structure and \(\overline{D} = \overline{\partial }+\phi \), for operators

$$\begin{aligned} \overline{\partial } : C^\infty ({{\mathcal {E}}}) \longrightarrow C^{\infty }({{\mathcal {E}}}\otimes \overline{T^*_X}) \end{aligned}$$

and

$$\begin{aligned} \phi : C^\infty ({{\mathcal {E}}}) \longrightarrow C^{\infty }({{\mathcal {E}}}\otimes T_X), \end{aligned}$$

the vanishing \(\overline{D}^2=0\) means that \( \overline{\partial }^2=0\) , \( \overline{\partial } \phi =0\) and \(\phi \wedge \phi =0\). By a classical result of Malgrange the condition \( \overline{\partial }^2=0\) implies that \({{\mathcal {E}}}\) is a holomorphic vector bundle. On the other hand, \( \overline{\partial } \phi =0\) implies that \(\phi \) is a holomorphic global section

$$\begin{aligned} \phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X) \end{aligned}$$

which satisfies an integrability condition \(\phi \wedge \phi =0\). A co-Higgs sheaf on a complex manifold X is a sheaf \({{\mathcal {E}}}\) together with a section \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\)(called a Higgs fields) for which \(\phi \wedge \phi =0\). General properties of co-Higgs bundles were studied in [8, 15]. There is a motivation in physics for studying co-Higgs bundles, see [7, 10] and [19].

There are no stable co-Higgs bundles with nonzero Higgs field on curves C of genus \(g>1\). (When \(g = 1\), a co-Higgs bundle is the same thing as a Higgs bundle in the usual sense.) In fact, contracting with a holomorphic differential gives a non-trivial endomorphism of \({{\mathcal {E}}}\) commuting with \(\phi \) which is impossible in the stable case [8, 16]. S. Rayan showed in [14] the non-existence of stable co-Higgs bundles with non trivial Higgs field on K3 and general-type surfaces. In this note we prove the following result.

Theorem 1.1

Let \(({{\mathcal {E}}}, \phi )\) be a rank two co-Higgs vector bundles on a Kähler compact surface X with \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\) nilpotent. If \(({{\mathcal {E}}}, \phi )\) is semi-stable, then one of the following holds up to finite étale cover:

  1. 1.

    X is uniruled.

  2. 2.

    X is a torus and \(({{\mathcal {E}}}, \phi )\) is strictly semi-stable.

  3. 3.

    X is a properly elliptic surface and \(({{\mathcal {E}}}, \phi )\) is strictly semi-stable.

It follows direct of proof of Theorem 1.1 that the we can consider a more general classes of singular projective surfaces.

Theorem 1.2

Let \(({{\mathcal {E}}}, \phi )\) be a rank two co-Higgs torsion-free sheaf on a normal projective surface X with \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\) nilpotent. If \(({{\mathcal {E}}}, \phi )\) is stable, then X is uniruled.

Finally, in this work we consider a relation between co-Higgs bundles and Poisson geometry on \({\mathbb {P}}^1\)-bundles. In [18] Polishchuk associated to each rank-2 co-Higgs bundle \(({{\mathcal {E}}}, \phi )\) a Poisson structure on its projectivized bundle \({\mathbb {P}}({{\mathcal {E}}})\). This relation was explained by Rayan in [15] as follows:

let \(Y:= {\mathbb {P}}({{\mathcal {E}}})\) and consider the natural projection \(\pi :Y \rightarrow X\). The exact sequence

$$\begin{aligned} 0\longrightarrow T_{X|Y}\longrightarrow T_Y\longrightarrow \pi ^*T_X\longrightarrow 0 \end{aligned}$$

implies that \(T_{X|Y}\otimes \pi ^*T_X \subset \bigwedge ^2 T_Y\). Since \(T_{X|Y}={\mathrm {Aut}}({\mathbb {P}}({{\mathcal {E}}}))={\mathrm {Aut}}({{\mathcal {E}}})/{\mathbb {C}}^*\) we get that

