This paper advances the local classification of pseudo-Riemannian manifolds with parallel Weyl tensor, focusing on those that are neither conformally flat nor locally symmetric, completing a key step in understanding their structure.
Contribution
It provides a comprehensive local classification of conformally symmetric manifolds that are not conformally flat or locally symmetric.
Findings
01
Classification of such manifolds completed
02
Identification of key geometric properties
03
Extension of previous classification results
Abstract
This is a final step in a local classification of pseudo-Riemannian manifolds with parallel Weyl tensor that are not conformally flat or locally symmetric.
Equations24
R(u,v)ψ=∇v∇uψ−∇u∇vψ+∇[u,v]ψ
R(u,v)ψ=∇v∇uψ−∇u∇vψ+∇[u,v]ψ
W=R−(n−2)−1g∧σ.
W=R−(n−2)−1g∧σ.
xtss=xsst+R(xt,xs)xs.
xtss=xsst+R(xt,xs)xs.
u′
u′
TxM
TxM
(T∗Σ×V,hD−2τ+γ−θρD),
(T∗Σ×V,hD−2τ+γ−θρD),
(I×R×V,κdt2+dtds+γ),
(I×R×V,κdt2+dtds+γ),
R(u′,v)v′=[fg(v,v′)+⟨Av,v′⟩]g(u′,u)u
R(u′,v)v′=[fg(v,v′)+⟨Av,v′⟩]g(u′,u)u
i)R(⋅,⋅)u=Ω⊗uor, in coordinates,ii)ulRjkls=Ωjkus,
i)R(⋅,⋅)u=Ω⊗uor, in coordinates,ii)ulRjkls=Ωjkus,
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TopicsGeometric Analysis and Curvature Flows · Geometry and complex manifolds · Advanced Differential Geometry Research
Full text
The local structure of
conformally
symmetric manifolds
Andrzej Derdzinski
and
Witold Roter
Department of Mathematics The Ohio State University Columbus, OH 43210 USA
This is a final step in a local classification of pseudo -Riemannian manifolds
with parallel Weyl tensor that are not conformally flat or locally
symmetric.
The present paper provides a finishing touch in a local classification of
essentially conformally symmetric pseudo -Riemannian metrics.
A pseudo -Riemannian manifold of dimension n≥4 is called essentially conformally
symmetric if it is conformally symmetric [2]
(in the sense that its Weyl conformal tensor is parallel) without being
conformally flat or locally symmetric.
The metric of an essentially conformally symmetric manifold is always indefinite
[4, Theorem 2]. Compact essentially conformally symmetric manifolds are
known to exist in all dimensions n≥5 with n≡5(mod 3), where they
represent all indefinite metric signatures [8], while
examples of essentially conformally symmetric pseudo -Riemannian metrics on open manifolds of all dimensions n≥4 were
first constructed in [16].
On every conformally symmetric manifold there is a naturally distinguished parallel distribution
D, of some dimension d, which we call the Olszak
distribution. As shown by Olszak [13], for an essentially conformally symmetric manifold d∈{1,2}.
In [7] we described the local structure of all conformally symmetric manifolds with d=2. See also Section 3. This paper establishes an
analogous result (Theorem 4.1) for the case d=1.
In both cases, some of the metrics in question are locally symmetric. In
Remark 4.2 we explain why a similar classification result cannot be
valid just for essentially conformally symmetric manifolds.
Essentially conformally symmetric manifolds with d=1 are all
Ricci-recurrent, in the sense that, for every tangent vector field v,
the Ricci tensor ρ and the covariant derivative ∇vρ
are linearly dependent at each point. The local structure of essentially conformally symmetric Ricci-recurrent manifolds at
points with ρ⊗∇ρ=0 has already been
determined by the second author [16]. Our new contribution settles the
one case still left open in the local classification problem, namely,
that of essentially conformally symmetric manifolds with d=1 at points where
ρ⊗∇ρ=0.
The literature dealing with conformally symmetric manifolds includes, among others,
[9, 10, 12, 15, 17, 18] and the papers cited
above. A local classification of homogeneous essentially conformally symmetric manifolds can be found in
[3].
1. Preliminaries
Throughout this paper, all manifolds and bundles, along with sections and
connections, are assumed to be of class C∞. A manifold is,
by definition, connected. Unless stated otherwise, a mapping is always a
C∞ mapping betweeen manifolds.
Given a connection ∇ in a vector bundle E over a manifold M,
a section ψ of E, and vector fields u,v tangent to M,
we use the sign convention
[TABLE]
for the curvature tensor R=R∇.
