• Source: Ricci curvature

In differential geometry, the Ricci curvature tensor, named after Gregorio Ricci-Curbastro, is a geometric object which is determined by a choice of Riemannian or pseudo-Riemannian metric on a manifold. It can be considered, broadly, as a measure of the degree to which the geometry of a given metric tensor differs locally from that of ordinary Euclidean space or pseudo-Euclidean space.
The Ricci tensor can be characterized by measurement of how a shape is deformed as one moves along geodesics in the space. In general relativity, which involves the pseudo-Riemannian setting, this is reflected by the presence of the Ricci tensor in the Raychaudhuri equation. Partly for this reason, the Einstein field equations propose that spacetime can be described by a pseudo-Riemannian metric, with a strikingly simple relationship between the Ricci tensor and the matter content of the universe.
Like the metric tensor, the Ricci tensor assigns to each tangent space of the manifold a symmetric bilinear form (Besse 1987, p. 43). Broadly, one could analogize the role of the Ricci curvature in Riemannian geometry to that of the Laplacian in the analysis of functions; in this analogy, the Riemann curvature tensor, of which the Ricci curvature is a natural by-product, would correspond to the full matrix of second derivatives of a function. However, there are other ways to draw the same analogy.
In three-dimensional topology, the Ricci tensor contains all of the information which in higher dimensions is encoded by the more complicated Riemann curvature tensor. In part, this simplicity allows for the application of many geometric and analytic tools, which led to the solution of the Poincaré conjecture through the work of Richard S. Hamilton and Grigori Perelman.
In differential geometry, lower bounds on the Ricci tensor on a Riemannian manifold allow one to extract global geometric and topological information by comparison (cf. comparison theorem) with the geometry of a constant curvature space form. This is since lower bounds on the Ricci tensor can be successfully used in studying the length functional in Riemannian geometry, as first shown in 1941 via Myers's theorem.
One common source of the Ricci tensor is that it arises whenever one commutes the covariant derivative with the tensor Laplacian. This, for instance, explains its presence in the Bochner formula, which is used ubiquitously in Riemannian geometry. For example, this formula explains why the gradient estimates due to Shing-Tung Yau (and their developments such as the Cheng-Yau and Li-Yau inequalities) nearly always depend on a lower bound for the Ricci curvature.
In 2007, John Lott, Karl-Theodor Sturm, and Cedric Villani demonstrated decisively that lower bounds on Ricci curvature can be understood entirely in terms of the metric space structure of a Riemannian manifold, together with its volume form. This established a deep link between Ricci curvature and Wasserstein geometry and optimal transport, which is presently the subject of much research.




Definition


Suppose that




(

M
,
g

)



{\displaystyle \left(M,g\right)}

is an



n


{\displaystyle n}

-dimensional
Riemannian or pseudo-Riemannian manifold, equipped
with its Levi-Civita connection



∇


{\displaystyle \nabla }

. The
Riemann curvature of



M


{\displaystyle M}

is a map which
takes smooth vector fields



X


{\displaystyle X}

,



Y


{\displaystyle Y}

, and



Z


{\displaystyle Z}

,
and returns the vector field



R
(
X
,
Y
)
Z
:=

∇

X



∇

Y


Z
−

∇

Y



∇

X


Z
−

∇

[
X
,
Y
]


Z


{\displaystyle R(X,Y)Z:=\nabla _{X}\nabla _{Y}Z-\nabla _{Y}\nabla _{X}Z-\nabla _{[X,Y]}Z}

on vector fields



X
,
Y
,
Z


{\displaystyle X,Y,Z}

. Since



R


{\displaystyle R}

is a tensor field, for
each point



p
∈
M


{\displaystyle p\in M}

, it gives rise to a (multilinear) map:




R

p


:

T

p


M
×

T

p


M
×

T

p


M
→

T

p


M
.


{\displaystyle \operatorname {R} _{p}:T_{p}M\times T_{p}M\times T_{p}M\to T_{p}M.}

Define for each point



p
∈
M


{\displaystyle p\in M}

the map




Ric

p


:

T

p


M
×

T

p


M
→

R



{\displaystyle \operatorname {Ric} _{p}:T_{p}M\times T_{p}M\to \mathbb {R} }

by





Ric

p


⁡
(
Y
,
Z
)
:=
tr
⁡


(


X
↦

R

p


⁡
(
X
,
Y
)
Z


)


.


{\displaystyle \operatorname {Ric} _{p}(Y,Z):=\operatorname {tr} {\big (}X\mapsto \operatorname {R} _{p}(X,Y)Z{\big )}.}


That is, having fixed



Y


{\displaystyle Y}

and



Z


{\displaystyle Z}

, then for any orthonormal basis





v

1


,
…
,

v

n




{\displaystyle v_{1},\ldots ,v_{n}}

of the vector space




T

p


M


{\displaystyle T_{p}M}

, one has





Ric

p


⁡
(
Y
,
Z
)
=

∑

i
=
1


⟨

R

p


⁡
(

v

i


,
Y
)
Z
,

v

i


⟩
.