$$\begin{aligned} \pi _*(T_{X|Y}\otimes \pi ^*T_X)=\pi _*T_{X|Y}\otimes T_X=End_0({{\mathcal {E}}})\otimes T_X, \end{aligned}$$

where \(End_0({{\mathcal {E}}})\) denotes the trace-free endomorphisms of \({{\mathcal {E}}}\). Therefore, we can associate a trace-free co-Higgs fields \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\) a bi-vector \(\pi ^*\phi \in H^0(X,T_{X|Y}\otimes \pi ^*T_X) \subset H^0(X, \bigwedge ^2 T_Y)\) on \({\mathbb {P}}({{\mathcal {E}}})\). The co-Higgs condition \(\phi \wedge \phi =0\) implies that bi-vector \(\pi ^*\phi \) is integrable, see the introduction of [15]. The codimension one foliation on \( {\mathbb {P}}({{\mathcal {E}}})\) is the called foliation by symplectic leaves induced by Poisson struture.

We get an interisting consequence of the proof Theorem 1.2.

Corollary 1.1

If \(({{\mathcal {E}}}, \phi )\) is locally free, stable and nilpotent , then the closure of the all leaves of the foliation by symplectic leaves on \({\mathbb {P}}({{\mathcal {E}}})\) are rational surfaces.

2 Semi-stable co-Higgs sheaves

Definition 2.1

A co-Higgs sheaf on a complex manifold X is a sheaf \({{\mathcal {E}}}\) together with a section \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\)(called a Higgs fields) for which \(\phi \wedge \phi =0\).

Denote by \(End_0({{\mathcal {E}}}) := ker(tr : End({{\mathcal {E}}}) \longrightarrow {\mathcal {O}}_X)\) the trace-free part of the endomorphism bundle of \({{\mathcal {E}}}\). Since

$$\begin{aligned} End({{\mathcal {E}}})= End_0({{\mathcal {E}}})\oplus {\mathcal {O}}_X \end{aligned}$$

we have that \(End({{\mathcal {E}}})\otimes T_X=(End_0({{\mathcal {E}}})\otimes T_X)\oplus T_X\). Thus, the Higgs field \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\) can be decomposed as \(\phi =\phi _1+\phi _2\), where \(\phi _1\) is the trace-free part and \(\phi _2\) is a global vector field on X. In particular, if the surface X has no global holomorphic vector fields, then every Higgs field is trace-free.

Definition 2.2

Let \((X,\omega )\) be a polarized Kähler compact manifold. We say that \(({{\mathcal {E}}},\phi )\) is semi-stable if

$$\begin{aligned} \frac{c_1(\mathcal {F})\cdot [\omega ]}{rank(\mathcal {F})}\le \frac{c_1({{\mathcal {E}}})\cdot [\omega ]}{rank({{\mathcal {E}}})} \end{aligned}$$

for all coherent subsheaves \(0\ne \mathcal {F}\subsetneq {{\mathcal {E}}}\) satisfying \(\Phi (\mathcal {F})\subseteq \mathcal {F}\otimes T_X\), and stable if the inequality is strict for all such \(\mathcal {F}\). We say that \(({{\mathcal {E}}},\phi )\) is strictly semi-stable if \(({{\mathcal {E}}},\phi )\) is semi-stable but non-stable.