The Levi-Civita connection of a given pseudo -Riemannian manifold (M,g) is always denoted by ∇.
We also use the symbol ∇ for connections induced by ∇,
in various ∇-parallel subbundles of TM and their quotients.
The Schouten tensor σ and Weyl conformal tensor W of a pseudo -Riemannian manifold (M,g) of dimension n≥4 are given by
σ=ρ−(2n−2)−1sg, with ρ
denoting the Ricci tensor,
s=trgρ standing for the
scalar curvature, and
[TABLE]
Here ∧ is the exterior multiplication of 1-forms valued in
1-forms, which uses the ordinary ∧ as the valuewise
multiplication; thus, g∧σ is a 2-form valued in
2-forms.
Let (t,s)↦x(s,t) be a fixed variation of curves in a pseudo -Riemannian manifold (M,g), that is, an M-valued C∞ mapping from a rectangle
(product of intervals) in the ts-plane. By a vector field w
along the variation we mean, as usual, a section of the pullback of
TM to the rectangle (so that w(t,s)∈Tx(t,s)M). Examples are xs
and xt, which assign to (t,s) the velocity of the curve
t↦x(t,s) or s↦x(t,s) at s or t. Further
examples are provided by restrictions to the variation of vector fields on
M. The partial covariant derivatives of a vector field w along the
variation are the vector fields wt,ws along the variation, obtained
by differentiating w covariantly along the curves t↦x(t,s)
or s↦x(t,s). Skipping parentheses, we write wts,wstt,
etc., rather than (wt)s,((ws)t)t for higher-order
derivatives, as well as xss,xst instead of
(xs)s,(xs)t. One always has wts=wst+R(xt,xs)w,
cf. [11, formula (5.29) on p. 460], and, since the
Levi-Civita connection ∇ is torsionfree, xst=xts. Thus, whenever
(t,s)↦x(s,t) is a variation of curves in M,
[TABLE]
2. The Olszak distribution
The Olszak distribution of a conformally symmetric manifold (M,g) is the parallel
subbundle D of TM, the sections of which are the vector
fields u with the property that ξ∧Ω=0 for all
vector fields v,v′ and for the differential forms
ξ=g(u,⋅) and
Ω=W(v,v′,⋅,⋅). The distribution
D was introduced, in a more general situation, by Olszak
[13], who also proved the following lemma.
Lemma 2.1**.**
The following conclusions hold for the dimension
d of the Olszak distribution D in any conformally symmetric manifold
(M,g) with dimM=n≥4.
(i)
d∈{0,1,2,n}, and d=n if and only if (M,g) is
conformally flat.
2. (ii)
d∈{1,2}* if (M,g) is essentially conformally symmetric.*
3. (iii)
d=2* if and only if rankW=1, in the sense that W, as an
operator acting on exterior 2-forms, has rank 1 at each point.*
4. (iv)
If d=2, the distribution D is spanned by all vector fields of
the form W(u,v)v′ for arbitrary vector fields u,v,v′ on M.
Proof..
See Appendix I.
∎
In the next lemma, parts (a) and (d) are due to Olszak
[13, 2o and 3o on p. 214].
Lemma 2.2**.**
If d∈{1,2}, where d is
the dimension of the Olszak distribution D of a given conformally symmetric manifold (M,g) with dimM=n≥4, then
(a)
D* is a null parallel distribution,*
2. (b)
at any x∈M the space Dx contains the image of the
Ricci tensor ρx treated, with the aid of gx, as an
endomorphism of TxM,
3. (c)
the scalar curvature is identically zero and
R=W+(n−2)−1g∧ρ,
4. (d)
W(u,⋅,⋅,⋅)=0* whenever u
is a section of D,*
5. (e)
R(v,v′,⋅,⋅)=W(v,v′,⋅,⋅)=0* for any sections
v and v′ of D⊥,*
6. (f)
of the connections in D and E=D⊥/D, induced by
the Levi-Civita connection of g, the latter is always flat, and the former is flat if
d=1.
Proof..
Assertion (e) for W is immediate from the definition of
D. Namely, at any point x∈M, every 2-form
Ωx in the image of Wx (for Wx acting on
2-forms at x) is ∧-divisible by
ξ=gx(u,⋅) for each
u∈Dx∖{0}, and so
Ωx(v,v′)=0 if v,v′∈Dx⊥.
We now proceed to prove (a), (b), (c) and (d).
