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http://dx.doi.org/10.4134/JKMS.2015.52.5.1037

THE SYMMETRY OF spin C DIRAC SPECTRUMS ON

RIEMANNIAN PRODUCT MANIFOLDS

Kyusik Hong and Chanyoung Sung

Abstract. It is well-known that the spectrum of a spin C Dirac operator on a closed Riemannian spin C manifold M 2k of dimension 2k for k ∈ N is symmetric. In this article, we prove that over an odd-dimensional Riemannian product M 1 2p × M 2 2q+1 with a product spin C structure for p ≥ 1, q ≥ 0, the spectrum of a spin C Dirac operator given by a product connection is symmetric if and only if either the spin C Dirac spectrum of M 2 2q+1 is symmetric or (e 1 2 c 1 (L 1 ) A(M ˆ 1 ))[M 1 ] = 0, where L 1 is the associated line bundle for the given spin C structure of M 1 .

1. Introduction

This article is a generalization of the paper [7] to a spin C Dirac operator on a spin C manifold. Let (M n , g) be an n-dimensional closed Riemannian manifold with a spin C structure given by an associated complex line bundle L with c 1 (L) ≡ w 2 (M n ) mod 2. Here c 1 is the first Chern class and w 2 is the 2-nd Stiefel-Whitney class. Let A be a U (1)-connection on the line bundle L. This combined with the Levi-Civita connection of g induces a covariant derivative

A : Γ(Σ(M, L)) → Γ(T M ⊗ Σ(M, L))

in the associated spinor bundle Σ(M, L). The associated spin C Dirac operator D A is the composition of the covariant derivative ∇ A and Clifford multiplica- tion γ

D A = γ ◦ ∇ A : Γ(Σ(M, L)) → Γ(T M ⊗ Σ(M, L)) → Γ(Σ(M, L)).

Then D A is a self-adjoint elliptic operator of first-order. Therefore the spectrum Spec(D A ) of D A is discrete and real. The behavior of Spec(D A ) generally depends on the U (1)-connection A, the metric, and the spin C structure. For general properties of Dirac operators we refer to [4, 8].

Definition 1.1. The Spec(D A ) is called symmetric, if the following conditions hold:

Received December 7, 2014; Revised February 12, 2015.

2010 Mathematics Subject Classification. 53C27, 58C40.

Key words and phrases. Dirac operator, spin C manifold, spectrum, eta invariant.

c

2015 Korean Mathematical Society

1037

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(1) There exits −λ ∈ Spec(D A ) whenever λ ∈ Spec(D A ).

(2) The multiplicity of −λ is equal to that of λ.

If n is even, then the volume form µ of (M n , g) anti-commutes with the spin C Dirac operator D A

D A ◦ µ = −µ ◦ D A . Thus, in this case Spec(D A ) is symmetric.

Since D A is elliptic, each eigenspace is finite-dimensional. The asymmetry of Spec(D A ) on an odd-dimensional manifold was investigated by Atiyah, Patodi and Singer [1] via the eta funtion defined as

η D A (s) := X

λ6=0

sign(λ)

|λ| s , s ∈ C,

where λ runs through the eigenvalues according to their multiplicities. The series η D A (s) converges for sufficiently large Re(s) and has the meromorphic continuation to the whole C with η D A (0) finite. They showed that the value η D A (0), called the eta invariant of D A , appears as a global correction term for the index theorem for compact manifolds with boundary. Note that η D A (s) ≡ 0 is a necessary condition for the symmetry of Spec(D A ).

In this paper, we prove a necessary and sufficient condition for the symmetry of Spec(D A ) on odd-dimensional Riemannian spin C product manifolds using the ideas mainly adapted from that of E. C. Kim [7]. We will take a convention that a superscript on a manifold denotes its dimension.

Theorem 1.2. Let (Q n := M 1 2p ×M 2 2q+1 , h := g 1 +g 2 ) be a Riemannian product of two closed Riemannian spin C manifolds (M 1 2p , g 1 ), p ≥ 1, and (M 2 2q+1 , g 2 ), q ≥ 0. Let π 1 : Q n → M 1 2p and π 2 : Q n → M 2 2q+1 be the natural projections.

Suppose that M 1 (resp. M 2 ) is equipped with a spin C structure given by a complex line bundle L 1 (resp. L 2 ) with c 1 (L 1 ) ≡ w 2 (M 1 2p ) mod 2 (resp. c 1 (L 2 )

≡ w 2 (M 2 2q+1 ) mod 2), and M 1 ×M 2 is equipped with the product spin C structure given by the complex line bundle L = π 1 (L 1 ) ⊗ π 2 (L 2 ).

Let A 1 (resp. A 2 ) be a U (1)-connection on L 1 (resp. L 2 ), and A = π 1 (A 1 )+

π 2 (A 2 ) be a connection of L. Let D M A 1 1 , D M A 2 2 , and D A be the associated spin C Dirac operators of (M 1 2p , g 1 ), (M 2 2q+1 , g 2 ), and (Q n , h), respectively. Then we have the following:

Spec(D A ) is symmetric if and only if either Spec(D M A 2 2 ) is symmetric or (e 1 2 c 1 (L 1 ) A(M ˆ 1 ))[M 1 ] = 0, where ˆ A(M 1 ) denotes the ˆ A-class of T M 1 .