3 Holomorphic foliations

Definition 3.1

Let X be a connected complex manifold. A one-dimensional holomorphic foliation is given by the following data:

  1. 1.

    an open covering \({\mathcal {U}}=\{U_{\alpha }\}\) of X;

  2. 2.

    for each \(U_{\alpha }\) an holomorphic vector field \(\zeta _\alpha \) ;

  3. 3.

    for every non-empty intersection, \(U_{\alpha }\cap U_{\beta } \ne \emptyset \), a holomorphic function

    $$\begin{aligned} f_{\alpha \beta } \in {\mathcal {O}}_X^*(U_\alpha \cap U_\beta ); \end{aligned}$$

such that \(\zeta _\alpha = f_{\alpha \beta }\zeta _\beta \) in \(U_\alpha \cap U_\beta \) and \(f_{\alpha \beta }f_{\beta \gamma } = f_{\alpha \gamma }\) in \(U_\alpha \cap U_\beta \cap U_\gamma \).

We denote by \(K_{\mathcal {F}}\) the line bundle defined by the cocycle \(\{f_{\alpha \beta }\}\in {\mathrm {H}}^1(X, {\mathcal {O}}^*)\). Thus, a one-dimensional holomorphic foliation \(\mathcal {F}\) on X induces a global holomorphic section \(\zeta _{\mathcal {F}}\in {\mathrm {H}}^0(X,T_X\otimes K_{\mathcal {F}})\). The line bundle \(K_{\mathcal {F}}\) is called the canonical bundle of \(\mathcal {F}\). Two sections \(\zeta _{\mathcal {F}}\) and \(\eta _{\mathcal {F}}\) of \( {\mathrm {H}}^0(X,T_X\otimes K_{\mathcal {F}})\) are equivalent, if there exists a never vanishing holomorphic function \(\varphi \in {\mathrm {H}}^0(X,{\mathcal {O}}^*) \), such that \(\zeta _{\mathcal {F}}= \varphi \cdot \eta _{\mathcal {F}}\). It is clear that \(\zeta _{\mathcal {F}}\) and \(\eta _{\mathcal {F}}\) define the same foliation. Thus, a holomorphic foliation \(\mathcal {F}\) on X is an equivalence of sections of \(H^0(X, T_X\otimes K_{\mathcal {F}})\).

4 Examples

4.1 Canonical example of split co-Higgs bundles

Here we will give an example which naturally generalizes the canonical example given by Rayan on [15, Chapter 6]. Let \((X, \omega )\) be a polarized Kähler compact manifold. Suppose that there exists a global section \(\zeta \in H^0(X , Hom(N,TX\otimes L))\simeq H^0(X ,TX\otimes L \otimes N^*)\). Now, consider the vector bundle

$$\begin{aligned} {{\mathcal {E}}}=L \oplus N. \end{aligned}$$

Define the following co-Higgs fields

$$\begin{aligned} \phi : L \oplus N \longrightarrow (T_X \otimes L)\oplus (T_X \otimes N)\in H^0(X,End({{\mathcal {E}}})\otimes T_X) \end{aligned}$$

by \(\phi (s,t)=(\zeta (t),0)\). Since \(\phi \circ \phi =0 \in H^0 (End({{\mathcal {E}}})\otimes T_X\otimes T_X) \) we get that \(\phi \wedge \phi =0\). Moreover, observe that the kernel of \(\phi \) is the \(\phi \)-invariant line bundle L. On the other hand, the line bundle L is destabilising only when

$$\begin{aligned}{}[2c_1(L)- c_1({{\mathcal {E}}})]\cdot [\omega ]=[c_1(L)-c_1(N)]\cdot [\omega ]> 0. \end{aligned}$$

That is, if

$$\begin{aligned}{}[c_1(L)]\cdot [\omega ]> [c_1(N)]\cdot [\omega ]. \end{aligned}$$

4.2 Co-Higgs bundles on ruled surfaces

Let C be a curve of genus \( g >1\). Now, consider the ruled surface \(X:={\mathbb {P}}(K_C\oplus {\mathcal {O}}_C)\) and

$$\begin{aligned} \pi :{\mathbb {P}}(K_C\oplus {\mathcal {O}}_C)\longrightarrow C \end{aligned}$$

the natural projection. Consider a Poisson structure on X given by a bivector \(\sigma \in H^0(X, \wedge ^2T_X)\). Let \(({{\mathcal {E}}},\phi )\) be a nilpotent Higgs bundle on C. S. Rayan showed in [15] that \((\pi ^*{{\mathcal {E}}},\sigma (\pi ^*\phi ))\) is a stable co-Higgs bundle on X.