{\displaystyle \operatorname {Ric} _{p}(Y,Z)=\sum _{i=1}\langle \operatorname {R} _{p}(v_{i},Y)Z,v_{i}\rangle .}


It is a standard exercise of (multi)linear
algebra to verify that this definition does not depend on the choice of the basis





v

1


,
…
,

v

n




{\displaystyle v_{1},\ldots ,v_{n}}

.
In abstract index notation,






R
i
c


a
b


=


R


c







b
c
a


=


R


c







a
c
b


.


{\displaystyle \mathrm {Ric} _{ab}=\mathrm {R} ^{c}{}_{bca}=\mathrm {R} ^{c}{}_{acb}.}


Sign conventions. Note that some sources define



R
(
X
,
Y
)
Z


{\displaystyle R(X,Y)Z}

to be
what would here be called



−
R
(
X
,
Y
)
Z
;


{\displaystyle -R(X,Y)Z;}

they would then define





Ric

p




{\displaystyle \operatorname {Ric} _{p}}

as



−
tr
⁡
(
X
↦

R

p


⁡
(
X
,
Y
)
Z
)
.


{\displaystyle -\operatorname {tr} (X\mapsto \operatorname {R} _{p}(X,Y)Z).}


Although sign conventions differ about the Riemann tensor, they do not differ about
the Ricci tensor.




= Definition via local coordinates on a smooth manifold

=
Let




(

M
,
g

)



{\displaystyle \left(M,g\right)}

be a smooth Riemannian
or pseudo-Riemannian



n


{\displaystyle n}

-manifold.
Given a smooth chart




(

U
,
φ

)



{\displaystyle \left(U,\varphi \right)}

one then has functions





g

i
j


:
φ
(
U
)
→

R



{\displaystyle g_{ij}:\varphi (U)\rightarrow \mathbb {R} }

and





g

i
j


:
φ
(
U
)
→

R



{\displaystyle g^{ij}:\varphi (U)\rightarrow \mathbb {R} }

for each




i
,
j
=
1
,
…
,
n


{\displaystyle i,j=1,\ldots ,n}

which satisfy





∑

k
=
1


n



g

i
k


(
x
)

g

k
j


(
x
)
=

δ

j


i


=


{



1


i
=
j




0


i
≠
j








{\displaystyle \sum _{k=1}^{n}g^{ik}(x)g_{kj}(x)=\delta _{j}^{i}={\begin{cases}1&i=j\\0&i\neq j\end{cases}}}


for all



x
∈
φ
(
U
)


{\displaystyle x\in \varphi (U)}

. The latter shows that, expressed as
matrices,




g

i
j


(
x
)
=
(

g

−
1



)

i
j


(
x
)


{\displaystyle g^{ij}(x)=(g^{-1})_{ij}(x)}

.
The functions




g

i
j




{\displaystyle g_{ij}}

are defined by evaluating



g


{\displaystyle g}

on
coordinate vector fields, while the functions




g

i
j




{\displaystyle g^{ij}}

are defined so
that, as a matrix-valued function, they provide an inverse to the matrix-valued
function



x
↦

g

i
j


(
x
)


{\displaystyle x\mapsto g_{ij}(x)}

.
Now define, for each



a


{\displaystyle a}

,



b


{\displaystyle b}

,



c


{\displaystyle c}

,



i


{\displaystyle i}

,
and



j


{\displaystyle j}

between 1 and



n


{\displaystyle n}

, the functions









Γ

a
b


c





:=


1
2



∑

d
=
1


n



(




∂

g

b
d




∂

x

a





+



∂

g

a
d




∂

x

b





−



∂

g

a
b




∂

x

d






)


g

c
d







R

i
j





:=

∑

a
=
1


n





∂

Γ

i
j


a




∂

x

a





−

∑

a
=
1


n





∂

Γ

a
i


a




∂

x

j





+

∑

a
=
1


n



∑

b
=
1


n



(


Γ

a
b


a



Γ

i
j


b


−

Γ

i
b


a



Γ

a
j


b



)







{\displaystyle {\begin{aligned}\Gamma _{ab}^{c}&:={\frac {1}{2}}\sum _{d=1}^{n}\left({\frac {\partial g_{bd}}{\partial x^{a}}}+{\frac {\partial g_{ad}}{\partial x^{b}}}-{\frac {\partial g_{ab}}{\partial x^{d}}}\right)g^{cd}\\R_{ij}&:=\sum _{a=1}^{n}{\frac {\partial \Gamma _{ij}^{a}}{\partial x^{a}}}-\sum _{a=1}^{n}{\frac {\partial \Gamma _{ai}^{a}}{\partial x^{j}}}+\sum _{a=1}^{n}\sum _{b=1}^{n}\left(\Gamma _{ab}^{a}\Gamma _{ij}^{b}-\Gamma _{ib}^{a}\Gamma _{aj}^{b}\right)\end{aligned}}}


as maps



φ
:
U
→

R



{\displaystyle \varphi :U\rightarrow \mathbb {R} }

.
Now let




(

U
,
φ

)