As a result auxiliary, we generalize real and quaternionic structures of spinor

bundles on spin manifolds to complex anti-linear mappings between Σ(M, L)

and Σ(M, −L) on spin C manifolds, and study several variations on product

spin C manifolds. These may be used as tools for studying the spectrum of a

spin C Dirac operator on a product spin C manifold.

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2. Preliminaries

This section is divided into two parts. In the first part, we explain that the spinor bundle of a Riemannian spin C product manifold has a natural tensor- product splitting. In the second part, we prove the decomposition property of L 2 -sections of a vector bundle given by the tensor product of two vector bundles.

Consider the following commutative diagram:

Spin C (k 1 + k 2 ) oo ? _

π



Spin C (k 1 ) ⊗ S

1

Spin C (k 2 ) ∋ (±a 1Z

2

±e

iθ12

) ⊗ S

1

(±a 2Z

2

±e

iθ22

)



SO(k 1 + k 2 ) ⊕ S 1 oo ? _

SO(k 1 ) ⊕ SO(k 2 ) ⊕ S 1 ∋ (a 1 , a 2 , e i(θ

1

2

) ),

where π is a 2-fold covering map.

Let P M 1 , P M 2 , and P Q be the SO(k 1 )-, SO(k 2 )-, and SO(k 1 + k 2 )-principal bundles of positively oriented orthonormal frames of (M 1 k 1 , g 1 ), (M 2 k 2 , g 2 ), and (Q n := M 1 k 1 × M 2 k 2 , h := g 1 + g 2 ), respectively. Let L 1 (resp. L 2 ) be a complex line bundle with c 1 (L 1 ) ≡ w 2 (M 1 k 1 ) mod 2 (resp. c 1 (L 2 ) ≡ w 2 (M 2 k 2 ) mod 2), and let L = π 1 L 1 ⊗π 2 L 2 , where π 1 : Q → M 1 and π 2 : Q → M 2 are the natural projections. To denote the double cover of a principal bundle, we will put e.

Then the above pointwise diagram globalizes over the whole manifold to give the following commutative diagram:

P ^ Q ⊕ L oo ? _

π



π 1 ( ^ P M 1 ⊕ L 1 ) ⊗ S 1 π 2 ( ^ P M 2 ⊕ L 2 )



P Q ⊕ (π 1 L 1 ⊗ π 2 L 2 ) oo ? _

1 P M 1 ⊕ π 2 P M 2 ) ⊕ (π 1 L 1 ⊗ π 2 L 2 ).

Thus, the Spin C (k 1 + k 2 )-principle bundle ^ P Q ⊕ L over (Q n , h) reduces to the Spin C (k 1 ) ⊗ S 1 Spin C (k 2 )-principal bundle π 1 ( ^ P M 1 ⊕ L 1 ) ⊗ π 2 ( ^ P M 2 ⊕ L 2 ) in a π-equivariant way.

Let (E 1 , . . . , E k 1 ) and (F 1 , . . . , F k 2 ) be local orthonormal frames on (M 1 k 1 , g 1 ) and (M 2 k 2 , g 2 ), respectively. We identify (E 1 , . . . , E k 1 ) and (F 1 , . . . , F k 2 ) with their lifts to (Q n , h). We may then regard (E 1 , . . . , E k 1 , F 1 , . . . , F k 2 ) as a local orthonormal frame on (Q n , h). Let µ 1 = E 1 ∧ · · · ∧ E k 1 , E t := g 1 (E t , ·), and µ 2 = F 1 ∧ · · · ∧ F k 2 , F l := g 2 (F l , ·), be the volume forms of (M 1 k 1 , g 1 ) and (M 2 k 2 , g 2 ), respectively, as well as their lifts to (Q n , h).

Now let’s assume that at least one of k 1 and k 2 is even. Say, k 1 = 2p for p ∈ N. Using the following Clifford action on the tensor product vector space [7, Section 2], one can extend the Spin C (k 1 ) ⊗ S 1 Spin C (k 2 )-action on △ k 1 ⊗ △ k 2

to the Spin C (k 1 + k 2 )-action:

(2.1) E t · (ϕ 1 ⊗ ϕ 2 ) = (E t · ϕ 1 ) ⊗ ϕ 2 , t = 1, . . . , 2p, (2.2) F l · (ϕ 1 ⊗ ϕ 2 ) = ( √

−1) p (µ 1 · ϕ 1 ) ⊗ (F l · ϕ 2 ), l = 1, . . . , k 2 ,

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where ϕ 1 ∈△ k 1 and ϕ 2 ∈△ k 2 . If k 2 = 2p, the Clifford actions are defined as:

E t · (ϕ 1 ⊗ ϕ 2 ) = (E t · ϕ 1 ) ⊗ ( √

−1) p (µ 2 · ϕ 2 ), t = 1, . . . , k 1 , F l · (ϕ 1 ⊗ ϕ 2 ) = ϕ 1 ⊗ (F l · ϕ 2 ), l = 1, . . . , 2p.

Hence we can conclude that the associated vector bundle π 1 (Σ(M 1 , L 1 )) ⊗ π 2 (Σ(M 2 , L 2 )) for the principal bundle π 1 ( ^ P M 1 ⊕ L 1 ) ⊗ S 1 π 2 ( ^ P M 2 ⊕ L 2 ) is also an associated vector bundle for ^ P Q ⊕ L.