First, let d=2. By Lemma 2.1(iii), this amounts to the condition
rankW=1, so that (a), (b) and (c) follow from Lemma 2.1(iv) combined
with [7, Lemma 17.1(ii) and Lemma 17.2]. Also, for a
nonzero 2-form Ωx chosen as in the last paragraph,
Dx is the image of Ωx, that is, Ωx
equals the exterior product of two vectors in Dx (treated as
1-forms, with the aid of gx). Now (d) follows since, by (a),
Ωx(ux,⋅)=0 if u is a section of D.
Next, suppose that d=1. Replacing M by a neighborhood of any given
point, we may assume that D is spanned by a vector field u. If
u were not null, we would have W(u,v,u,v′)=0 for any
sections v,v′ of D⊥, as one sees contracting the
twice-covariant tensor field W(⋅,v,⋅,v′)=0, at
any point x, in an orthogonal basis containing the vector ux. (We
have already established (e) for W.) Combined with (e) for W
and the symmetries of W, the relation W(u,v,u,v′)=0 for
v,v′ in D⊥ would then give W=0, contrary to the assumption
that d=1. Thus, u is null, which yields (a). Now
[TABLE]
For any section v of D⊥ one sees that
W(u,⋅,u′,v)=0 by contracting the tensor field
W(⋅,⋅,⋅,v)=0 in the first and third arguments,
at any point x, in
[TABLE]
and using (e) for W, along with the inclusion D⊂D⊥,
cf. (a). Since u′ and D⊥ span TM, assertion (e) for W
thus implies (d).
To prove (b) and (c) when d=1, we distinguish two cases: (M,g) is
either essentially conformally symmetric, or locally symmetric. For (c), it suffices to establish vanishing
of the scalar curvature s (cf. (2)). Now, in
the former case, s=0 according to
[5, Theorem 7], while (b) follows since, as shown in
[6, Theorem 7 on p. 18], for arbitrary vector fields
v,v′ and v′′ on an essentially conformally symmetric pseudo -Riemannian manifold, ξ∧Ω=0,
where ξ=ρ(v,⋅) and
Ω=W(v′,v′′,⋅,⋅). In the case
where g is locally symmetric, (b) and (c) are established in Appendix II.
Assertion (e) for R is now obvious from (e) for W and (c), since,
by (b), ρ(v,⋅)=0 for any section v of D⊥. The
claim about E in (f) is in turn immediate from (1) and (e)
for R, which states that R(w,w′)v, for arbitrary vector
fields w,w′ and any section v of D⊥, is orthogonal to all
sections of D⊥ (and hence must be a section of D). Finally, to
prove (f) for D, with d=1, let us fix a section u of
D, a vector field v, and define a differential 2-form ζ by
ζ(w,w′)=(n−2)R(w,w′,u,v) for any vector fields
w,w′. By (c) and (e),
ζ=g(u,⋅)∧ρ(v,⋅), as D⊂D⊥ (cf. (a)), and so ρ(u,⋅)=0 in view of (b) and symmetry of ρ.
However, by (b), both g(u,⋅) and ρ(v,⋅) are
sections of the subbundle of T∗M corresponding to D under the
bundle isomorphism TM→T∗M induced by g, so that ζ=0
since the distribution D is one-dimensional.
∎
3. The case d=2
For more details of the construction described below, we refer the reader
to [7].
Let there be given a surface Σ, a projectively flat torsionfree connection D on Σ
with a D -parallel area form α, an integer
n≥4, a sign factor ε=±1, a real vector space V of dimension
n−4, and a pseudo -Euclidean inner product ⟨,⟩
on V.
We also assume the existence of a twice-contravariant symmetric
tensor field T on Σ with
divD(divDT)+(ρD,T)=ε (in coordinates:
Tjk,jk+TjkRjk=ε). Here
divD denotes the
D -divergence, ρD is the Ricci tensor of D , and (,) stands for the
obvious pairing. Such T always exists locally in Σ. In fact,
according to [7, Theorem 10.2(i)] combined with
[7, Lemma 11.2], T exists whenever Σ is
simply connected and noncompact.
For T chosen as above, we define a twice-covariant symmetric
tensor field τ on Σ, that is, a section of
[T∗Σ]⊙2, by requiring τ to correspond to the section
T of [TΣ]⊙2 under the vector-bundle isomorphism
TΣ→T∗Σ which acts on vector fields v by
v↦α(v,⋅). In coordinates,
τjk=αjlαkmTlm.