{\displaystyle \left(U,\varphi \right)}

and




(

V
,
ψ

)



{\displaystyle \left(V,\psi \right)}

be two smooth charts with



U
∩
V
≠
∅


{\displaystyle U\cap V\neq \emptyset }

.
Let




R

i
j


:
φ
(
U
)
→

R



{\displaystyle R_{ij}:\varphi (U)\rightarrow \mathbb {R} }

be the functions computed as above via the chart




(

U
,
φ

)



{\displaystyle \left(U,\varphi \right)}

and let




r

i
j


:
ψ
(
V
)
→

R



{\displaystyle r_{ij}:\psi (V)\rightarrow \mathbb {R} }

be the functions computed as above via the chart




(

V
,
ψ

)



{\displaystyle \left(V,\psi \right)}

.
Then one can check by a calculation with the chain rule and the product rule that





R

i
j


(
x
)
=

∑

k
,
l
=
1


n



r

k
l



(

ψ
∘

φ

−
1


(
x
)

)


D

i





|



x




(

ψ
∘

φ

−
1



)


k



D

j





|



x




(

ψ
∘

φ

−
1



)


l


.


{\displaystyle R_{ij}(x)=\sum _{k,l=1}^{n}r_{kl}\left(\psi \circ \varphi ^{-1}(x)\right)D_{i}{\Big |}_{x}\left(\psi \circ \varphi ^{-1}\right)^{k}D_{j}{\Big |}_{x}\left(\psi \circ \varphi ^{-1}\right)^{l}.}


where




D

i




{\displaystyle D_{i}}

is the first derivative along



i


{\displaystyle i}

th direction
of





R


n




{\displaystyle \mathbb {R} ^{n}}

.
This shows that the following definition does not depend on the choice of





(

U
,
φ

)



{\displaystyle \left(U,\varphi \right)}

.
For any



p
∈
U


{\displaystyle p\in U}

, define a bilinear map





Ric

p


:

T

p


M
×

T

p


M
→

R



{\displaystyle \operatorname {Ric} _{p}:T_{p}M\times T_{p}M\rightarrow \mathbb {R} }

by




(
X
,
Y
)
∈

T

p


M
×

T

p


M
↦

Ric

p


⁡
(
X
,
Y
)
=

∑

i
,
j
=
1


n



R

i
j


(
φ
(
x
)
)

X

i


(
p
)

Y

j


(
p
)
,


{\displaystyle (X,Y)\in T_{p}M\times T_{p}M\mapsto \operatorname {Ric} _{p}(X,Y)=\sum _{i,j=1}^{n}R_{ij}(\varphi (x))X^{i}(p)Y^{j}(p),}


where




X

1


,
…
,

X

n




{\displaystyle X^{1},\ldots ,X^{n}}

and




Y

1


,
…
,

Y

n




{\displaystyle Y^{1},\ldots ,Y^{n}}

are the
components of the tangent vectors at



p


{\displaystyle p}

in



X


{\displaystyle X}

and



Y


{\displaystyle Y}

relative to
the coordinate vector fields of




(

U
,
φ

)



{\displaystyle \left(U,\varphi \right)}

.
It is common to abbreviate the above formal presentation in the following style:

The final line includes the demonstration that the bilinear map Ric is well-defined,
which is much easier to write out with the informal notation.




= Comparison of the definitions

=
The two above definitions are identical. The formulas defining




Γ

i
j


k




{\displaystyle \Gamma _{ij}^{k}}

and




R

i
j




{\displaystyle R_{ij}}

in the coordinate approach have an exact parallel in the formulas defining the Levi-Civita connection, and the Riemann curvature via the Levi-Civita connection. Arguably, the definitions directly using local coordinates are preferable, since the "crucial property" of the Riemann tensor mentioned above requires



M


{\displaystyle M}

to be Hausdorff in order to hold. By contrast, the local coordinate approach only requires a smooth atlas. It is also somewhat easier to connect the "invariance" philosophy underlying the local approach with the methods of constructing more exotic geometric objects, such as spinor fields.
The complicated formula defining




R

i
j




{\displaystyle R_{ij}}

in the introductory section is the same as that in the following section. The only difference is that terms have been grouped so that it is easy to see that




R

i
j


=

R

j
i


.


{\displaystyle R_{ij}=R_{ji}.}





Properties


As can be seen from the symmetries of the Riemann curvature tensor, the Ricci tensor of a Riemannian
manifold is symmetric, in the sense that




Ric
⁡
(
X
,
Y
)
=
Ric
⁡
(
Y
,
X
)


{\displaystyle \operatorname {Ric} (X,Y)=\operatorname {Ric} (Y,X)}


for all



X
,
Y
∈

T

p


M
.