Recall that there is a unique spinor bundle Σ(M 1 × M 2 , L) on M 1 × M 2 , if k 1 + k 2 is even, and there exist two of them, if k 1 + k 2 is odd. Suppose that dim M 1 = 2p and dim M 2 = 2q + 1 for p ≥ 1 and q ≥ 0. Then we have two non-isomorphic spinor bundles

Σ(M 1 , L 1 ) ⊗ Σ (M 2 , L 2 ) and Σ(M 1 , L 1 ) ⊗ Σ ′′ (M 2 , L 2 )

on M 1 ×M 2 , where Σ(M 1 , L 1 ) is a unique spinor bundle on M 1 , and Σ (M 2 , L 2 ), Σ ′′ (M 2 , L 2 ) denote two non-isomorphic spinor bundles corresponding to Σ(M 2 , L 2 ) on M 2 (more precisely, they are the eigenbundles of +( √

−1) q+1 and

−( √

−1) q+1 under the action of µ 2 , respectively). One can easily check that Σ(M 1 , L 1 ) ⊗ Σ (M 2 , L 2 ) and Σ(M 1 , L 1 ) ⊗ Σ ′′ (M 2 , L 2 ) are the eigenbundles of +( √

−1) p+q+1 and −( √

−1) p+q+1 under the action of the volume form µ 1 ∧ µ 2 on M 1 × M 2 , respectively.

Since the tensor product bundle π 1 (Σ(M 1 , L 1 )) ⊗ π 2 (Σ(M 2 , L 2 )) and the spinor bundle Σ(M 1 × M 2 , L = π 1 L 1 ⊗ π 2 L 2 ) have the same dimension, we have proved the first part of the following:

Lemma 2.3. If at least one of k 1 and k 2 is even, then

Σ(M 1 × M 2 , L = π 1 L 1 ⊗ π 2 L 2 ) = π 1 (Σ(M 1 , L 1 )) ⊗ π 2 (Σ(M 2 , L 2 )).

If both k 1 and k 2 are odd, then

Σ(M 1 × M 2 , L = π 1 L 1 ⊗ π 2 L 2 )

= (π 1 (M 1 , L 1 )) ⊕ π 1 ′′ (M 1 , L 1 ))) ⊗ π 2 (Σ(M 2 , L 2 )).

The proof of the second part can be done in the same as the spin case, whose details can be found in [7, Section 4].

Moreover the connections on the LHS of the previous diagram are induced ones from the RHS, which are subbundles. A spin C connection on

π 1 ( ^ P M 1 ⊕ L 1 ) ⊗ S 1 π 2 ( ^ P M 2 ⊕ L 2 ),

which is lifted from downstairs is given by the tensor-product. Therefore, letting A i for i = 1, 2 and A = π 1 (A 1 ) + π 2 (A 2 ) be connections on L i and L respectively, and ∇ A 1 , ∇ A 2 , and ∇ A be the spinor derivatives of Σ(M 1 , L 1 ), Σ(M 2 , L 2 ), and Σ(M 1 × M 2 , L) respectively, we have

(2.4) ∇ A X (ϕ 1 ⊗ ϕ 2 ) = (∇ A π 1∗ 1 (X) ϕ 1 ) ⊗ ϕ 2 + ϕ 1 ⊗ (∇ A π 2∗ 2 (X) ϕ 2 )

for ϕ i ∈ Γ(π i (Σ(M i , L i ))) and X ∈ T (M 1 × M 2 ).

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Now we prove some analysis lemmas on general vector bundles.

Lemma 2.5. Let E and F be hermitian vector bundles over M 1 , M 2 , respec- tively, and π 1 E ⊗ π 2 F be the induced bundle over M 1 × M 2 , where each π l : M 1 ×M 2 → M l for l = 1, 2 is the natural projection. Let L 21 E ⊗π 2 F ), L 2 (E), L 2 (F ) be the completion, with respect to the L 2 -norm, of C 0 1 E ⊗ π 2 F), C 0 (E), C 0 (F ), respectively. Then we have

L 2 1 E ⊗ π 2 F ) = π 1 (L 2 (E)) ⊗ π 2 (L 2 (F )), where the over-line denotes the L 2 -completion.

Proof. Let {ϕ α (x)} and {ψ β (y)} be orthonormal bases for π 1 (L 2 (E)) and π 2 (L 2 (F )) respectively. Then {ϕ α (x) ⊗ ψ β (y)} forms an orthonormal set in L 2 1 E ⊗ π 2 F ), and hence

L 2 1 E ⊗ π 2 F ) ⊇ π 1 (L 2 (E)) ⊗ π 2 (L 2 (F )).

To prove the reverse direction, we will prove that {ϕ α (x)⊗ψ β (y)} is actually a maximal orthonormal set, i.e., basis. Let rank(E) = m and f ∈ C 0 1 E ⊗ π 2 F ). Take U × M 2 ⊂ M 1 × M 2 , where U is a small open neighborhood of a point in M 1 . Since f | x×{M 2 } for each x ∈ U is continuous and hence in L 2 (F ), the section f on U × M 2 is expressed as

f (x, y) = (f 1 (x, y), . . . , f m (x, y)) = X

β

a β (x)ψ β (y)

= ( X

β

a β,1 (x)ψ β (y), . . . , X

β

a β,m (x)ψ β (y)).