Next, we denote by hD the Patterson -Walker
Riemann extension metric [14] on the total space T∗Σ,
obtained by requiring that all vertical and all
D -horizontal vectors be
hD-null, while
hxD(ζ,w)=ζ(dπxw) for x∈T∗Σ, any vector
w∈TxT∗Σ, any vertical vector
ζ∈Kerdπx=Tπ(x)∗Σ, and the bundle projection π:T∗Σ→Σ.
Finally, let γ and θ be the constant pseudo -Riemannian metric on V
corresponding to the inner product ⟨,⟩, and the function
V→R with θ(v)=⟨v,v⟩.
Our Σ,D,α,n,ε,V,⟨,⟩ now give rise to the
pseudo -Riemannian manifold
[TABLE]
of dimension n, with the metric
hD−2τ+γ−θρD,
where the function θ and covariant tensor fields
τ,ρD,hD,γ on
Σ,T∗Σ or V are identified with their pullbacks to
T∗Σ×V. (Thus, for instance,
hD−2τ+γ is a product metric.)
We have the following local classification result, in which d stands
for the dimension of Olszak distribution D.
Theorem 3.1**.**
The pseudo -Riemannian manifold (6) obtained as above from
any data Σ,D,α,n,ε,V,⟨,⟩ with the stated
properties is conformally symmetric and has d=2. Conversely, in any conformally symmetric pseudo -Riemannian manifold such
that d=2, every point has a connected neighborhood isometric to an open
subset of a manifold (6) constructed above from some data
Σ,D,α,n,ε,V,⟨,⟩.
The manifold (6) is never conformally flat, and it
is locally symmetric if and only if the Ricci tensor ρD is
D -parallel.
Proof..
See [7, Section 22]. Note that, in view of
Lemma 2.1(iii), the condition rankW=1 used in
[7] is equivalent to d=2.
∎
The objects Σ,D,α,n,ε,V,⟨,⟩ are treated
as parameters of the above construction, while T is merely assumed to
exist, even though the metric g in (6) clearly depends on
τ (and hence on T). This is justified by the fact that, with
fixed Σ,D,α,n,ε,V,⟨,⟩, the metrics
corresponding to two choices of T are, locally, isometric to each
other, cf. [7, Remark 22.1].
The metric signature of (6) is clearly given by
−−…++, with the dots standing for the sign pattern of
⟨,⟩.
4. The case d=1
Let there be given an open interval I, a C∞ function
f:I→R, an integer n≥4, a real vector space V of dimension
n−2 with a pseudo -Euclidean inner product ⟨,⟩, and a
nonzero traceless linear operator A:V→V, self-adjoint relative
to ⟨,⟩. As in [16], we then define an n-dimensional pseudo -Riemannian manifold
[TABLE]
where products of differentials represent symmetric products, t,s denote
the Cartesian coordinates on the I×R factor, γ stands for
the pullback to I×R×V of the flat pseudo -Riemannian metric on V that
corresponds to the inner product ⟨,⟩, and the function
κ:I×R×V→R is given by
κ(t,s,ψ)=f(t)⟨ψ,ψ⟩+⟨Aψ,ψ⟩.
The manifolds (7) are characterized by the following local
classification result, analogous to Theorem 3.1. As before,
d is the dimension of the Olszak distribution.
Theorem 4.1**.**
For any I,f,n,V,⟨,⟩,A as above,
the pseudo -Riemannian manifold (7) is conformally symmetric and has d=1. Conversely, in
any conformally symmetric pseudo -Riemannian manifold such that d=1, every point has a connected neighborhood
isometric to an open subset of a manifold (7) constructed from
some such I,f,n,V,⟨,⟩,A.
The manifold (7) is never conformally flat, and it
is locally symmetric if and only if f is constant.
A proof of Theorem 4.1 is given at the end of the next section.
Obviously, the metric κdt2+dtds+γ in (7)
has the sign pattern −…+, where the dots stand for the
sign pattern of ⟨,⟩.
Remark 4.2**.**
A classification result of the same format as
Theorem 4.1 cannot be true just for essentially
conformally symmetric manifolds with d=1. Namely, such manifolds do not
satisfy a principle of unique continuation: formula (7) with
f which is nonconstant on I, but constant on some nonempty
open subinterval I′ of I, defines an essentially conformally symmetric manifold with a locally
symmetric open submanifold U=I′×R×V. At
points of U, the local structure of (7) does not, therefore,
arise from a construction that, locally, produces all essentially conformally symmetric manifolds and nothing
else.
As explained in [7, Section 24], an analogous
situation arises when d=2.
The following assumptions will be used in Lemma 5.1.
(a)
(M,g) is a conformally symmetric manifold of dimension n≥4 and y∈M.