{\displaystyle X,Y\in T_{p}M.}


It thus follows linear-algebraically that the Ricci tensor is completely determined
by knowing the quantity



Ric
⁡
(
X
,
X
)


{\displaystyle \operatorname {Ric} (X,X)}

for all vectors




X


{\displaystyle X}

of unit length. This function on the set of unit tangent vectors
is often also called the Ricci curvature, since knowing it is equivalent to
knowing the Ricci curvature tensor.
The Ricci curvature is determined by the sectional curvatures of a Riemannian
manifold, but generally contains less information. Indeed, if



ξ


{\displaystyle \xi }

is a
vector of unit length on a Riemannian



n


{\displaystyle n}

-manifold, then




Ric
⁡
(
ξ
,
ξ
)


{\displaystyle \operatorname {Ric} (\xi ,\xi )}

is precisely



(
n
−
1
)


{\displaystyle (n-1)}


times the average value of the sectional curvature, taken over all the 2-planes
containing



ξ


{\displaystyle \xi }

. There is an



(
n
−
2
)


{\displaystyle (n-2)}

-dimensional family
of such 2-planes, and so only in dimensions 2 and 3 does the Ricci tensor determine
the full curvature tensor. A notable exception is when the manifold is given a
priori as a hypersurface of Euclidean space. The second fundamental form,
which determines the full curvature via the Gauss–Codazzi equation,
is itself determined by the Ricci tensor and the principal directions
of the hypersurface are also the eigendirections of the Ricci tensor. The
tensor was introduced by Ricci for this reason.
As can be seen from the second Bianchi identity, one has




div
⁡
Ric
=


1
2


d
R
,


{\displaystyle \operatorname {div} \operatorname {Ric} ={\frac {1}{2}}dR,}


where



R


{\displaystyle R}

is the scalar curvature, defined in local coordinates as




g

i
j



R

i
j


.


{\displaystyle g^{ij}R_{ij}.}

This is often called the contracted second Bianchi identity.




Direct geometric meaning


Near any point



p


{\displaystyle p}

in a Riemannian manifold




(

M
,
g

)



{\displaystyle \left(M,g\right)}

,
one can define preferred local coordinates, called geodesic normal coordinates.
These are adapted to the metric so that geodesics through



p


{\displaystyle p}

correspond
to straight lines through the origin, in such a manner that the geodesic distance
from



p


{\displaystyle p}

corresponds to the Euclidean distance from the origin.
In these coordinates, the metric tensor is well-approximated by the Euclidean
metric, in the precise sense that





g

i
j


=

δ

i
j


+
O

(


|

x


|


2



)

.


{\displaystyle g_{ij}=\delta _{ij}+O\left(|x|^{2}\right).}


In fact, by taking the Taylor expansion of the metric applied to a Jacobi field along a radial geodesic in the normal coordinate system, one has





g

i
j


=

δ

i
j


−


1
3



R

i
k
j
l



x

k



x

l


+
O

(


|

x


|


3



)

.


{\displaystyle g_{ij}=\delta _{ij}-{\frac {1}{3}}R_{ikjl}x^{k}x^{l}+O\left(|x|^{3}\right).}


In these coordinates, the metric volume element then has the following expansion at p:




d

μ

g


=

[

1
−


1
6



R

j
k



x

j



x

k


+
O

(


|

x


|


3



)


]

d

μ

Euclidean


,


{\displaystyle d\mu _{g}=\left[1-{\frac {1}{6}}R_{jk}x^{j}x^{k}+O\left(|x|^{3}\right)\right]d\mu _{\text{Euclidean}},}


which follows by expanding the square root of the determinant of the metric.
Thus, if the Ricci curvature



Ric
⁡
(
ξ
,
ξ
)


{\displaystyle \operatorname {Ric} (\xi ,\xi )}

is positive
in the direction of a vector



ξ


{\displaystyle \xi }

, the conical region in



M


{\displaystyle M}


swept out by a tightly focused family of geodesic segments of length




ε


{\displaystyle \varepsilon }

emanating from



p


{\displaystyle p}

, with initial velocity inside
a small cone about



ξ


{\displaystyle \xi }

, will have smaller volume than the corresponding
conical region in Euclidean space, at least provided that



ε


{\displaystyle \varepsilon }


is sufficiently small. Similarly, if the Ricci curvature is negative in the
direction of a given vector



ξ


{\displaystyle \xi }

, such a conical region in the manifold
will instead have larger volume than it would in Euclidean space.
The Ricci curvature is essentially an average of curvatures in the planes including




ξ


{\displaystyle \xi }

. Thus if a cone emitted with an initially circular (or spherical)
cross-section becomes distorted into an ellipse (ellipsoid), it is possible
for the volume distortion to vanish if the distortions along the
principal axes counteract one another. The Ricci
curvature would then vanish along



ξ


{\displaystyle \xi }

. In physical applications, the
presence of a nonvanishing sectional curvature does not necessarily indicate the
presence of any mass locally; if an initially circular cross-section of a cone
of worldlines later becomes elliptical, without changing its volume, then
this is due to tidal effects from a mass at some other location.




