VOL. 73 1997 NO. 1
SOME NONEXISTENCE THEOREMS ON STABLE MINIMAL SUBMANIFOLDS
BY
HAIZHONG L I (BEIJING)
We prove that there exist no stable minimal submanifolds in some n- dimensional ellipsoids, which generalizes J. Simons’ result about the unit sphere and gives a partial answer to Lawson–Simons’ conjecture.
1. Introduction. In [S], J. Simons proved that there exist no stable minimal submanifolds in the n-dimensional unit sphere S n . In this paper, we establish the following general results.
Theorem 1. Let N n be an n-dimensional compact hypersurface in the (n + 1)-dimensional Euclidean space R n+1 . If the sectional curvature K of N n satisfies
(1) 1/2 < K ≤ 1,
then there exist no stable m-dimensional minimal submanifolds in N n for each m with 1 ≤ m ≤ n − 1.
R e m a r k 1. If N n is an n-dimensional unit hypersphere S n in R n+1 , then the sectional curvature K of S n is 1, and from Theorem 1 we deduce that there exist no stable m-dimensional minimal submanifolds in S n for each m with 1 ≤ m ≤ n − 1, which was proved by Simons [S].
Theorem 2. Let N n be an n-dimensional (n ≥ 4) compact submanifold in an (n + p)-dimensional Euclidean space R n+p . Let R and H denote the normalized scalar curvature and the mean curvature functions of N n , re- spectively. If R satisfies the following pointwise n(n − 2)/(n − 1) 2 -pinching condition :
(2) n(n − 2)
(n − 1) 2 H 2 < R ≤ H 2 ,
then there exist no stable m-dimensional minimal submanifolds in N n for each m with 2 ≤ m ≤ n − 2.
1991 Mathematics Subject Classification: Primary 53C42.
This work is supported by Postdoctoral Foundation of China.
[1]
Corollary 1. Let N n be an n-dimensional (n ≥ 4) compact hypersur- face in R n+1 . If all the principal curvatures k a of N n satisfy
(3) 0 < k a <
s 1
n(n − 1)
n
X
b=1
k b , 1 ≤ a ≤ n,
then there exists no m-dimensional minimal submanifold in N n for each m with 2 ≤ m ≤ n − 2.
As direct applications of Theorem 1 and Corollary 1, we have
Proposition 1. Let N n be the following n-dimensional (n ≥ 4) ellipsoid in R n+1 :
(4) N n : x 2 1
a 2 1 + . . . + x 2 n+1
a 2 n+1 = 1, 0 < a 1 ≤ a 2 ≤ . . . ≤ a n+1 , (1) If 1 ≤ a n+1 < √ 3
2 and a 1 ≥ √ a n+1 , then there exist no stable m- dimensional minimal submanifolds of N n for each m with 1 ≤ m ≤ n − 1.
(2) If a n+1 /a 1 < pn/(n − 1), then there exist no stable m-dimensional 6 minimal submanifolds of N n for each m with 2 ≤ m ≤ n − 2.
R e m a r k 2. It can be proved in a similar way that the above results all keep valid for stable m-currents on N n (for concepts of stable current, see Lawson–Simons [LS]). For example, we can state the counterpart of Theorem 1 as follows:
Theorem 1 ′ . Let N n be an n-dimensional compact hypersurface in the (n + 1)-dimensional Euclidean space R n+1 . If the sectional curvature K of N n satisfies
(5) 1/2 < K ≤ 1,
then there exist no stable m-currents on N n for each m with 1 ≤ m ≤ n − 1.
R e m a r k 3. Let N n be an n-dimensional compact hypersurface in R n+1 and suppose that every principal curvature k a of N n satisfies √
δ < k a ≤ 1 (a = 1, . . . , n). H. Mori [M] and Y. Ohnita [O] proved the conclusion of Theorem 1 ′ under the stronger conditions δ > n/(n + 1) and δ > 1/2, respectively. Our Theorem 1 ′ also gives a partial answer to the following Lawson–Simons’ conjecture:
Conjecture ([LS]). Let N n be a compact n-dimensional connected Rie- mannian manifold with the sectional curvature K satisfying
(6) 1/4 < K ≤ 1.
Then there exist no stable m-currents on N n for each m with 1 ≤ m ≤ n−1.
We are greatly indebted to P. F. Leung’s papers [L1, L2] which motivated
us to do this work.
2. Basic formulas and notations. In this paper, we shall make use of the following convention on the ranges of indices:
1 ≤ A, B, C, . . . ≤ n + p; 1 ≤ a, b, c, . . . ≤ n; n + 1 ≤ µ, ν, . . . ≤ n + p;
1 ≤ i, j, k . . . ≤ m; m + 1 ≤ α, β, γ . . . ≤ n.