2. (b)
The Olszak distribution D of (M,g) is one-dimensional.
3. (c)
u is a global parallel vector field spanning D.
4. (d)
t:M→R is a C∞ function with g(u,⋅)=dt
and t(y)=0.
5. (e)
dimV=n−2 for the space V of all parallel sections of
E=D⊥/D.
6. (f)
ρ=(2−n)f(t)dt⊗dt for some C∞ function
f:I′→R on an open interval I′, where ρ
is the Ricci tensor and f(t) denotes the composite
f∘t.
For local considerations, only (a) and (b) are essential. In fact, condition
(e) (in which ‘parallel’ refers to the connection in E induced by the
Levi-Civita connection of g), as well (c) and (d) for some u and t, follow from
(a) – (b) if M is simply connected. See Lemma 2.2(f). On the
other hand, (c) – (d), Lemma 2.2(b) and symmetry of ρ give
∇dt=0 and ρ=χdt⊗dt for some function
χ:M→R, so that
∇ρ=dχ⊗dt⊗dt. However, ∇ρ
is totally symmetric (that is, ρ satisfies the Codazzi equation):
our assumption ∇W=0 implies the condition
divW=0, well known
[11, formula (5.29) on p. 460] to be equivalent to
the Codazzi equation for the Schouten tensor σ, while
σ=ρ by Lemma 2.2(c). Thus, dχ equals
a function times dt, and so χ is, locally, a function of t,
which (locally) yields (f).
For any section v of D⊥, we denote by v the image of
v under the quotient-projection morphism
D⊥→E=D⊥/D.
The data required for the construction in Section 4 consist of
I,f,n,V appearing in (a) – (f), along with the
pseudo -Euclidean inner product ⟨,⟩ in V,
induced in an obvious way by g (cf. Lemma 2.2(f)), and
A:V→V characterized by
⟨Aψ,ψ′⟩=W(u′,v,v′,u′), for ψ,ψ′∈V, with a
vector field u′ and sections v,v′ of D⊥ chosen, locally,
so that g(u,u′)=1, ψ=v and ψ′=v′. (The
resulting bilinear form
(ψ,ψ′)↦⟨Aψ,ψ′⟩ on V is
well-defined, that is, unaffected by the choices of u′,v or
v′, as a consequence of Lemma 2.2(d), (e), while the
function W(u′,v,v′,u′) is in fact constant, by
Lemma 2.2(d), as ones sees differentiating it via the Leibniz rule
and noting that, since v and v′ are parallel, the covariant
derivatives of v and v′ in the direction of any vector field are
sections of D.) That A is traceless and self-adjoint is
immediate from the symmetries of W. Finally, A=0 since,
otherwise, W would vanish. (Namely, in view of
Lemma 2.2(d), (e), W would yield 0 when evaluated on any quadruple of vector fields,
each of which is either u′ or a section of D⊥.)
Under the assumptions (a) – (f), with f=f(t), we then have
[TABLE]
for any sections v,v′ of D⊥ and any vector field u′.
In fact, ρ(v,⋅)=ρ(v′,⋅)=0 from symmetry
of ρ and Lemma 2.2(b), so that, by Lemma 2.2(c),
R(u′,v)v′=W(u′,v)v′−(n−2)−1g(v,v′)ρu′, where ρu′ denotes the unique
vector field with g(ρu′,⋅)=ρ(u′,⋅).
Now (8) follows: due to (d), (f) and the definition of A,
both sides have the same g-inner product with u′, and are
orthogonal to u⊥=D⊥ (with R(u′,v)v′ orthogonal
to D⊥ in view of Lemma 2.2(e)).
We fix an open subinterval I of I′, containing 0, and a
null geodesic I∋t↦x(t) in M with x(0)=y,
parametrized by the function t (in the sense that the function t
restricted to the geodesic coincides with the geodesic parameter). Namely,
since ∇dt=0, the restriction of t to any geodesic is an affine
function of the parameter; thus, by (d), it suffices to prescribe the initial
data formed by x(0)=y and a null vector x˙(0)∈TyM with
g(x˙(0),uy)=1.
As g(x˙(0),uy)=1, the plane P in TyM, spanned
by the null vectors x˙(0) and uy (cf. Lemma 2.2(a)) is
gy-nondegenerate, and so TyM=P⊕V, for
V=P⊥. Let
pr:TyM→V be the orthogonal projection.
Since pr(Dy)={0}, the restriction of
pr to Dy⊥ descends to the quotient
Ey=Dy⊥/Dy, producing an isomorphism
Ey→V, also denoted by pr .