Applications


Ricci curvature plays an important role in general relativity, where it is
the key term in the Einstein field equations.
Ricci curvature also appears in the Ricci flow equation, first
introduced by Richard S. Hamilton in 1982, where certain
one-parameter families of Riemannian metrics are singled out as solutions of a
geometrically-defined partial differential equation.
In harmonic local coordinates the Ricci tensor can be expressed as (Chow & Knopf 2004, Lemma 3.32).





R

i
j


=
−


1
2


Δ

(

g

i
j


)

+

lower-order terms

,


{\displaystyle R_{ij}=-{\frac {1}{2}}\Delta \left(g_{ij}\right)+{\text{lower-order terms}},}


where




g

i
j




{\displaystyle g_{ij}}

are the components of the metric tensor and



Δ


{\displaystyle \Delta }

is the Laplace–Beltrami operator.
This fact motivates the introduction of the Ricci flow equation
as a natural extension of the heat equation for the metric.
Since heat tends to spread through
a solid until the body reaches an equilibrium state of constant temperature, if
one is given a manifold, the Ricci flow may be hoped to produce an 'equilibrium'
Riemannian metric which is Einstein or of constant curvature.
However, such a clean "convergence" picture cannot be achieved since many manifolds
cannot support such metrics. A detailed study of the nature of solutions of the
Ricci flow, due principally to Hamilton and Grigori Perelman, shows that the
types of "singularities" that occur along a Ricci flow, corresponding to the
failure of convergence, encodes deep information about 3-dimensional topology.
The culmination of this work was a proof of the geometrization conjecture
first proposed by William Thurston in the 1970s, which can be thought of as
a classification of compact 3-manifolds.
On a Kähler manifold, the Ricci curvature determines the first Chern class
of the manifold (mod torsion). However, the Ricci curvature has no analogous
topological interpretation on a generic Riemannian manifold.




Global geometry and topology


Here is a short list of global results concerning manifolds with positive Ricci curvature; see also classical theorems of Riemannian geometry. Briefly, positive Ricci curvature of a Riemannian manifold has strong topological consequences, while (for dimension at least 3), negative Ricci curvature has no topological implications. (The Ricci curvature is said to be positive if the Ricci curvature function



Ric
⁡
(
ξ
,
ξ
)


{\displaystyle \operatorname {Ric} (\xi ,\xi )}

is positive on the set of non-zero tangent vectors



ξ


{\displaystyle \xi }

.) Some results are also known for pseudo-Riemannian manifolds.

Myers' theorem (1941) states that if the Ricci curvature is bounded from below on a complete Riemannian n-manifold by



(
n
−
1
)
k
>
0


{\displaystyle (n-1)k>0}

, then the manifold has diameter



≤
π

/



k




{\displaystyle \leq \pi /{\sqrt {k}}}

. By a covering-space argument, it follows that any compact manifold of positive Ricci curvature must have finite fundamental group. Cheng (1975) showed that, in this setting, equality in the diameter inequality occurs if only if the manifold is isometric to a sphere of a constant curvature



k


{\displaystyle k}

.
The Bishop–Gromov inequality states that if a complete



n


{\displaystyle n}

-dimensional Riemannian manifold has non-negative Ricci curvature, then the volume of a geodesic ball is less than or equal to the volume of a geodesic ball of the same radius in Euclidean



n


{\displaystyle n}

-space. Moreover, if




v

p


(
R
)


{\displaystyle v_{p}(R)}

denotes the volume of the ball with center



p


{\displaystyle p}

and radius



R


{\displaystyle R}

in the manifold and



V
(
R
)
=

c

n



R

n




{\displaystyle V(R)=c_{n}R^{n}}

denotes the volume of the ball of radius



R


{\displaystyle R}

in Euclidean



n


{\displaystyle n}

-space then the function




v

p


(
R
)

/

V
(
R
)


{\displaystyle v_{p}(R)/V(R)}

is nonincreasing. This can be generalized to any lower bound on the Ricci curvature (not just nonnegativity), and is the key point in the proof of Gromov's compactness theorem.)
The Cheeger–Gromoll splitting theorem states that if a complete Riemannian manifold




(

M
,
g

)



{\displaystyle \left(M,g\right)}

with



Ric
≥
0


{\displaystyle \operatorname {Ric} \geq 0}

contains a line, meaning a geodesic



γ
:

