98 Submanifolds and Holonomy
3.6.9), which span the first normal space by Exercise 3.6.11. Then n
1
and n
2
are
linearly independent and locally there exists a parallel unit normal vector field
ξ
such that n
1
,
ξ
= n
2
,
ξ
. Therefore A
ξ
is a constant multiple of the identity, that
is,
ξ
is an umbilical section of
ν
M.ThenM contained in a sphere and so it is an
isoparametric hypersurface of a sphere with two distinct principal curvatures. Each
one-dimensional eigendistribution E
1
,E
2
of the shape operator of M,regardedasa
hypersurface of the sphere, is an autoparallel distribution. In fact, this follows from
(2.14) in the proof of Theorem 2.9.4. Then E
1
and E
2
= E
⊥
1
are autoparallel, which
implies that E
1
and E
2
are parallel distributions. Moreover,
α
(E
1
,E
2
)=0, where
α
is the second fundamental form of M as a submanifold of the Euclidean space. Then
we can apply Lemma 1.7.1 to conclude that M is an extrinsic product of circles.
If Φ
∗
= SO
2
,thenΦ
∗
p
is transitive on the unit sphere in
ν
p
M for all p ∈ M.
This implies that there exist constants
¯
H
k
such that H
k
(
ξ
)=
¯
H
k
, k = 1,2, for all unit
vectors
ξ
∈
ν
p
M. In particular,
¯
H
1
= H
1
(
ξ
)=H,
ξ
= 0for
ξ
orthogonal to H.
Thus H = 0, that is, M is a minimal submanifold. Moreover, as a ref ormulation of
the condition on H
2
, for any normal vectors
ξ
and
η
we have A
ξ
,A
η
= tr(A
ξ
A
η
)=
μ
2
ξ
,
η
for some
μ
≥0. Now, either M is totally geodesic or
μ
> 0. In the latter case
each shape operator A
ξ
with respect to a unit normal vector field
ξ
has two distinct
eigenvalues ±
μ
. We can then choose local orthonormal frame fields e
1
,e
2
of TM and
ξ
1
,
ξ
2
of
ν
M such that A
ξ
1
is represented by the matrix
μ
0
0 −
μ
. Suppose that A
ξ
2
is represented by the matrix
bd
d −b
.SinceA
ξ
1
,A
ξ
2
= 0wegetb = 0, and since
A
ξ
1
,A
ξ
1
= A
ξ
2
,A
ξ
2
we get d = ±
μ
. Without loss of generality we may assume
that d =
μ
,sothatA
ξ
2
has the form
0
μ
μ
0
. In particular, from the equations of
Gauss and Ricci we get that the sectional curvature K of M is equal to K =
κ
−2
μ
2
,
while the normal curvature K
⊥
= R
⊥
(e
1
,e
2
)
ξ
1
,
ξ
2
satisfies K
⊥
= 2
μ
2
. Next, using
the Codazzi equation we see that 0 = Δlog
μ
= 2K −K
⊥
,whereΔ is the L aplace-
Beltrami operator on M acting o n functions by
Δ f =
∑
i
∇
2
e
i
e
i
f =
∑
i
d
2
f (e
i
,e
i
) −
∑
i
df(∇
e
i
e
i
)
(this is left as an exercise, cf. also [83, formula 3.5]). So 2
μ
2
= 2
κ
−4
μ
2
,thatis,
κ
=
3
μ
2
> 0. Hence M has the same second fundamental form as the Veronese surface
S
2
(
κ
/
√
3) → S
4
(
κ
) (cf. Section 2.4). We now apply Theorem 2.10.2, which shows
that M coincides locally with the Veronese surface S
2
(
κ
√
3
) ⊂ S
4
(
κ
).
The case k = 3.
If M is minimal, then the first normal space has dimension two, namely the d im-
ension of the space of traceless 2 ×2-symmetric matrices. By assumption it must be
equal to the codimension. It follows that M cannot be a minimal submanifold. More-
over,
ξ
1
=
H
H
is a global parallel unit normal vector field o n M and A
ξ
1
commutes
with all shape operators by the Ricci equation. If A
ξ
1
has two distinct eigenvalues,
then all shape operators are simultaneously diagonalizable and M is isoparametric,