ARCHIVUM MATHEMATICUM (BRNO) Tomus 47 (2011), 77–82 THE FIRST EIGENVALUE OF SPACELIKE SUBMANIFOLDS IN INDEFINITE SPACE FORM Rpn+p Yingbo Han and Shuxiang Feng Abstract. In this paper, we prove that the first eigenvalue of a complete spacelike submanifold in Rpn+p with the bounded Gauss map must be zero. 1. Introduction n Let M be a complete noncompact Riemannian manifold and Ω ⊂ M n be a domain with compact closure and nonempty boundary ∂Ω. The Dirichlet eigenvalue λ1 (Ω) of Ω is defined by R |∇f |2 dM 2 λ1 (Ω) = inf ΩR : f ∈ L (Ω) {0} , 1,0 f 2 dM M where dM is the volume element on M n and L21,0 (Ω) the completion of C0∞ with respect to the norm Z Z kϕk2Ω = ϕ2 dM + |∇ϕ|2 dM . M M If Ω1 ⊂ Ω2 are bounded domains, then λ1 (Ω1 ) ≥ λ1 (Ω2 ) ≥ 0. Thus one may define the first Dirichlet eigenvalue of M n as the following limit λ1 (M ) = lim λ1 B(p, r) ≥ 0 , r→∞ where B(p, r) is the geodesic ball of M n with radius r centered at p. It is clear that the definition of λ1 (M ) does not depend on the center point p. It is interesting to ask that for what geometries a noncompact manifold M n has zero first eigenvalue. Cheng and Yau [1] showed that λ1 (M ) = 0 if M n has polynomial volume growth. In [5], B. Wu proved the following result. Theorem A. Let M n be a complete spacelike hypersurface in R1n+1 whose Gauss map is bounded, then λ1 (M ) = 0. In this note, we discover that Wu’s result still holds for higher codimensional complete spacelike submanifolds in Rpn+p . In fact, we prove 2010 Mathematics Subject Classification: primary 53C42; secondary 53B30. Key words and phrases: spacelike submanifolds, the first eigenvalue. The first author is supported by NSFC grant No. 10971029 and NSFC-TianYuan Fund. No. 11026062. Received September 17, 2010. Editor O. Kowalski. 78 Y. HAN AND S. FENG Theorem 3.1. Let M n be a complete spacelike submanifold in Rpn+p whose Gauss map is bounded, then λ1 (M ) = 0. 2. The geometry of pseudo-Grassmannian In this section we review some basic properties about the geometry of pseudo-Grassmannian. For details one referred to see [6, 3]. Let Rpn+p be the (n + p)-dimensional pseudo-Euclidean space with index p, where, for simplicity, we assume that n ≥ p. The case n < p can be treated similarly. We choose a pseudo-Euclidean frame field {e1 ,P . . . , en+p } such P that the pseudo-Euclidean metric of Rpn+p is given by ds2 = (ωi )2 − α ωα = i P 2 A εA (ωA ) , where {ω1 , . . . , ωn=p } is the dual frame field of {e1 , . . . , en+p }, εi = 1 and εα = −1. Here and in the following we shall use the following convention on the ranges of indices: 1 ≤ i, j, · · · ≤ n; n + 1 ≤ α, β, · · · ≤ n + p ; 1 ≤ A, B, · · · ≤ n + p . The structure equations of Rpn+p are given by X deA = − εA ωAB eB , B dωA = − X ωAB ∧ ωB , ωAB + ωBA = 0 , B dωAB = − X εC ωAC ∧ ωCB . C Let Gpn,p be the pseudo-Grassmannian of all spacelike n-subspace in Rpn+p , and p n+p g G . They are n,p be the pseudo-Grassmannian of all timelike p-subspace in R p specific Cartan-Hadamard manifolds, and the canonical Riemannian metric on p g Gpn,p and G n,p is X dsG = dsG (ωαi )2 . e= iα Rpn+p . 