R

→
M


{\displaystyle \gamma :\mathbb {R} \to M}

such that



d
(
γ
(
u
)
,
γ
(
v
)
)
=

|

u
−
v

|



{\displaystyle d(\gamma (u),\gamma (v))=\left|u-v\right|}

for all



u
,
v
∈

R



{\displaystyle u,v\in \mathbb {R} }

, then it is isometric to a product space




R

×
L


{\displaystyle \mathbb {R} \times L}

. Consequently, a complete manifold of positive Ricci curvature can have at most one topological end. The theorem is also true under some additional hypotheses for complete Lorentzian manifolds (of metric signature




(

+
−
−
…

)



{\displaystyle \left(+--\ldots \right)}

) with non-negative Ricci tensor (Galloway 2000).
Hamilton's first convergence theorem for Ricci flow has, as a corollary, that the only compact 3-manifolds which have Riemannian metrics of positive Ricci curvature are the quotients of the 3-sphere by discrete subgroups of SO(4) which act properly discontinuously. He later extended this to allow for nonnegative Ricci curvature. In particular, the only simply-connected possibility is the 3-sphere itself.
These results, particularly Myers' and Hamilton's, show that positive Ricci curvature has strong topological consequences. By contrast, excluding the case of surfaces, negative Ricci curvature is now known to have no topological implications; Lohkamp (1994) has shown that any manifold of dimension greater than two admits a complete Riemannian metric of negative Ricci curvature. In the case of two-dimensional manifolds, negativity of the Ricci curvature is synonymous with negativity of the Gaussian curvature, which has very clear topological implications. There are very few two-dimensional manifolds which fail to admit Riemannian metrics of negative Gaussian curvature.




Behavior under conformal rescaling


If the metric



g


{\displaystyle g}

is changed by multiplying it by a conformal factor





e

2
f




{\displaystyle e^{2f}}

, the Ricci tensor of the new, conformally-related metric







g
~



=

e

2
f


g


{\displaystyle {\tilde {g}}=e^{2f}g}

is given (Besse 1987, p. 59) by







Ric
~



=
Ric
+
(
2
−
n
)

[

∇
d
f
−
d
f
⊗
d
f

]

+

[

Δ
f
−
(
n
−
2
)
‖
d
f

‖

2



]

g
,


{\displaystyle {\widetilde {\operatorname {Ric} }}=\operatorname {Ric} +(2-n)\left[\nabla df-df\otimes df\right]+\left[\Delta f-(n-2)\|df\|^{2}\right]g,}


where



Δ
=
∗
d
∗
d


{\displaystyle \Delta =*d*d}

is the (positive spectrum) Hodge Laplacian, i.e.,
the opposite of the usual trace of the Hessian.
In particular, given a point



p


{\displaystyle p}

in a Riemannian manifold, it is always
possible to find metrics conformal to the given metric



g


{\displaystyle g}

for which the
Ricci tensor vanishes at



p


{\displaystyle p}

. Note, however, that this is only pointwise
assertion; it is usually impossible to make the Ricci curvature vanish identically
on the entire manifold by a conformal rescaling.
For two dimensional manifolds, the above formula shows that if



f


{\displaystyle f}

is a
harmonic function, then the conformal scaling



g
↦

e

2
f


g


{\displaystyle g\mapsto e^{2f}g}


does not change the Ricci tensor (although it still changes its trace with respect
to the metric unless



f
=
0


{\displaystyle f=0}

.




Trace-free Ricci tensor


In Riemannian geometry and pseudo-Riemannian geometry, the
trace-free Ricci tensor (also called traceless Ricci tensor) of a
Riemannian or pseudo-Riemannian



n


{\displaystyle n}

-manifold




(

M
,
g

)



{\displaystyle \left(M,g\right)}


is the tensor defined by




Z
=
Ric
−


1
n


R
g
,


{\displaystyle Z=\operatorname {Ric} -{\frac {1}{n}}Rg,}


where



Ric


{\displaystyle \operatorname {Ric} }

and



R


{\displaystyle R}

denote the Ricci curvature
and scalar curvature of



g


{\displaystyle g}

. The name of this object reflects the
fact that its trace automatically vanishes:





tr

g


⁡
Z
≡

g

a
b



Z

a
b


=
0.


{\displaystyle \operatorname {tr} _{g}Z\equiv g^{ab}Z_{ab}=0.}

However, it is quite an
important tensor since it reflects an "orthogonal decomposition" of the Ricci tensor.




= The orthogonal decomposition of the Ricci tensor

=
The following, not so trivial, property is




Ric
=
Z
+


1
n


R
g
.


{\displaystyle \operatorname {Ric} =Z+{\frac {1}{n}}Rg.}


It is less immediately obvious that the two terms on the right hand side are orthogonal
to each other:






⟨

Z
,


1
n


R
g

⟩


g


≡

g

a
b



(


R

a
b


−


1
n


R

g

a
b



)

=
0.


{\displaystyle \left\langle Z,{\frac {1}{n}}Rg\right\rangle _{g}\equiv g^{ab}\left(R_{ab}-{\frac {1}{n}}Rg_{ab}\right)=0.}


An identity which is intimately connected with this (but which could be proved directly)
is that






|
Ric
|


g


2


=

|

Z


|


g


2


+


1
n



R

2


.