Since f is continuous, we have the continuity of a β,k (x) = hf k (x, y), ψ β (y)i L 2 (F ) =

Z

M 2

hf k (x, y), ψ β (y)i F dy,

where h·, ·i F is the hermitian inner product on F . Applying the H¨ older’s in- equality, we obtain

Z

U |a β,k (x)| 2 dx ≤ Z

U

( Z

M 2

|f k (x, y)| Fβ (y)| F dy) 2 dx

≤ Z

U

( Z

M 2

|f k (x, y)| 2 F dy Z

M 2

|ψ β (y)| 2 F dy) dx

= Z

U

( Z

M 2

|f k (x, y)| 2 F dy ) dx < ∞,

where the finiteness is due to the fact that f ∈ L 21 E ⊗ π 2 F ) and hence f k ∈ L 2 1 E | U(p) ⊗ π 2 F). This implies that a β,k and hence a β are locally in L 2 . Moreover, since f ∈ Γ(π 1 E ⊗ π 2 F ) and ψ β ∈ Γ(π 2 F), we have

a β (x) = Z

M 2

hf(x, y), ψ β (y)i F dy ∈ Γ(π 1 E).

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Therefore, we can write

a β (x) = X

α

c αβ ϕ α (x) for c αβ ∈ C, and hence f can be expressed as

f (x, y) = X

β

X

α

c αβ ϕ α (x) ⊗ ψ β (y).

Because the subset of continuous sections is dense in the space of L 2 -sections,

the proof is completed. 

Remark 2.6. Lemma 2.5 remains valid when E and F are real vector bundles with Riemannian metrics over M 1 and M 2 , respectively.

Corollary 2.7. Let D M 1 : E → E (resp. D M 2 : F → F ) denote a linear self- adjoint elliptic differential operator on a complex vector bundle over a closed manifold M 1 (resp. M 2 ) and let Γ ρ (D M j ), for j ∈ {1, 2}, denote the space of all eigenvectors of D M j with eigenvalue ρ ∈ R. If D M 1 ⊗ Id + Id ⊗ D M 2 : π 1 E ⊗ π 2 F → π 1 E ⊗ π 2 F as an operator on M 1 × M 2 is elliptic, then we have

Γ γ (D M 1 ⊗ Id + Id ⊗ D M 2 ) = M

γ=χ+ν

1 (Γ χ (D M 1 )) ⊗ π 2 (Γ ν (D M 2 ))).

Proof. “ ⊇ ” part is obvious, and we will show the other direction. Note that D M 1 ⊗ Id + Id ⊗ D M 2 is also self-adjoint. Since the unit norm eigenvectors of D M 1 , D M 2 , and D M 1 ⊗Id+Id⊗D M 2 form orthonormal bases of L 2 (E), L 2 (F ), and L 2 1 E ⊗ π 2 F ), respectively, the proof follows from Lemma 2.5.  Lemma 2.8. Let D : E → E be a linear self-adjoint elliptic operator, where E is a complex vector bundle over a closed manifold M . Then all the eigenvectors of D 2 come from the eigenvectors of D, and the squares of the eigenvalues of D are exactly the eigenvalues of D 2 .

Proof. Obviously, the eigenvector of D is the eigenvector of D 2 . Since the unit norm eigenvectors of D form an orthonormal basis of L 2 (E), and the same is true for the unit norm eigenvectors of D 2 , the conclusion follows. 

3. Real and quaternionic structures

Let’s first review some basic properties of real or quaternionic structures j 0

and j 1 of the spinor representation. For more details, the readers are referred to [3, 4, 6, 7, 9].

The real Clifford algebra Cl(R n ) is multiplicatively generated by the stan-

dard basis {e 1 , . . . , e n } of the Euclidean space R n subject to the relations

e 2 i = −1 for all i ≤ n and e i e j = −e j e i for all i 6= j. Note that the di-

mension of Cl(R n ) is 2 n . The complexification Cl(R n ; C) := Cl(R n ) ⊗ R C is

isomorphic to the matrix algebra M (2 m ; C) for n = 2m and to the matrix al-

gebra M (2 m ; C) ⊕ M(2 m ; C) for n = 2m + 1. For an explicit isomorphism map

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for n ≥ 2, we refer to [5, Section 1] (or [7, Section 2]). Following them, let us denote by u(ǫ) ∈ C 2 the vector

(3.1) u(ǫ) := 1

√ 2

 1

−ǫ √

−1



, ǫ = ±1.

Then

(3.2) u(ǫ 1 , . . . , ǫ m ) := u(ǫ 1 ) ⊗ . . . , ⊗u(ǫ m ), m = [ n 2 ] ≥ 1,

form an orthonormal basis for the spinor space △ n := C 2 m , m = [ n 2 ] ≥ 1, with respect to the standard hermitian inner product.

Definition 3.3. The complex-antilinear mappings j 0 , j 1 :△ n →△ n defined, in the notations of (3.1) and (3.2), by

j 0 u(ǫ 1 , . . . , ǫ m ) = ( √

−1) P m α=1 αǫ α u (−ǫ 1 , . . . , −ǫ m ), j 1 u(ǫ 1 , . . . , ǫ m ) = ( √

−1) P m α=1 (m−α+1)ǫ α u (−ǫ 1 , . . . , −ǫ m ), m = [ n 2 ], are called the j 0 -structure and j 1 -structure, respectively.