Let M m and N n be Riemannian manifolds of dimension m and dimen- sion n, respectively. Let M m be an m-dimensional compact minimal sub- manifold of N n , n > m. For any normal variation vector field U = P
α u α e α of M m , the second variation of the volume is given by (see [S])
(7) I(U, U ) =
\
M m
h X
α,i
u 2 αi − X
α,β
(σ αβ + R αβ u α u β ) i dv, where u αi are the covariant derivatives of u α ,
σ αβ = X
i,j
h α ij h β ij , (8)
R αβ = X
i
R αiβi , (9)
and h α ij are the components of the second fundamental form h of M m in N n .
Now let x : N n → R n+p be an n-dimensional submanifold in the (n + p)- dimensional Euclidean space R n+p . We choose a local field of orthonor- mal frames e 1 , . . . , e n , e n+1 , . . . , e n+p in R n+p such that, restricted to N n , the vectors e 1 , . . . , e n are tangent to N n . Their dual coframe fields are ω 1 , . . . , ω n , ω n+1 , . . . , ω n+p . Then we have
dx = X
a
ω a e a , (10)
de a = X
b
ω ab e b + X
µ,b
B ab µ ω b e µ , (11)
de µ = − X
a,b
B ab µ ω b e a + X
ν
ω µν e ν , (12)
and the second fundamental form of N n in R n+p is
(13) B = X
a,b,µ
B ab µ ω a ⊗ ω b ⊗ e µ . The Gauss equation of N n in R n+p is
(14) n(n − 1)R = n 2 H 2 − S,
where R, H and S are the normalized scalar curvature, the mean curva-
ture and the length square of the second fundamental form of N n in R n+p ,
respectively.
3. An m-dimensional minimal submanifold in N n . Let M m be an m-dimensional minimal submanifold in N n , and N n be an n-dimensional submanifold in R n+p . In this case we can choose a local orthonormal ba- sis e 1 , . . . , e m , e m+1 , . . . , e n , e n+1 , . . . , e n+p in R n+p such that, restricted to M m , the vectors e 1 , . . . , e m are tangent to M m , e 1 , . . . , e n are tangent to N n , e n+1 , . . . , e n+p are normal to N n . Their dual coframe fields are ω 1 , . . . , ω m , ω m+1 , . . . , ω n , ω n+1 , . . . , ω n+p . From (10)–(12), restricted to M m , we have
dx = X
i
ω i e i , (15)
de i = X
j
ω ij e j + X
α,j
h α ij ω j e α + X
µ,j
B ij µ ω j e µ , (16)
de α = − X
i,j
h α ij ω i e j + X
β
ω αβ e β + X
µ,j
B αj µ ω j e µ , (17)
de µ = − X
i,j
B ij µ ω i e j − X
α,j
B αj µ ω j e α + X
ν
ω µν e ν , (18)
where h = P
i,j,α h α ij ω i ⊗ ω j ⊗ e α is the second fundamental form of M m in N n and P
i h α ii = 0 for any α, since M m is a minimal submanifold in N n . We choose the following normal variation vector field of M m in N n :
(19) U = X
α
u α e α , u α = hΛ, e α i, where Λ is a constant vector in R n+p .
Using (15)–(18), a straightforward computation shows u αi = − X
k
h α ki u k + X
µ
B αi µ u µ , (20)
X
α,i
u 2 αi = X
α,i
h X
j,k
h α ki h α ij u k u j + X
µ,ν
B αi µ B αi ν u µ u ν − 2 X
µ,k
h α ki B αi µ u k u µ i , (21)
where
(22) u j = hΛ, e j i, u µ = hΛ, e µ i.
Let E 1 , . . . , E n+p be a fixed orthonormal basis of R n+p , and U A = P
α hE A , e α ie α . Since (23)
n+p
X
A=1
hE A , vihE B , wi = hv, wi
for any vectors v, w in R n+p , putting (21) into (7) and using (22) and (23),
we obtain
trace(I) ≡
n+p
X
A=1
I(U A , U A ) (24)
= −
\
M m
h
− X
α,k,µ
(B αk µ ) 2 + X
α
R αα
i dv
= −
\
M m
X
α,k
h − X
µ
(B αk µ ) 2 + R αkαk i dv
= −
\
M m
h − X
α,µ,k
B αα µ B kk µ + 2 X
α,k
R αkαk i dv
=
\
M m
h 2 X
µ,α,k
(B αk µ ) 2 − X
µ,α,k
B αα µ B µ kk i dv.