Finally, for ψ∈V, we let t↦ψ~(t)∈Tx(t)M
be the parallel field with
ψ~(0)=prψy, and set
κ(t,s,ψ)=f(t)⟨ψ,ψ⟩+⟨Aψ,ψ⟩, as in
Section 4.
The formula F(t,s,ψ)=expx(t)(ψ~(t)+sux(t)/2) now
defines a C∞ mapping F from an open subset of
R2×V into M.
Lemma 5.1**.**
Under the above hypotheses,
F∗g=κdt2+dtds+h.
Proof..
The F-images w,w′,F∗ψ of the constant
vector fields (1,0,0),(0,1,0) and (0,0,ψ) in
R2×V, for ψ∈V, are vector fields tangent to
M along F (sections of F∗TM). Since D⊥ is parallel,
its leaves are totally geodesic and, by Lemma 2.2(e), the Levi-Civita connection of
g induces on each leaf a flat torsionfree connection. Thus,
w′ and each F∗ψ are parallel along each leaf of D⊥, as
well as tangent to the leaf, and parallel along the geodesic
t↦x(t). Therefore, w′=u/2, while the
functions g(w′,F∗ψ) and g(F∗ψ,F∗ψ′), for
ψ,ψ′∈V, are constant, and hence equal to their values at
y, that is, 0 and ⟨ψ,ψ′⟩. It now remains to be
shown that g(w,w)=κ∘F, g(w,u/2)=1/2 and
g(w,F∗ψ)=0. To this end, we consider the variation
x(t,s)=F(t,sa,sψ) of curves in M, with any fixed a∈R and
ψ∈V. Clearly, w=xt along the variation (notation of
Section 1). Next, xts=xst is tangent to D⊥, since
so is xs, while D⊥ is parallel. Consequently,
[g(xt,u)]s=0, as u is parallel and tangent to D.
Thus, g(w,u)=g(xt,u)=1. (Note that g(xt,u)=1 at s=0, due to
(d), as the geodesic t↦x(t) is parametrized by the function
t.) However, xss=0 and xs is tangent to D⊥, so
that (3) and (8) now give
xtss=[fg(xs,xs)+⟨Axs,xs⟩]u, which is parallel
in the s direction, while xts=xst=0 at s=0. Hence
xts=s[fg(xs,xs)+⟨Axs,xs⟩]u, and so
g(xts,xts)=0 (cf. (c) above and Lemma 2.2(a)). This
further yields [g(xt,xt)]ss/2=g(xt,xtss)=fg(xs,xs)+⟨Axs,xs⟩. The last function is constant in the
s direction, while g(xt,xt)=[g(xt,xt)]s=0 at s=0, and
so g(w,w)=g(xt,xt)=s2[fg(xs,xs)+⟨Axs,xs⟩]=κ.
Finally, being proportional to u at each point, xts is orthogonal
to D⊥, and hence to F∗ψ, which imples that
[g(xt,F∗ψ)]s=0, and, as g(w,F∗ψ)=g(xt,F∗ψ)=0
at s=0, we get g(w,F∗ψ)=0 everywhere.
∎
We are now in a position to prove Theorem 4.1. First, (7) is
conformally symmetric and has d=1, as one can verify by a direct calculation, cf. [16, Theorem 3]. Conversely, if conditions (a) and (b) above are
satisfied, we may also assume (c) – (f). (See the comment following (f).) Our
assertion is now immediate from Lemma 5.1.
We prove Lemma 2.1 here, since Olszak’s paper [13] may be
difficult to obtain.
The condition d=n is equivalent to conformal flatness
of (M,g), since n>2 and so Ω=0 is the only
2-form ∧-divisible by all nonzero 1-forms ξ. At a
fixed point x, the metric gx allows us to treat the Ricci tensor
ρx and any 2-form Ωx as endomorphisms of
TxM, so that we may consider their images (which are subspaces of
TxM). If W=0, fixing a nonzero 2-form Ωx in
the image of Wx acting on 2-forms at x we see that, for
every u∈Dx, our Ωx is ∧-divisible by
ξ=gx(u,⋅), and so the image of Ωx contains
Dx. Thus, d≤2, and (i) follows. (Being nonzero and decomposable,
Ωx has rank 2.) As shown in [6, Theorem 7 on p. 18], if (M,g) is essentially conformally symmetric, the image of ρx is a
subspace of Dx, so that (i) yields (ii), since g in (ii) cannot be
Ricci-flat. Next, if d=2, the image of our Ωx
coincides with Dx (as rankΩx=2). Every
2-form in the image of Wx thus is a multiple of
Ωx, being the exterior product of two vectors in Dx,
identified, via gx, with 1-forms. Hence rankW=1. Conversely, if
rankW=1, all nonzero 2-forms Ωx in the image of
Wx are of rank 2, as Wx, being self-adjoint, is a
multiple of Ωx⊗Ωx, and so the Bianchi
identity for W gives Ωx∧Ωx=0. All such
Ωx are therefore ∧-divisible by
ξ=gx(u,⋅), for every nonzero vector u in the common
2-dimensional image of such Ωx, which shows that d=2.