0 Let 0 be the origin of Let SO (n + p, p) denote the identity component of the Lorentzian group O(n + p, p). SO0 (n + p, p) can be viewed as the manifold consisting of all pseudo-Euclidean frames (0; ei , eα ), and SO0 (n + p, p)/SO(n) × p p g SO(p) can be viewed as Gp or G can be represented by n,p . Any element in G n,p n,p p g a unit simple n-vector e1 ∧ · · · ∧ en , while any element in G n,p can be represented by a unit simple p-vector en+1 ∧ · · · ∧ en+p . They are unique up to an action of SO(n) × SO(p). The Hodge star ∗ provides an one to one correspondence between p p g Gpn,p and G n,p . The product h, i on Gn,p for e1 ∧ · · · ∧ en , v1 ∧ · · · ∧ vn is defined by he1 ∧ · · · ∧ en , v1 ∧ · · · ∧ vn i = det hei , vj i . p g The product on G n,p can be defined similarly. Now we fix a standard pseudo-Euclidean frame ei , eα for Rpn+p , and take g0 = p g e ∧ · · · ∧ e ∈ Gp , ge = ∗g = e ∧ ··· ∧ e ∈G n,p . Then we can span the 1 n n,p 0 0 n+1 n+p n+p THE FIRST EIGENVALUE OF SPACELIKE SUBMANIFOLDS IN Rp 79 spacelike n-subspace g in a neighborhood of g0 by n spacelike vectors fi : X fi = e i + ziα eα , α where (ziα ) are the local coordinates of g. By an action of SO(n) × SO(p) we can assume that µ1 .. . (ziα ) = . µp 0 From [3] we know that the normal geodesic g(t) between g0 and g has local coordinates tanh(λ1 t) .. . (ziα ) = , tanh(λp t) 0 Pp for real numbers λ1 . . . λp such that i=1 λ2i = 1. This means that g(t) is spanned by f1 (t) = e1 + tanh(λ1 t)en+1 , . . . , fp (t) = ep + tanh(λp t)en+p , fp+1 = ep+1 , . . . , fn = en . Consequently, g(t) can also be represented by a unit simple n-vector as following: g(t) = cosh(λ1 t)e1 + sinh(λ1 t)en+1 ∧ · · · ∧ cosh(λp t e1 + sinh(λp t)en+p ) ∧ ep+1 ∧ · · · ∧ en . Set λα = λα−n , then it is clear that cosh(λ1 t)e1 + sinh(λ1 t)en+1 , . . . , cosh(λp t)e1 + sinh(λp t)en+p , ep+1 , . . . , en , sinh(λn+1 t)e1 + cosh(λn+1 t)en+1 , . . . , sinh(λn+p t)ep + cosh(λn+p t)en+p is again a pseudo-Euclidean frame for Rpn+p , so we have g = ∗g(t) = sinh(λn+1 t)e1 + cosh(λn+1 t)en+1 ∧ · · · ∧ sinh(λn+p t)ep g(t) g p + cosh(λn+p t)en+p ∈ G n,p . Thus we have hg0 , gi = (−1)p h∗g0 , ∗gi = (−1)p hge0 , gei = Y cosh(λα t) . α In this note, we also need the following lemma, Q P Lemma 2.1 ([4]). Let µ1 ≥ 1, . . . , µp ≥ 1 and α µα = C. Then α cosh2 (λα ) ≤ C 2 + p − 1, and the equality holds if and only if µi0 = C for some 1 ≤ i0 ≤ p and µi = 1 for any i 6= i0 . 80 Y. HAN AND S. FENG 3. Main results for space-like submanifolds In this note, we get the following result: Theorem 3.1. Let M n be a complete space-like submanifold in Rpn+p whose Gauss map is bounded, then we have λ1 (M ) = 0. Proof. We choose a local frames e1 . . . , en+p in Rpn+p such that restricted to M n , e1 , . . . , en are tangent to M n , en+1 , . . . , en+p are normal to M n , the Gauss map p g is defined by en+1 ∧ · · · ∧ en+p : M n → G n,p . Let us fix p-vector and n-vector p g an+1 ∧ · · · ∧ an+p ∈ G , a ∧ · · · ∧ a ∈ Gpn,p , where haα , aβ i = −δαβ and n,p 1 n hai , aj i = δij . We defined the projection Π : M n → Ran by n+p X Π(x) = x + (1) hx, aα iaα , α=n+1 where h, i is the standard indefinite inner product on Rpn+p and Ran the totally geodesic Euclidean n-space determined by a = an+1 ∧ · · · ∧ an+p which is defined by Ran = {x ∈ Rpn+p : hx, an+1 i = · · · = hx, an+p i = 0} . (2) It is clear from (1) that dΠ(X) = X + (3) n+p X hX, aα iaα α=n+1 for any tangent vector field on M n and consequently, |dΠ(X)|2 = |X|2 + (4) n+p X hX, aα i2 . α=n+1 From the equation (4), we know that the map Π : M n → Ran increases the distance. If a map, from a complete Riemannian manifold M1 into another Riemannian manifold M2 of same dimension, increases the distance, then it is a covering map and M2 is complete (in [2, VIII, Lemma 8.1]). Hence Π is a covering map, but Ran being simply connected this means that Π is in face a diffeomorphism between M n and Ran , and thus M n is noncompact. Now assume that the Gauss map p g en+1 ∧ · · · ∧ en+p : M n → G n,p is bounded, then there exists ρ > 0 such that 1 ≤ (−1)p hen+1 ∧ · · · ∧ en+p , an+1 ∧ · · · ∧ an+p i ≤ ρ . (5) From Section 2 we know that by an action of SO(n) × SO(p) we can assume that en+1 = sinh(λn+1 t)a1 + cosh(λn+1 t)an+1 , . . . , en+p = sinh(λn+p t)a1 + cosh(λn+p t)an+p , where P α λ2α = 1 and t ∈ R. n+p THE FIRST EIGENVALUE OF SPACELIKE SUBMANIFOLDS IN Rp 81 Write aα = a> − (6) n+p X haα , eβ ieβ , β=n+1 n where a> α denote the component of aα which is tangent to M , and α = n + 1, . . . , n + p. Since haα , aβ i = −δαβ , we have −1= (7) 2 |a> α| n+p X − 2 2 haα , eβ i2 = |a> α | − cosh (λα t) , β=n+1 where α = n + 1, . . . , n + p. It follows from Lemma 2.1 and Eq. (5), (7), we have (8) 1+ n+p X 2 |a> α| = α=n+1 n+p X cosh2 (λα t) − p + 1 ≤ Y cosh2 (λα t) ≤ ρ2 . α=n+1 From Eq.(4) and (8), we have (9) 2 2 |dΠ(X)| = |X| + n+p X 2 hX, a> αi 2 ≤ |X| (1 + α=n+1 n+p X 2 2 2 |a> α | ) ≤ ρ |X| . α=n+1 n for any tangent vector field on M . Let B(p, r) is the geodesic ball of M n with e p, ρr) e p, ρr), where B(e radius r centered at p ∈ M n . We claim that Π(B(p, r)) ⊂ B(e denotes the geodesic ball of Ran with radius ρr centered at pe = Π(p). In fact, for any qe ∈ Π(B(p, r)) let q ∈ B(p, r) be the unique point such that Π(q) = qe, and γ : [a, b] → M n is the minimal geodesic joining p and q, then from (9) we have Z b Z b e p, qe) ≤ L(Π ◦ r) = dΠ γ 0 (t) dt ≤ ρ d(e |γ 0 (t)| dt = ρL(γ) = ρd(p, q) ≤ ρr , a a Ran where de and d denote the distance in and M n , respectively. This prove our claim. Let dV denotes the n-dimensional volume element on Ran . Using (3) and (6) it follows that Π∗ (dV )(X1 , . . . , Xn ) = det dΠ(X1 ), . . . , dΠ(Xn ), an+1 , . . . , an+p = det(X1 , . . . , Xn , an+1 , . . . , an+p ) = (−1)p hen+1 ∧ · · · ∧ en+p , an+1 ∧ · · · ∧ an+p i det(X1 , . . . , Xn , en+1 , . . . , en+p ) = (−1)p hen+1 ∧ · · · ∧ en+p , an+1 ∧ · · · ∧ an+p i dM (X1 , . . . , Xn ) for any tangent vector fields X1 , . . . , Xn of M n . In other words, (10) Π∗ (dV ) = (−1)p hen+1 ∧ · · · ∧ en+p , an+1 ∧ · · · ∧ an+p idM ≥ dM . 82 Y. HAN AND S. FENG e p, ρr) and Π : M n → Ran is diffeomorphism, it follows from Since Π(B(p, r)) ⊂ B(e Eq. (10) that Z n n e ρ r ωn = Vol B(e p, ρr) ≥ Vol Π(B(p, r)) = dV Π(B(p,r)) Z Z (11) = Π∗ dV ≥ dM = Vol B(p, r) , B(p,r) B(p,r) where ωn denotes the volume of unit ball in Euclidean n-space. (11) means that the order of the volume growth of M n is not larger than n, thus by [1] we see that λ1 (M ) = 0. References [1] Cheng, S. Y., Yau, S. T., Differential equations on Riemannian manifolds and geometric applications, Comm. Pure Appl. Math. 28 (1975), 333–354. [2] Kobayashi, S., Nomizu, K., Foundations of differential geometry, John Wiley & Sons, Inc., 1969. [3] Wong, Y. C., Euclidean n-space in pseudo-Euclidean spaces and differential geometry of Cartan domain, Bull. Amer. Math. Soc. (N.S.) 75 (1969), 409–414. [4] Wu, B. Y., On the volume and Gauss map image of spacelike submanifolds in de Sitter space form, J. Geom. Phys. 53 (2005), 336–344. [5] Wu, B. Y., On the first eigenvalue of spacelike hypersurfaces in Lorentzian space, Arch. Math. (Brno) 42 (2006), 233–238. [6] Xin, Y. L., A rigidity theorem for spacelike graph of higher codimension, Manuscripta Math. 103 (2000), 191–202. College of Mathematics and information Science, Xinyang Normal University, Xinyang 464000, Henan, P. R. China E-mail: yingbhan@yahoo.com.cn fsxhyb@yahoo.com.cn