Thus we obtain
Proposition 2. Let N n be an n-dimensional compact submanifold in R n+p . Let M m be an m-dimensional compact minimal submanifold of N n . If
(25) trace(I) =
\
M m
h 2 X
µ,α,k
(B αk µ ) 2 − X
µ,α,k
B αα µ B kk µ i
dv < 0,
then M m is not a stable minimal submanifold of N n .
4. The proof of Theorem 1. Let N n be an n-dimensional hypersur- face in R n+1 and M m be an m-dimensional compact minimal submanifold in N n . At a given point p ∈ M m in N n , we can choose a local orthonormal frame field e ∗ 1 , . . . , e ∗ n , ~n in R n+1 such that e ∗ 1 , . . . , e ∗ n are tangent to N n and at p ∈ M m ,
(26) B ab ∗ = hB(e ∗ a , e ∗ b ), ~ni = k a δ ab , 1 ≤ a, b ≤ n, where the k a are the principal curvatures of N n in R n+1 .
Since M m is an m-dimensional compact minimal submanifold in N n , at a given point p ∈ M m in N n , we can also choose a local orthonormal frame field e 1 , . . . , e m , e m+1 , . . . , e n in N n such that e 1 , . . . , e m are tangent to M m . Noting that e 1 , . . . , e n and e ∗ 1 , . . . , e ∗ n are two local orthonormal frame fields in a neighborhood of p ∈ M m , we can set
e i =
n
X
b=1
A b i e ∗ b , 1 ≤ i ≤ m, (27)
e α =
n
X
b=1
A b α e ∗ b , m + 1 ≤ α ≤ n,
(28)
where (A b a ) ∈ SO(n), i.e.
(29)
n
X
a=1
A a b A a c = δ bc ,
n
X
a=1
A b a A c a = δ bc .
It is a direct verification that at p ∈ M m , by use of (26)–(29) and (1), X
α,k
B αα B kk = X
α,k
hB(e α , e α ), B(e k , e k )i (30)
= X
α,k,a,b,c,d
A a α A b α A c k A d k hB(e ∗ a , e ∗ b ), B(e ∗ c , e ∗ d )i
= X
α,k,a,c
k a k c (A a α ) 2 (A c k ) 2
= X
a,c
R acac (A a α ) 2 (A c k ) 2
≤ X
a,c,α,k
(A a α ) 2 (A c k ) 2 = m(n − m),
where R acac = k a k c is the sectional curvature of N n . From (1), we also have
(31) −2 X
α,k
R αkαk < −2 · 1
2 m(n − m) = −m(n − m).
Putting (30) and (31) into (24), we obtain trace(I) < 0. From Proposi- tion 2, we infer that M m is not a stable minimal submanifold of N n .
5. The proof of Theorem 2. We first establish the following algebraic lemma in order to prove our Theorem 2:
Lemma 1. Let
1 ≤ a, b ≤ n; 1 ≤ i, j ≤ m; m + 1 ≤ α, β ≤ n, and consider the symmetric n × n matrix
T ij T iα T βj T βα
such that
(32)
m
X
i=1
T ii +
n
X
α=m+1
T αα = D,
n
X
a,b=1
T ab 2 = S.
Then:
(1) If m = 1 or m = n − 1, we have
(33) X
i
T ii 2
− D X
i
T ii + 2 X
i,α
(T iα ) 2 ≤ S + n − 5
2 D 2 .
(2) If 2 ≤ m ≤ n − 2, we have (34) X
i
T ii 2
− D X
i
T ii + 2 X
i,α
(T iα ) 2
≤ m(n − m)
n S + |(2m − n)D|
n 2 pm(n − m)(Sn − D 2 ) − 2m(n − m)D 2
n 2 .
P r o o f. We apply the Lagrange multiplier method to the problem (cf.
P. F. Leung [L1, L2])
(35) X
i
X ii 2
− D X
i
X ii + 2 X
i,α
(X iα ) 2 = max!
subject to the constraints
(36) X
i
X ii + X
α
X αα = D and
(37) X
i
(X ii ) 2 + X
α
(X αα ) 2 +2 X
i<j
(X ij ) 2 +2 X
α<β
(X αβ ) 2 +2 X
i,α
(X iα ) 2 = S, where S = P
a,b (T ab ) 2 and the X ab form a symmetric n × n matrix
X ij X iα X βj X βα
. We consider the function
f = X
i
X ii 2
− D X
i
X ii + 2 X
i,α
(X iα ) 2 + λ X
i
X ii + X
α
X αα − D
+ µ h X
i
(X ii ) 2 + X
α
(X αα ) 2 + 2 X
i<j
(X ij ) 2 + 2 X
α<β
(X αβ ) 2 + 2 X
i,α
(X iα ) 2 − S i , where λ, µ are the Lagrange multipliers.