4.3 Co-Higgs orbibundles on weighted projective spaces

Let \(w_{0},w_1,w_{2}\) be positive integers, set \(|w|:= w_0+ w_1 + w_2\). Assume that \(w_{0},w_1,w_{2}\) are relatively prime. Define an action of \({{\mathbb {C}}}^*\) in \({{\mathbb {C}}}^{3} \setminus \{0\}\) by

$$\begin{aligned} \begin{array}{ccc} {{\mathbb {C}}}^*\times ({{\mathbb {C}}}^{3} \setminus \{0\} )&{} \longrightarrow &{}( {{\mathbb {C}}}^{3} \setminus \{0\}) \\ \lambda . (z_0, z_1, z_2) &{} \longmapsto &{} (\lambda ^{w_0} z_0, \lambda ^{w_1} z_1, \lambda ^{w_2} z_2)\\ \end{array} \end{aligned}$$
(4.1)

and consider the weighted projective plane

$$\begin{aligned} {\mathbb {P}}(w_{0},w_1,w_{2}) := ({{\mathbb {C}}}^{3} \setminus \{0\} )/ \sim \end{aligned}$$

induced by the action above. We will denote this space by \({\mathbb {P}}(\omega )\). On \({\mathbb {P}}(\omega )\) we have an Euler sequence

$$\begin{aligned} 0\longrightarrow {\mathcal {O}}_{{\mathbb {P}}(\omega )} \mathop {\longrightarrow }\limits ^{\varsigma }\bigoplus _{i=0}^{2 }{\mathcal {O}}_{{\mathbb {P}}(\omega )}(\omega _i) \longrightarrow T{\mathbb {P}}(\omega ) \longrightarrow 0, \end{aligned}$$

where \({\mathcal {O}}_{{\mathbb {P}}(\omega )}\) is the trivial line orbibundle and \(T{\mathbb {P}}(\omega ) = {\mathrm {Hom}} (\Omega _{{\mathbb {P}}(\omega )}^ 1, {\mathcal {O}}_{{\mathbb {P}}(\omega )} )\) is the tangent orbibundle of \({\mathbb {P}}(\omega )\). The map \(\varsigma \) is given explicitly by \( \varsigma (1)=(\omega _0z_0,\omega _1z_1,\omega _2z_2).\) Now, let \(({{\mathcal {E}}},\phi )\) be a co-Higgs orbibundle on \({\mathbb {P}}(\omega )\). Tensoring the Euler sequence by \(End({{\mathcal {E}}})\), we obtain

$$\begin{aligned} 0 \longrightarrow End({{\mathcal {E}}}) \longrightarrow \bigoplus \limits _{i=0}^2 End({{\mathcal {E}}}) ( \omega _i ) \longrightarrow End({{\mathcal {E}}}) \otimes T {\mathbb {P}}(\omega ) \longrightarrow 0. \end{aligned}$$

Thus, the co-Higgs fields \(\phi \) can be represented, in homogeneous coordinates, by

$$\begin{aligned} \phi =\phi _0\otimes \frac{\partial }{\partial z_0}+\phi _1\otimes \frac{\partial }{\partial z_1}+\phi _2\otimes \frac{\partial }{\partial z_2} , \end{aligned}$$

where \(\phi _i\in H^0({\mathbb {P}}(\omega ), End({{\mathcal {E}}})(w_i))\), for all \(i=0,1,2\), and \( \phi +\theta \otimes R_\omega \) define the same co-Higgs field as \(\phi \), where \(R_\omega \) is the adapted radial vector field