Finally, (iv) follows if one chooses Ωx=0 equal to
Wx(v,v′,⋅,⋅) for some
v,v′∈TxM.
Parts (b) and (c) of Lemma 2.2 for locally symmetric manifolds
with d=1 could, in principle, be derived from Cahen and Parker’s
classification [1] of
pseudo-Riemannian symmetric manifolds. We prove them here
directly, for the reader’s convenience. Our argument uses assertions (a),
(d) in Lemma 2.2, along with (e) for W, which were
established in the proof of Lemma 2.2 before Appendix II was
mentioned.
Suppose that ∇R=0 and d=1. Replacing M by an open
subset, we also assume that the Olszak distribution D is spanned by a vector field
u. By (1),
[TABLE]
for some differential 2-form Ω, which obviously does not
depend on the choice of u. (It is also clear from (1) that
Ω is the curvature form of the connection in the line bundle
D, induced by the Levi-Civita connection of g.) Being unique, Ω is
parallel, and so are ρ and W, which implies the Ricci
identities R⋅Ω=0, R⋅ρ=0, and R⋅W=0. In
coordinates: Rmljsτsk+Rmlksτjs=0, where
τ=Ω or τ=ρ, and
[TABLE]
Summing RmljsΩsk+RmlksΩjs=0
against ul, we obtain Ω∘Ω=0, where the
metric g is used to treat Ω as a bundle morphism
TM→TM that sends each vector field v to the vector field
Ωv with
g(Ωv,v′)=Ω(v,v′) for all vector
fields v′. Lemma 2.2(d) and (9.i) give
W(⋅,⋅,u,v)=R(⋅,⋅,u,v)=0 for our
fixed vector field u, spanning D, and any section v of
D⊥. Hence, by (2),
g(u,⋅)∧σ(v,⋅)=g(v,⋅)∧σ(u,⋅). Thus, σu=cu for
the Schouten tensor σ and some constant c, with
σu defined analogously to Ωv. (Otherwise, choosing
v such that u,σu and v are linearly independent at a
given point x, we would obtain a contradiction with the equality between
planes in TxM, corresponding to the above equality between exterior
products.) Consequently,
g(u,⋅)∧(σ+cg)(v,⋅)=0, and so
σv+cv is a section of D whenever v is a section
of D⊥. Let us now fix u′ as in (4). Symmetry of
σ gives g(σu′,u)=c. In a suitably ordered
basis with (5), at any point x, the endomorphism of TxM
corresponding to σx thus has an upper triangular matrix with the
diagonal entries c,−c,…,−c,c, so that
trgσ=(4−n)c. Consequently,
(n−2)s=2(n−1)(4−n)c, for the scalar curvature
s , and (n−2)ρu=2cu. However, contracting
(9.ii) in k=s, we get ρu=−Ωu, and so
(n−2)Ωu=−2cu. The equality
Ω∘Ω=0 that we derived from the Ricci
identity R⋅Ω=0 now gives c=0. Hence
s=0 (which yields Lemma 2.2(c)), and
ρu=0.
As c=0 and σ=ρ, the assertion about σv+cv
obtained above means that ρv is a section of D
whenever v is a section of D⊥. Let λ,μ,ξ
be the 1-forms with λ=g(u,⋅),
μ=g(u′,⋅), ξ(u′)=0, and
ρv=ξ(v)u for sections v of D⊥.
Transvecting (9.ii) with μs, we get
Ω=R(⋅,⋅,u,u′)=(n−2)−1λ∧ρ(u′,⋅) from
Lemma 2.2(c) with ρu=0 and Lemma 2.2(d).
However, evaluating ρ(u′,⋅) on u′,u
and sections v of D⊥, we see that
ρ(u′,⋅)=hλ+ξ, with
h=ρ(u′,u′). (Note that ξ(u)=0 since
ρu=0, while D⊂D⊥ by Lemma 2.2(a).)