Differentiating with respect to each variable and equating to zero, we obtain
2 X
j
X jj − D + λ + 2µX ii = 0, (38)
λ + 2µX αα = 0, (39)
4X iα + 4µX iα = 0, (40)
4µX ij = 0, i < j, (41)
4µX αβ = 0, α < β.
(42)
Hence (with the numbers standing for the corresponding left hand sides) X
i
X ii (38) + X
α
X αα (39) + X
i,α
X iα (40) + X
i<j
X ij (41) + X
α<β
X αβ (42) = 0 gives
(43) 2 X
i
X ii
2
− D X
i
X ii + 4 X
i,α
(X iα ) 2 = −(λD + 2µS).
(1) C a s e µ = 0. It is easy to see in this case
(44) X
i
X ii 2
− D X
i
X ii + 2 X
i,α
(X iα ) 2 = − D 2 4 .
(2) C a s e µ = −1. First we suppose m(n − m) > n, and putting X αα = λ/2, P
i X ii = D − (n − m)λ/2 into (38), we have λ = (m − 2)D
m(n − m) − n , X ii = (n − m − 2)D 2[m(n − m) − n] , (45)
X αα = (m − 2)D 2[m(n − m) − n] , and
(46) X
i
X ii
2
− D X
i
X ii + 2 X
i,α
(X iα ) 2 = S − m(n − m) − 4 4[m(n − m) − n] D 2 is another critical value.
Now suppose m(n − m) = n, i.e. n = 4, m = 2. If µ = −1, then X ii = 1
2 (D − λ), X αα = λ 2 , (47)
X
i
X ii
2
− D X
i
X ii + 2 X
i,α
(X iα ) 2 = S − D 2 2 , (48)
that is, equality holds in (34) in this case.
(3) C a s e µ 6= 0, −1. Let X = P
i X ii . Then X αα = − λ
2µ , 2µ(X − D) = (n − m)λ, (49)
λ = D − 2
1 + µ
m
X.
(50)
Substituting (50) into the second formula of (49), we get (51) µ = m(n − m)(D − 2X)
2(nX − mD) , λ
µ = 2
n − m (X − D).
From (43), we have
(52) X(D − 2X)
µ = λ
µ D + 2S.
Putting (51) into (52), we get X 2 − 2mD
n X − m(n − m)
n S − m
n D 2
= 0, that is,
(53) X = m
n D ± s
m(n − m) n
S − D 2 n
. The critical value is
(54) X
i
X ii
2
− D X
i
X ii + 2 X
i,α
(X iα ) 2
= m(n − m)
n S + |(2m − n)D|
n 2 pm(n − m)(Sn − D 2 ) − 2m(n − m)D 2
n 2 .
Hence, the critical values are
− D 2
4 , S − m(n − m) − 4 4[m(n − m) − n] D 2 , m(n − m)
n S + |(2m − n)D|
n 2 pm(n − m)(Sn − D 2 ) − 2m(n − m)D 2
n 2 .
It can be verified directly by calculation that if m = 1 or m = n − 1, then m(n − m) = n − 1 and the maximum is S + n−5 4 D 2 ; if 2 ≤ m ≤ n − 2, the maximum is (cf. [L1])
m(n − m)
n S + |(2m − n)D|
n 2 pm(n − m)(Sn − D 2 ) − 2m(n − m)D 2
n 2 .
This completes the proof of Lemma 1.
Proposition 3. Let N n be an n-dimensional (n ≥ 4) compact subman- ifold in R n+p . Let S be the length square of the second fundamental form.
If
(55) S < 2nH 2 − |(2m − n)H|
r n
m(n − m) (S H − nH 2 ),
then there exist no stable m-dimensional minimal submanifolds of N n for each m with 2 ≤ m ≤ n − 2, where S H is the length square of the second fundamental form in the direction of the mean curvature vector of N n .
P r o o f. We choose a local orthonormal frame field e 1 , . . . , e n+p in R n+p
with e 1 , . . . , e n tangent to N n and e n+1 , . . . , e n+p normal to N n . Let e n+1
be parallel to the mean curvature vector − → H and
(56) B(X, Y ) =
n+p
X
µ=n+1
B µ (X, Y )e µ , then
(57) X
a
B n+1 (e a , e a ) = nH, X
a
B µ (e a , e a ) = 0, n + 2 ≤ µ ≤ n + p.