{\displaystyle \left|\operatorname {Ric} \right|_{g}^{2}=|Z|_{g}^{2}+{\frac {1}{n}}R^{2}.}





= The trace-free Ricci tensor and Einstein metrics

=
By taking a divergence, and using the contracted Bianchi identity, one sees that




Z
=
0


{\displaystyle Z=0}

implies





1
2


d
R
−


1
n


d
R
=
0


{\textstyle {\frac {1}{2}}dR-{\frac {1}{n}}dR=0}

.
So, provided that n ≥ 3 and



M


{\displaystyle M}

is connected, the vanishing
of



Z


{\displaystyle Z}

implies that the scalar curvature is constant. One can then see
that the following are equivalent:




Z
=
0


{\displaystyle Z=0}





Ric
=
λ
g


{\displaystyle \operatorname {Ric} =\lambda g}

for some number



λ


{\displaystyle \lambda }





Ric
=


1
n


R
g


{\displaystyle \operatorname {Ric} ={\frac {1}{n}}Rg}


In the Riemannian setting, the above orthogonal decomposition shows that





R

2


=
n

|

Ric
⁡


|


2




{\displaystyle R^{2}=n|\operatorname {Ric} |^{2}}

is also equivalent to these conditions.
In the pseudo-Riemmannian setting, by contrast, the condition




|

Z


|


g


2


=
0


{\displaystyle |Z|_{g}^{2}=0}


does not necessarily imply



Z
=
0
,


{\displaystyle Z=0,}

so the most that one can say is that
these conditions imply




R

2


=
n


|
Ric
|


g


2


.


{\displaystyle R^{2}=n\left|\operatorname {Ric} \right|_{g}^{2}.}


In particular, the vanishing of trace-free Ricci tensor characterizes
Einstein manifolds, as defined by the condition



Ric
=
λ
g


{\displaystyle \operatorname {Ric} =\lambda g}


for a number



λ
.


{\displaystyle \lambda .}

In general relativity, this equation states
that




(

M
,
g

)



{\displaystyle \left(M,g\right)}

is a solution of Einstein's vacuum field
equations with cosmological constant.




Kähler manifolds


On a Kähler manifold



X


{\displaystyle X}

, the Ricci curvature determines the
curvature form of the canonical line bundle
(Moroianu 2007, Chapter 12). The canonical line bundle is the top
exterior power of the bundle of holomorphic Kähler differentials:




κ
=



⋀



n




Ω

X


.


{\displaystyle \kappa ={\textstyle \bigwedge }^{n}~\Omega _{X}.}


The Levi-Civita connection corresponding to the metric on



X


{\displaystyle X}

gives
rise to a connection on



κ


{\displaystyle \kappa }

. The curvature of this connection is
the 2-form defined by




ρ
(
X
,
Y
)





=


def





Ric
⁡
(
J
X
,
Y
)


{\displaystyle \rho (X,Y)\;{\stackrel {\text{def}}{=}}\;\operatorname {Ric} (JX,Y)}


where



J


{\displaystyle J}

is the complex structure map on the
tangent bundle determined by the structure of the Kähler manifold. The Ricci
form is a closed 2-form. Its cohomology class is,
up to a real constant factor, the first Chern class of the canonical bundle,
and is therefore a topological invariant of



X


{\displaystyle X}

(for compact



X


{\displaystyle X}

)
in the sense that it depends only on the topology of



X


{\displaystyle X}

and the
homotopy class of the complex structure.
Conversely, the Ricci form determines the Ricci tensor by




Ric
⁡
(
X
,
Y
)
=
ρ
(
X
,
J
Y
)
.


{\displaystyle \operatorname {Ric} (X,Y)=\rho (X,JY).}


In local holomorphic coordinates




z

α




{\displaystyle z^{\alpha }}

, the Ricci form is given by




ρ
=
−
i
∂


∂
¯


log
⁡
det

(

g

α


β
¯




)



{\displaystyle \rho =-i\partial {\overline {\partial }}\log \det \left(g_{\alpha {\overline {\beta }}}\right)}


where ∂ is the Dolbeault operator and





g

α


β
¯




=
g

(



∂

∂

z

α





,


∂

∂



z
¯



β






)

.


{\displaystyle g_{\alpha {\overline {\beta }}}=g\left({\frac {\partial }{\partial z^{\alpha }}},{\frac {\partial }{\partial {\overline {z}}^{\beta }}}\right).}


If the Ricci tensor vanishes, then the canonical bundle is flat, so the
structure group can be locally reduced to a subgroup of the
special linear group



S
L
(
n
;

C

)


{\displaystyle SL(n;\mathbb {C} )}

. However, Kähler manifolds
already possess holonomy in



U
(
n
)


{\displaystyle U(n)}

, and so the (restricted)
holonomy of a Ricci-flat Kähler manifold is contained in



S
U
(
n
)


{\displaystyle SU(n)}

.
Conversely, if the (restricted) holonomy of a 2



n


{\displaystyle n}

-dimensional Riemannian
manifold is contained in



S
U
(
n
)


{\displaystyle SU(n)}

, then the manifold is a Ricci-flat
Kähler manifold (Kobayashi & Nomizu 1996, IX, §4).