The following facts are well-known [3, 7]. Fix m = [ n 2 ].

(A) j 0 ◦ e k = e k ◦ j 0 for all k = 1, . . . , 2m and j 0 ◦ e 2m+1 = (−1) m+1 e 2m+1 ◦ j 0 . Thus, the mapping j 0 :△ n →△ n is Spin(n)-equivariant for n, n 6≡

1 mod 4.

(B) j 1 ◦ e l = (−1) m+1 e l ◦ j 1 for all l = 1, . . . , n. Thus, the mapping j 1 :△ n →△ n is Spin(n)-equivariant for all n ≥ 2.

(C) j 0 ◦ j 0 = j 1 ◦ j 1 = (−1) m(m+1)/2 and j 0 ◦ j 1 = j 1 ◦ j 0 .

(D) hj 0 (ψ), j 0 (ϕ)i = hj 1 (ψ), j 1 (ϕ)i = hϕ, ψi, ϕ, ψ ∈△ n , where h·, ·i is the standard hermitian inner product on △ n .

Thus, j 0 (for n 6≡ 1 mod 4) and j 1 give real (resp. quaternionic) structures on

n as Spin(n)-representations, if m ≡ 0, 3 mod 4 (resp. m ≡ 1, 2 mod 4).

Let us now fix a local trivialization of Σ(M, L) on a spin C manifold M n . Namely, let ∪ α U α be an open covering of M for which there exits a system of transition functions {g α 1 α 2 : U α 1 ∩ U α 2 → Spin C (n) = Spin(n) ⊗ Z 2 S 1 }. Define g α 1 α 2 : U α 1 ∩ U α 2 → Spin C (n) by

x 7→ f(x) ⊗ Z 2 h(x),

where f (x) ⊗ Z 2 h(x) = g α 1 α 2 (x) for x ∈ U α 1 ∩ U α 2 , f (x) ∈ Spin(n) and h(x) ∈ S 1 . Then g α 1 α 2 is the transition function of a local trivialization for Σ(M, −L).

By the property (A), j 0 ◦(f(x)⊗ Z 2 h (x)) = (f (x)⊗ Z 2 h (x))◦j 0 for n 6≡ 1 mod 4.

Also, by the property (B), j 1 ◦ (f(x) ⊗ Z 2 h (x)) = (f (x) ⊗ Z 2 h (x)) ◦ j 1 for n ≥ 2.

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We then have the following commutative diagram:

U α 1 × △ n g α1α2

//

j r



U α 2 × △ n



j r



U α 1 × △ n g α1α2 // U α 2 × △ n ,

where r = 0 with n 6≡ 1 mod 4, or r = 1 with n ≥ 2. Thus, the mapping j r is compatible with the transition functions of Σ(M, L) and Σ(M, −L) so that the j 0 - and j 1 -structure can be globalized to mappings j 0 , j 1 : Σ(M, L) → Σ(M, −L), and we can carry all the properties (A)–(D) over to Σ(M, L). Be aware that the mapping j 0 is well-defined for n 6≡ 1 mod 4, and j 1 is well-defined for all n ≥ 2.

Lemma 3.4.

D −A ◦ j 0 = j 0 ◦ D A for n 6≡ 1 mod 4, and

D −A ◦ j 1 = (−1) m+1 j 1 ◦ D A .

Proof. Let (ω i,j ) be the so(n)-valued 1-form on U α coming from the Levi- Civita connection of (M n , g ). The spinor derivative ∇ A with respect to a U (1)-connection A in the bundle L is locally expressed as

j k (∇ A X s) = j k (X(s) + 1 2 ( √

−1A(X) + X

i<j

ω j,i (X)e i · e j ) · s)

= X(j k (s)) + 1 2 (− √

−1A(X) + X

i<j

ω j,i (X)e i · e j ) · j k (s)

= ∇ −A X j k (s),

where s ∈ Γ(Σ(M, L)), X ∈ Γ(T M), and k = 1, 2. Thus, we have (3.5) ∇ −A ◦ j 0 = j 0 ◦ ∇ A and ∇ −A ◦ j 1 = j 1 ◦ ∇ A .

Now the conclusion immediately follows from the properties (A) and (B).  As a corollary, we have proved that if m is odd (resp. even), then Spec(D A ) = Spec(D −A ) (resp. −Spec(D −A )) with the same multiplicities.

Now we take up the case of Theorem 1.2. Using (2.1), (2.2), and (2.4), one can easily verify the following formulas:

(3.6) D A (ϕ 1 ⊗ ϕ 2 ) = (D A M 1 1 ϕ 1 ) ⊗ ϕ 2 + ( √

−1) p (µ 1 · ϕ 1 ) ⊗ (D M A 2 2 ϕ 2 ), (3.7) (D A ) 2 (ϕ 1 ⊗ ϕ 2 ) = ((D A M 1 1 ) 2 ϕ 1 ) ⊗ ϕ 2 + ϕ 1 ⊗ ((D A M 2 2 ) 2 ϕ 2 )

for ϕ i ∈ Γ(π i (Σ(M i , L i ))).