Moreover,
(58) X
i,α
[2kB(e i , e α )k 2 − hB(e i , e i ), B(e α , e α )i]
= X
i
B n+1 (e i , e i ) 2
+ 2 X
i,α
(B n+1 (e i , e α )) 2 − nH X
i
B n+1 (e i , e i )
+
n+p
X
µ=n+2
h X
i
B µ (e i , e i ) 2
+ 2 X
i,α
(B µ (e i , e α )) 2 i .
For each symmetric n ×n-matrix (B n+1 (e a , e b )) and (B µ (e a , e b )), 1 ≤ a, b ≤ n, n + 1 ≤ µ ≤ n + p, applying Lemma 1, we have
(59) X
i
B n+1 (e i , e i ) 2
+ 2 X
i,α
(B n+1 (e i , e α )) 2 − nH X
i
B n+1 (e i , e i )
≤ m(n − m)
n S H + |(2m − n)H|
r m(n − m)
n (S H − nH 2 ) − 2m(n − m)H 2 and
(60) X
i
B µ (e i , e i ) 2
+ 2 X
i,α
(B µ (e i , e α )) 2 ≤ m(n − m) n
X
a,b
(B µ (e a , e b )) 2 . Combining (58), (59) with (60), from assumption (55) we get
(61) X
i,α
[2kB(e i , e α )k 2 − hB(e i , e i ), B(e α , e α )i]
≤ m(n − m)
n S − 2m(n − m)H 2 + |(2m − n)H|
r m(n − m)
n (S H − nH 2 ) < 0.
This completes the proof of Proposition 3.
P r o o f o f T h e o r e m 2. Let N n be an n-dimensional (n ≥ 4) compact submanifold in R n+p . By the Gauss equation (14) and the fact that S ≥ nH 2 , we know that condition (2) is equivalent to
(62) S < n 2 H 2
n − 1 .
But (62) is equivalent to (63) p
S − nH 2 <
r n
n − 1 |H| = 1 2
r n
n − 1 n|H| − 1
2 (n − 2)
r n
n − 1 |H|.
Now (63) is equivalent to (64)
p S − nH 2 + 1
2 (n − 2)
r n
n − 1 |H|
2
< 1 2
r n
n − 1 n|H|
2 , that is,
(65) S < 2nH 2 − (n − 2)
r n
n − 1 |H| p
S − nH 2 .
Since |2m−n|pn/(m(n − m)) ≤ (n−2)pn/(n − 1) and S H ≤ S, we see that (65) implies (55) for each m with 2 ≤ m ≤ n−2. Therefore, Theorem 2 follows from Proposition 3 directly.
6. The proof of Corollary 1 and Proposition 1
P r o o f o f C o r o l l a r y 1. Let N n be an n-dimensional compact hy- persurface in R n+1 and let the principal curvatures be k a , 1 ≤ a ≤ n. By assumption (3), we have
(66) S = X
i
k 2 i < n 2 H 2 n − 1 .
By the Gauss equation (14) and the fact S ≥ nH 2 , (66) is equivalent to (2). Now Corollary 1 follows from Theorem 2 directly.
P r o o f o f P r o p o s i t i o n 1. Let N n be the following n-dimensional (n ≥ 4) ellipsoid in R n+1 :
N n : x 2 1
a 2 1 + . . . + x 2 n+1
a 2 n+1 = 1, 0 < a 1 ≤ a 2 ≤ . . . ≤ a n+1 .
It is not difficult to verify by a direct computation that the maximum and minimum of the principal curvatures are
k max = a n+1
a 2 1 , k min = a 1
a 2 n+1 , respectively.
(1) If 1 ≤ a n+1 < √ 3
2 and a 1 ≥ √ a n+1 , then the sectional curvature K of N n satisfies
1 2 < a 2 1
a 4 n+1 = k min 2 ≤ K ≤ k 2 max = a 2 n+1 a 4 1 ≤ 1.
Thus the conclusion of Proposition 1 follows from Theorem 1.
(2) If a n+1 /a 1 < pn/(n − 1), then 6 k a −
s 1
n(n − 1)
n
X
b=1
k b ≤ a n+1 a 2 1 −
r n
n − 1 a 1
a 2 n+1 < 0.
Thus the conclusion of Proposition 1 follows from Corollary 1.
7. Some remarks. Let N n be an n-dimensional compact submanifold in an (n + p)-dimensional unit sphere S n+p and B the second fundamental form of N n . By a reduction as in the proof of (24) (cf. (2.11) of Pan–Shen [PS]) we have
trace(I) = −
\
M m
h
− X
α,k,µ
(B αk µ ) 2 + X
α
R αα
i dv (67)
=
\