$$\begin{aligned} R_\omega = \omega _0 z_0 \frac{\partial }{\partial z_0} +\omega _1 z_1 \frac{\partial }{\partial z_1}+ + \omega _2 z_2 \frac{\partial }{\partial z_2}, \end{aligned}$$

with \(\theta \) a endomorphism of \({{\mathcal {E}}}\). Suppose that

$$\begin{aligned} {{\mathcal {E}}}= {\mathcal {O}}(m_1) \oplus {\mathcal {O}}(m_2) \end{aligned}$$

and that there exists a stable \(\phi \) for \({{\mathcal {E}}}\) such that \(m_1 \ge m_2\). Then

$$\begin{aligned} |m_1- m_2| \le \max \limits _{0 \le i\ne j \le 2}\{\omega _{i}+\omega _{j} \}. \end{aligned}$$

In fact, this is a consequence of Bott’s Formulae for weighted projective spaces. It follows from (see [5]) that

$$\begin{aligned} {\mathrm {H}}^0({\mathbb {P}}(\omega ),T{\mathbb {P}}(\omega )\otimes {\mathcal {O}}_{\omega }(k))\simeq {\mathrm {H}}^0({\mathbb {P}}(\omega ), \Omega ^{1}_{{\mathbb {P}}(\omega )}\left( \sum \nolimits _{i=0}^{2} \omega _{i}+k)\right) \ne \emptyset \end{aligned}$$

if and only if \(k>-\max \limits _{0 \le i\ne j \le 2}\{\omega _{i}+\omega _{j} \}\). This generalize the example given by S. Rayan in [14].

4.4 Co-Higgs bundles on two dimensional complex tori

Let X be a two dimensional complex torus and a co-Higgs bundle \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\). Then \(\phi \) is equivalente to a pair of commutative endomorphism of \({{\mathcal {E}}}\). In fact, since the tangent bundle \(T_X\) is holomorphically trivial, we can take a trivialization by choosing two linearly independent global vector fields \(v_1,v_2\in H^0(X,T_X)\). Then, we can write

$$\begin{aligned} \phi = \phi _1 \otimes v_1 +\phi _2 \otimes v_2. \end{aligned}$$

The condition \(\phi \wedge \phi =0\) implies that

$$\begin{aligned} \phi _1\circ \phi _2=\phi _2\circ \phi _1. \end{aligned}$$

We have a canonical nilpotent co-Higgs bundle \(({{\mathcal {E}}},\phi )\), where \({{\mathcal {E}}}=T_X={\mathcal {O}}\oplus {\mathcal {O}}\) and

$$\begin{aligned} \left( {\begin{array}{*{20}c} 0 &{} v \\ 0 &{} 0 \\ \end{array} } \right) , \end{aligned}$$

where v is a global vector field on X.

5 Proof of Theorem

By using that the Higgs field \(\phi \in H^0(X,End({{\mathcal {E}}})\otimes T_X)\) is nilpotent we have that \(Ker(\phi )=:L\) is a well defined line bundle on X. Thus , we have a exact sequence

$$\begin{aligned} 0\rightarrow L\longrightarrow {{\mathcal {E}}}\longrightarrow {\mathcal {I}}_Z\otimes N \longrightarrow 0, \end{aligned}$$

where the nilpotent Higgs field \(\phi \) factors as

$$\begin{aligned} \begin{array}{ccc} {{\mathcal {E}}}&{} \longrightarrow &{}{{\mathcal {E}}}\otimes T_X \\ \\ \downarrow &{} &{} \uparrow \\ \\ {\mathcal {I}}_Z\otimes N&{} \longrightarrow &{}L\otimes T_X. \end{array} \end{aligned}$$
(5.1)