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Consider the partial spin C Dirac operators D A + 1 , D A 2 acting on sections ψ ∈ Γ(Σ(Q, L)) of the spinor bundle over (Q n , h):

D + A 1 ψ = X 2p k=1

E k · ∇ A E 1 k ψ, D A 2 ψ =

2q+1 X

l=1

F l · ∇ A F l 2 ψ.

Define the twist e D A of the spin C Dirac operator D A = D + A 1 + D A 2 by D e A = D A + 1 − D − A 2 .

By (2.1) and (2.2), for i = 1, 2

D A + 1 ◦ µ i = −µ i ◦ D + A 1 , D A 2 ◦ µ i = µ i ◦ D − A 2 , and

(3.8) D A ◦ µ i = −µ i ◦ e D A , D e A ◦ µ i = −µ i ◦ D A . Since the Spin C (2p + 2q + 1)-principle bundle ^ P Q ⊕ L over

(Q n := M 1 2p × M 2 2q+1 , h)

reduces to the Spin C (2p) ⊗ S 1 Spin C (2q + 1)-principal bundle π 1 ( ^ P M 1 ⊕ L 1 ) ⊗ π 2 ( ^ P M 2 ⊕ L 2 ), the complex-antilinear mapping j :△ 2p+2q+1 →△ 2p+2q+1 de- fined by

j u(ǫ 1 , . . . , ǫ p , ǫ p+1 , . . . , ǫ p+q ) = {j 0 u(ǫ 1 , . . . , ǫ p )} ⊗ {j 1 u(ǫ p+1 , . . . , ǫ p+q )}, combining the j 0 - and j 1 -structure in Definition 3.3, globalizes to mapping j : Σ(Q, L) → Σ(Q, −L). Then the mapping j is well-defined for all p ≥ 1, q ≥ 1.

Using the properties (A) and (B) below Definition 3.3, the formulas (2.1) and (2.2), we have the following:

j ◦ E k = E k ◦ j , k = 1, . . . , 2p, j ◦ F l = (−1) p+q+1 F l ◦ j , l = 1, . . . , 2q + 1.

From the formulas (2.4) and (3.5), it follows that

−A ◦ j = j ◦ ∇ A , and hence

(3.9) D −A + 1 ◦ j = j ◦ D + A 1 , D −A 2 ◦ j = (−1) p+q+1 j ◦ D A2 .

Similarly we also define complex-antilinear mappings b j , j 0 , j 1 : Σ(Q, L) → Σ(Q, −L) as

bj u(ǫ 1 , . . . , ǫ p , ǫ p+1 , · · · , ǫ p+q ) = {j 1 u(ǫ 1 , . . . , ǫ p )} ⊗ {j 0 u(ǫ p+1 , . . . , ǫ p+q )}, j 0 u(ǫ 1 , . . . , ǫ p , ǫ p+1 , . . . , ǫ p+q ) = {j 0 u(ǫ 1 , . . . , ǫ p )} ⊗ {j 0 u(ǫ p+1 , . . . , ǫ p+q )}, j 1 u(ǫ 1 , . . . , ǫ p , ǫ p+1 , . . . , ǫ p+q ) = {j 1 u(ǫ 1 , . . . , ǫ p )} ⊗ {j 1 u(ǫ p+1 , . . . , ǫ p+q )}.

The mappings b j and j 0 are well-defined when q is odd, and j 1 is well-defined for all p ≥ 1, q ≥ 1. One can easily check that

D + −A 1 ◦ bj = (−1) p+1 bj ◦ D A + 1 , D −A 2 ◦ bj = (−1) p bj ◦ D A2 ,

(3.10)

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D + −A 1 ◦ j 0 = j 0 ◦ D A + 1 , D −A 2 ◦ j 0 = (−1) p j 0 ◦ D A2 , (3.11)

D + −A 1 ◦ j 1 = (−1) p+1 j 1 ◦ D A + 1 , D −A 2 ◦ j 1 = (−1) p+q+1 j 1 ◦ D − A 2 . (3.12)

Putting these together, we can produce various operators which anti-commute with spin C Dirac operators:

Proposition 3.13. Under the assumptions of Theorem 1.2 and with the above notations, for i = 1, 2:

(1) For p ≥ 1 and q ≥ 0, D A ◦ (µ i ◦ D A + 1 ) = −(µ i ◦ D A + 1 ) ◦ D A .

(2) Let p ≥ 1 and q ≥ 1. If p and q are either both even or both odd, then D −A ◦ (µ i ◦ j ) = −(µ i ◦ j ) ◦ D A .

(3) Let p ≥ 1 and q ≥ 1. If p and q are odd, then D −A ◦ (µ i ◦ bj ) =

−(µ i ◦ bj ) ◦ D A and D −A ◦ (µ i ◦ j 0 ) = −(µ i ◦ j 0 ) ◦ D A .

(4) Let p ≥ 1 and q ≥ 1. If p and q are even, then D −A ◦ j 1 = −j 1 ◦ D A . Proof. Since the Riemann curvatures R(E k , F l , ·, ·) = 0 vanish and the Clifford multiplication anti-commutes, we have

(3.14) D A 2 D A + 1 + D + A 1 D A 2 = 0.