Therefore,
[TABLE]
In addition, if v′ denotes the unique vector field with
g(v′,⋅)=ξ, then u and v′ are null and
orthogonal, or, equivalently,
[TABLE]
In fact, g(u,u)=0 by Lemma 2.2(a),
g(u,v′)=0 as ξ(u)=0, and v′ is null since
(11) yields (n−2)[ρ(Ωu′)−Ω(ρu′)]=2g(v′,v′)u,
while, transvecting the Ricci identity
RmljsRsk+RmlksRjs=0 with ul and using
(9.ii), we see that ρ and Ω commute
as bundle morphisms TM→TM.
Furthermore, transvecting with μkμm the coordinate form
Rmljsτsk+Rmlksτjs=0 of the Ricci
identity R⋅τ=0 for the parallel tensor field
τ=(n−2)Ω+ρ=hλ⊗λ+2λ⊗ξ (cf. (11)),
we get 2λjblsξs=0, where
b=W(u′,⋅,u′,⋅). Namely,
R=W+(n−2)−1g∧ρ by Lemma 2.2(c),
Wmljsτsk=0 in view of Lemma 2.2(d),
μkμmWmlksτjs=2λjblsξs since
b(u,⋅)=0 (again from Lemma 2.2(d)), and the
remaining terms, related to g∧ρ, add up to 0 as a
consequence of (12), (11.ii) and the formula for τ.
(Note that (12) gives Rjsτsk=Rjsτks=0,
and so four out of the eight remaining terms vanish individually.)
However, u=0, and so λ=0, which gives
b(⋅,v′)=0, where v′ is the vector field
with g(v′,⋅)=ξ. Thus,
W(u′,⋅,u′,v′)=0. As a result, the
3-tensor W(⋅,⋅,⋅,v′) must vanish:
it yields the value 0 whenever each of the three arguments is
either u′ or a section of D⊥. (Lemma 2.2(e) for
W is already established.)
The relation W(⋅,⋅,⋅,v′)=0 implies in
turn that W(⋅,⋅,⋅,ρv)=0 (in
coordinates: WjklsRsp=0). In fact, by (11.ii), the
image of ρ is spanned by u and v′, while
W(⋅,⋅,⋅,u)=0 according to
Lemma 2.2(d).
As in [13, 1o on p. 214], we have
W=(λ⊗λ)∧b (notation of (2)),
where, again, b=W(u′,⋅,u′,⋅). Namely, by
Lemma 2.2(e) for W, both sides agree on any quadruple of vector
fields, each of which is either u′ or a section of D⊥.
Finally, transvecting (10) with μkμm and replacing
R by W+(n−2)−1g∧ρ, we obtain two
contributions, one from W and one from g∧ρ, the sum
of which is zero. Since W=(λ⊗λ)∧b, the
W contribution vanishes: its first two terms add up to 0, and so do
its other two terms. (As we saw, b(u,⋅)=0, while, obviously,
b(u′,⋅)=0.) Out of the sixteen terms forming the
g∧ρ contribution, eight are separately equal to zero since
WjklsRsp=0, and so, in view of (11.ii) and the
relation W=(λ⊗λ)∧b, vanishing of the
g∧ρ contribution gives λpSjlq=λqSjlp, for
Sjlq=2bjlξq−bqlξj−bqjξl. Thus, Sjlq=ηjlλq for some
twice-covariant symmetric tensor field η, which, summed
cyclically over j,l,q, yields 0 (due to the definition
of Sjlq and symmetry of b). As λ=0 and the
symmetric product has no zero divisors, we get η=0 and
Sjlq=0. The expression bjlξq−bqlξj is,
therefore, skew-symmetric in j,l. As it is also, clearly,
skew-symmetric in j,q, it must be totally skew-symmetric
and hence equal to one-third of its cyclic sum over j,l,q. That
cyclic sum, however, is 0 in view of symmetry of b, so that
bjlξq=bqlξj. Thus, ξ=0, for otherwise the last
equality would yield b=φξ⊗ξ for some function
φ, and hence W=(λ⊗λ)∧b=φ(λ⊗λ)∧(ξ⊗ξ), which would
clearly imply that the vector field v′ with
g(v′,⋅)=ξ is a section of the Olszak distribution D, not
equal to a function times u (as ξ(u′)=0, while
g(u,u′)=1), contradicting one-dimensionality of D.
Therefore, ρ=hλ⊗λ by (11.ii) with
ξ=0, which proves assertion (b) of Lemma 2.2 in our case.
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