Generalization to affine connections


The Ricci tensor can also be generalized to arbitrary affine connections,
where it is an invariant that plays an especially important role in the study of
projective geometry (geometry associated to
unparameterized geodesics) (Nomizu & Sasaki 1994). If



∇


{\displaystyle \nabla }


denotes an affine connection, then the curvature tensor



R


{\displaystyle R}

is the
(1,3)-tensor defined by




R
(
X
,
Y
)
Z
=

∇

X



∇

Y


Z
−

∇

Y



∇

X


Z
−

∇

[
X
,
Y
]


Z


{\displaystyle R(X,Y)Z=\nabla _{X}\nabla _{Y}Z-\nabla _{Y}\nabla _{X}Z-\nabla _{[X,Y]}Z}


for any vector fields



X
,
Y
,
Z


{\displaystyle X,Y,Z}

. The Ricci tensor is defined to be the trace:




ric
⁡
(
X
,
Y
)
=
tr
⁡


(


Z
↦
R
(
Z
,
X
)
Y


)


.


{\displaystyle \operatorname {ric} (X,Y)=\operatorname {tr} {\big (}Z\mapsto R(Z,X)Y{\big )}.}


In this more general situation, the Ricci tensor is symmetric if and only if there
exists locally a parallel volume form for the connection.




Discrete Ricci curvature


Notions of Ricci curvature on discrete manifolds have been defined on graphs and
networks, where they quantify local divergence properties of edges. Ollivier's
Ricci curvature is defined using optimal transport theory.
A different (and earlier) notion, Forman's Ricci curvature, is based on
topological arguments.




See also






Footnotes






References


Besse, A.L. (1987), Einstein manifolds, Springer, ISBN 978-3-540-15279-8.
Chow, Bennet & Knopf, Dan (2004), The Ricci Flow: an introduction, American Mathematical Society, ISBN 0-8218-3515-7.
Eisenhart, L.P. (1949), Riemannian geometry, Princeton Univ. Press.
Forman (2003), "Bochner's Method for Cell Complexes and Combinatorial Ricci Curvature", Discrete & Computational Geometry, 29 (3): 323–374. doi:10.1007/s00454-002-0743-x. ISSN 1432-0444
Galloway, Gregory (2000), "Maximum Principles for Null Hypersurfaces and Null Splitting Theorems", Annales de l'Institut Henri Poincaré A, 1 (3): 543–567, arXiv:math/9909158, Bibcode:2000AnHP....1..543G, doi:10.1007/s000230050006, S2CID 9619157.
Kobayashi, S.; Nomizu, K. (1963), Foundations of Differential Geometry, Volume 1, Interscience.
Kobayashi, Shoshichi; Nomizu, Katsumi (1996), Foundations of Differential Geometry, Vol. 2, Wiley-Interscience, ISBN 978-0-471-15732-8.
Lohkamp, Joachim (1994), "Metrics of negative Ricci curvature", Annals of Mathematics, Second Series, 140 (3), Annals of Mathematics: 655–683, doi:10.2307/2118620, ISSN 0003-486X, JSTOR 2118620, MR 1307899.
Moroianu, Andrei (2007), Lectures on Kähler geometry, London Mathematical Society Student Texts, vol. 69, Cambridge University Press, arXiv:math/0402223, doi:10.1017/CBO9780511618666, ISBN 978-0-521-68897-0, MR 2325093, S2CID 209824092
Nomizu, Katsumi; Sasaki, Takeshi (1994), Affine differential geometry, Cambridge University Press, ISBN 978-0-521-44177-3.
Ollivier, Yann (2009), "Ricci curvature of Markov chains on metric spaces", Journal of Functional Analysis 256 (3): 810–864. doi:10.1016/j.jfa.2008.11.001. ISSN 0022-1236
Ricci, G. (1903–1904), "Direzioni e invarianti principali in una varietà qualunque", Atti R. Inst. Veneto, 63 (2): 1233–1239.
L.A. Sidorov (2001) [1994], "Ricci tensor", Encyclopedia of Mathematics, EMS Press
L.A. Sidorov (2001) [1994], "Ricci curvature", Encyclopedia of Mathematics, EMS Press
Najman, Laurent and Romon, Pascal (2017): Modern approaches to discrete curvature, Springer (Cham), Lecture notes in mathematics




External links


Z. Shen, C. Sormani "The Topology of Open Manifolds with Nonnegative Ricci Curvature" (a survey)
G. Wei, "Manifolds with A Lower Ricci Curvature Bound" (a survey)

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