Using (3.8) and (3.14), we obtain

D A ◦ (µ i ◦ D A + 1 ) = −µ i ◦ e D A ◦ D A + 1

= −µ i ◦ ((D A + 1 ) 2 − D − A 2 ◦ D A + 1 )

= −µ i ◦ ((D A + 1 ) 2 + D + A 1 ◦ D A2 )

= −µ i ◦ D + A 1 ◦ D A .

Suppose that p and q are either both even or both odd. By (3.8) and (3.9), we have

D −A ◦ (µ i ◦ j ) = −(µ i ◦ e D −A ) ◦ j = −µ i ◦ (D + −A 1 − D − −A 2 ) ◦ j

= −µ i ◦ j ◦ (D + A 1 + D A 2 ) = −(µ i ◦ j ) ◦ D A .

For the statement (3), we assume that p and q are odd. By (3.8), (3.10) and (3.11), we see that

D −A ◦ (µ i ◦ bj ) = −(µ i ◦ e D −A ) ◦ bj = −(µ i ◦ bj ) ◦ D A and D −A ◦ (µ i ◦ j 0 ) = −(µ i ◦ e D −A ) ◦ j 0 = −(µ i ◦ j 0 ) ◦ D A .

The statement (4) follows from (3.12). 

4. Proof of Theorem 1.2

By Corollary 2.7 and (3.7), we see that the eigenvalues of (D A ) 2 are all

possible sums of one eigenvalue of (D M A 1 1 ) 2 and one of (D M A 2 2 ) 2 .

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From now on, we omit the projections and rewrite the formula of Corollary 2.7 as

(4.1) Γ γ ((D A ) 2 ) = M

γ=χ+ν

(Γ χ ((D A M 1

1 ) 2 ) ⊗ Γ ν ((D M A 2

2 ) 2 )).

Using the decomposition

Σ(M, L) = Σ + (M, L) ⊕ Σ (M, L), where

Σ ± (M 1 , L 1 ) := {ϕ ∈ Σ(M 1 , L 1 ) | µ 1 · ϕ = ±( √

−1) p ϕ },

we have a decomposition Σ(Q, L) = Σ + (Q, L) ⊕ Σ (Q, L) due to the action of the volume form µ 1 = E 1 ∧ · · · ∧ E 2p ,

Σ ± (Q, L) := Σ ± (M 1 , L 1 ) ⊗ Σ(M 2 , L 2 ).

The positive part ψ + (resp. negative part ψ ) of ψ ∈ Γ(Σ(Q, L)) is in fact equal to

ψ ± = 1 2 ψ ± 1

2 (− √

−1) p µ 1 · ψ.

Lemma 4.2. Let Γ ± 0 (D A M 1 1 ) be the space of all positive (resp. negative) har- monic spinors of D M A 1

1 . For any λ 6= 0 ∈ Spec(D A ), define a complex vector space

H λ := {ψ ∈ Γ λ (D A ) | D A + 1 ψ = 0, D A 2 ψ = λψ}.

Then, in the notation (4.1), we have

H λ = {Γ + 0 (D M A 1 1 ) ⊗ Γ (−1) p λ (D A M 2 2 )} ⊕ {Γ 0 (D A M 1 1 ) ⊗ Γ −(−1) p λ (D A M 2 2 )}.

Proof. By (3.6), it is enough to show that

H λ ⊂ {Γ + 0 (D M A 1 1 ) ⊗ Γ (−1) p λ (D A M 2 2 )} ⊕ {Γ 0 (D A M 1 1 ) ⊗ Γ −(−1) p λ (D A M 2 2 )}.

Suppose that ψ ∈ H λ . Then ψ ∈ Γ λ 2 ((D A ) 2 ) and (4.1) implies that

(4.3) ψ = X

k,l

c k,l ϕ 0,k ⊗ ϕ λ 2 ,l , c k,l 6= 0 ∈ C,

is a finite linear combination of tensor products of some ϕ 0,k ∈ Γ 0 ((D M A 1 1 ) 2 ) and some ϕ λ 2 ,l ∈ Γ λ 2 ((D A M 2 2 ) 2 ). By the decomposition of Σ(Q, L), we can rewrite (4.3) as

ψ = X

k,l

c k,l ϕ + 0,k ⊗ ϕ λ 2 ,l + X

k,l

c k,l ϕ 0,k ⊗ ϕ λ 2 ,l ,

where ϕ ± 0,k ∈ Γ ± 0 ((D A M 1 1 ) 2 ). By Lemma 2.8, the eigenvalue λ 2 of (D M A 2 2 ) 2 comes from the eigenvalue λ or −λ of D A M 2 2 . Since D A 2 ψ = λψ, one can easily see from (3.6)

ψ ∈ {Γ + 0 (D M A 1 1 ) ⊗ Γ (−1) p λ (D A M 2 2 )} ⊕ {Γ 0 (D M A 1 1 ) ⊗ Γ −(−1) p λ (D A M 2 2 )}. 

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Proof of Theorem 1.2. At first, using Proposition 3.13(1), one can define a map:

f : Γ λ (D A ) ∩ H λ −→ Γ −λ (D A ) ∩ H −λ defined by ψ 7→ µ 1 · D + A 1 ψ, where H λ is the orthogonal complement of H λ . Note that f is bijective via the inverse map

f −1 := (−1) p (D A + 1 ) −1 · µ 1 . By Lemma 4.2,

(4.4) H −λ = {Γ + 0 (D M A 1 1 ) ⊗ Γ −(−1) p λ (D A M 2 2 )} ⊕ {Γ 0 (D M A 1 1 ) ⊗ Γ (−1) p λ (D A M 2 2 )}.