The morphism \({\mathcal {I}}_Z\otimes N\rightarrow L\otimes T_X \) induces a holomorphic foliation on X which induces a global section \(\zeta _{\phi } \in H^0(X, T_X\otimes L\otimes N^*)\). Since \(\det ({{\mathcal {E}}})=L\otimes N\) we conclude that \(L\otimes N^*=L^2\otimes \det ({{\mathcal {E}}}^*) \). Then

$$\begin{aligned} \zeta _{\phi }\in H^0(X, T_X\otimes L^2\otimes \det ({{\mathcal {E}}}^*) ). \end{aligned}$$

Let \(K:=L^2\otimes \det ({{\mathcal {E}}}^*)\) the canonical bundle of the foliation \(\mathcal {F}\) associated to the co-Higgs fields \(\phi \). If \({{\mathcal {E}}}\) is semi-stable then

$$\begin{aligned}{}[c_1(K)]\cdot [\omega ]=[2c_1(L)- c_1({{\mathcal {E}}})]\cdot [\omega ]\le 0 \end{aligned}$$

for some Kähler class \(\omega \). If \(K\cdot [\omega ]<0\), it follows from [11] that K is not pseudo-efective [4]. It follows from Brunella’s Theorem [1] that X is uniruled.

Now, suppose X is a normal projective surface and that \(K\cdot H=0\), for some H ample By Hodge index theorem we have that \(K^2\cdot H^2\le (K\cdot H)^2=0\), then \(K^2\le 0\). Suppose that \(K^2<0\). We have that \(D=H+\epsilon K\) is a \({\mathbb {Q}}\)-divisor ample for \(0<\epsilon <<1\), see [12, proposition 1.3.6]. Thus, we have that

$$\begin{aligned} K\cdot D=K\cdot H+\epsilon ^2K^2=\epsilon ^2 K^2<0. \end{aligned}$$

By Bogomolov-McQuillan-Miyaoka’s theorem [3] we conclude that X is uniruled. If \(K^2=0\), then K is numerically trivial. This fact is well known, but for convenience of the reader we give a proof. Suppose that there exists \(C\subset X\) such that \(K\cdot C>0\). Now, Consider the divisor \(B=(H^2)C-(H\cdot C)H\). Then \(B\cdot H=0\) and \(K\cdot B=(H^2)K\cdot C<0.\) Define \(F=mK+B\) for \(0<m<<1\). Therefore \(F\cdot H=0\) and \(F^2>0\). This is a contradiction by the Hodge index Theorem. In this case \({{\mathcal {E}}}\) is strictly semi-stable.

Now, we apply the classification, up to finite étale cover, of holomorphic foliations on projective surfaces with canonical bundle numerically trivial [2, 13, 17]. Therefore, up to finite étale cover, either:

  1. (i)

    X is uniruled;

  2. (ii)

    X is a torus;

  3. (iii)

    \(k(X)=1\) and \(X=B\times C\) with \(g(B)\ge 2\), C is elliptic. That is, X is a sesquielliptic surface.

If X is Kähler and non-algebraic it follows from [2] that, up to finite étale cover, either X has a unique elliptic fibration or X is a torus.

6 Proof of Corollary 1.1

Since \(({{\mathcal {E}}},\phi )\) is nilpotent and stable the co-Higgs fields induces a foliation \(\mathcal {F}\) by rational curves on X. Now, consider the projective bundle \(\pi :{\mathbb {P}}({{\mathcal {E}}}) \rightarrow X\). Then the foliation by symplectic leaves \({\mathcal {G}}\) on \({\mathbb {P}}({{\mathcal {E}}})\) is the pull-back of \(\mathcal {F}\) by \(\pi \). In particular, a closure of the a leaf of the foliation by symplectic leaves \({\mathcal {G}}\) is of type \(\pi ^{-1}(f({\mathbb {P}}^1))\), where \(f:{\mathbb {P}}^1\rightarrow X\) is the uniformization of a rational leaf of \(\mathcal {F}\). Clearly \(\pi ^{-1}(f({\mathbb {P}}^1))\) is a rational surface.