The symmetry of Spec(D A ) holds if and only if dim C H λ = dim C H −λ for any λ 6= 0 ∈ Spec(D A ). Letting dim C (Γ + 0 (D M A 1 1 )) = a 1 , dim C (Γ 0 (D M A 1 1 )) = a 2 , dim C (Γ (−1) p λ (D A M 2

2 )) = b 1,λ , and dim C (Γ −(−1) p λ (D A M 2

2 )) = b 2,λ , Lemma 4.2 and (4.4) give

dim C H λ − dim C H −λ = (a 1 − a 2 )(b 1,λ − b 2,λ )

= (ind (D A M 1 1 | Σ + (M 1 ,L 1 ) ))(b 1,λ − b 2,λ )

= (e 1 2 c 1 (L 1 ) A(M ˆ 1 ))[M 1 ](b 1,λ − b 2,λ ),

where the last equality is due to the Atiyah-Singer index theorem [8]. Now the

desired conclusion follows immediately. 

5. Examples

In this section, applying Theorem 1.2, we present an important example.

Let D 0 := i∂ θ be the Dirac operator of (S 1 , g 2 = dθ 2 ). Then the eigenvectors of unit L 2 -norm are

e inθ

√ 2π for n ∈ Z

with multiplicity 1, and hence Spec(D 0 ) = Z. Thus Spec(D 0 ) is symmetric, and since

X

n∈Z\{0}

sign(n)

|n| s = 0 for Re(s) ≫ 1,

η D 0 (s) = 0 for all s ∈ C. In [7], it is shown that the Dirac spectrum of (M 1 2p × S 1 , g 1 + g 2 ) for a spin manifold M 1 2p is symmetric. We can generalize this to the spin C case:

Example 5.1. Note that D −iadθ = D 0 + a for a ∈ R is a spin C Dirac operator of (S 1 , g 2 = dθ 2 ). Thus

Spec(D −iadθ ) = {n + a | n ∈ Z},

and hence Spec(D −iadθ ) is symmetric if and only if a ∈ Z ∪ 1 2 Z. In this

case, by Theorem 1.2, the spin C Dirac spectrum of (M 1 2p × S 1 , g 1 + g 2 ) for

any product spin C structure is symmetric, and hence the corresponding eta

invariant vanishes.

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The eta invariant of a spin C Dirac operator on a product spin C manifold M 1 2 ×S 1 appears when computing the dimension of the moduli space of Seiberg- Witten equations on a cylindrical-ended 4-manifold with asymptotic boundary equal to M 1 2 × S 1 . For details, the readers are referred to [10].

For general a, it is known that the eta invariant of D −iadθ is 1 − 2a. (See [10, Example 4.1.7] or [2].)

Acknowledgments. The first author was supported by National Researcher Program of the National Research Foundation (NRF) funded by the Ministry of Science, ICT and Future Planning (No.2014028806). The second-named author was supported by the National Research Foundation of Korea grant funded by the Korea government. (NRF-2014R1A1A4A01008987).

References

[1] M. F. Atiyah, V. K. Patodi, and I. M. Singer, Spectral asymmetry and Riemannian geometry I, Math. Proc. Cambridge Philos. Soc. 77 (1975), 43–69.

[2] , Spectral asymmetry and Riemannian geometry II, Math. Proc. Cambidge Phi- los. Soc. 78 (1975), 405–432.

[3] H. Baum, A remark on the spectrum of the Dirac operator on pseudo-Riemannian spin manifolds, SFB 288, Preprint 136, 1994.

[4] Th. Friedrich, Dirac Operators in Riemannian Geometry, Graduate Studies in Mathe- matics, vol. 25, AMS, Providence, RI, 2000.

[5] Th. Friedrich and E. C. Kim, The Einstein-Dirac equation on Riemannian spin mani- folds, J. Geom. Phys. 33 (2000), no. 1-2, 128–172.

[6] E. C. Kim, Die Einstein-Dirac-Gleichung ¨ uber Riemannschen Spin-Mannigfaltigkeiten, Thesis, Humboldt-Universit¨ at zu Berlin, 1999.

[7] , The ˆ A-genus and symmetry of the Dirac spectrum on Riemannian product manifolds, Differential Geom. Appl. 25 (2007), 309–321.

[8] H.-B. Lawson and M.-L. Michelsohn, Spin Geometry, Princeton University Press, Prince- ton, NJ, 1989.

[9] A. Lichnerowicz, Champs spinoriels et propagateurs en relativit´ e g´ en´ eral, Bull. Sci.

Math. France 92 (1964), 11–100.

[10] L. I. Nicolaescu, Notes on Seiberg-Witten Theory, Graduate Studies in Mathematics, 28. American Mathematical Society, Providence, RI, 2000.

Kyusik Hong

School of Mathematics

Korea Institute for Advanced Study Seoul 130-722, Korea

E-mail address: [email protected] Chanyoung Sung

Department of Mathematics Education Korea National University of Education Chungbuk 363-791, Korea

E-mail address: [email protected]

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