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.

- Definition
- Introduction and local definition
- Definition via local coordinates on a smooth manifold
- Definition via differentiation of vector fields
- Comparison of the definitions
- Properties
- Informal properties
- Direct geometric meaning
- Applications
- Global geometry and topology
- Behavior under conformal rescaling
- Trace-free Ricci tensor
- The orthogonal decomposition of the Ricci tensor
- The trace-free Ricci tensor and Einstein metrics
- Kähler manifolds
- Generalization to affine connections
- Discrete Ricci curvature
- See also
- Footnotes
- References
- External links

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).^{ [1] } 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 Grigory 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.^{ [2] } This established a deep link between Ricci curvature and Wasserstein geometry and optimal transport, which is presently the subject of much research.^{[ citation needed ]}

The first subsection here is meant as an indication of the definition of the Ricci tensor for readers who are comfortable with linear algebra and multivariable calculus. The later subsections use more sophisticated terminology.

Let *U* be an open subset of ℝ^{n}, and for each pair of numbers i and j between 1 and n, let *g*_{ij} : *U* → ℝ be a smooth function, subject to the condition that, for each p in U, the matrix

is symmetric and invertible. For each p in U, let [*g*^{ij}(*p*)] be the inverse of the above matrix [*g*_{ij}(*p*)]. The functions *R*_{ij} are defined explicitly by the following formulae:

It can be seen directly from inspection of this formula that *R*_{ij} must equal *R*_{ji} for any i and j. So one can view the functions *R*_{ij} as associating to any point p of U a symmetric *n* × *n* matrix. This matrix-valued map on U is called the **Ricci curvature** associated to the collection of functions *g*_{ij}.

As presented, there is nothing intuitive or natural about the definition of Ricci curvature. It is singled out as an object for study only because it satisfies the following remarkable property. Let *V* ⊂ ℝ^{n} be another open set and let *y* : *V* → *U* be a smooth map whose matrix of first derivatives

is invertible for any choice of *q* ∈ *V*. Define *g*_{ij} : *V* → ℝ by the matrix product

One can compute, using the product rule and the chain rule, the following relationship between the Ricci curvature of the collection of functions g_{ij} and the Ricci curvature of the collection of functions *g*_{ij}: for any q in V, one has

This is quite unexpected since, directly plugging the formula which defines *g*_{ij} into the formula defining *R*_{ij}, one sees that one will have to consider up to third derivatives of y, arising when the second derivatives in the first four terms of the definition of *R*_{ij} act upon the components of J. The "miracle" is that the imposing collection of first derivatives, second derivatives, and inverses comprising the definition of the Ricci curvature is perfectly set up so that all of these higher derivatives of y cancel out, and one is left with the remarkably clean matrix formula above which relates *R*_{ij} and *R*_{ij}. It is even more remarkable that this cancellation of terms is such that the matrix formula relating *R*_{ij} to *R*_{ij} is identical to the matrix formula relating *g*_{ij} to *g*_{ij}.

With the use of some sophisticated terminology, the definition of Ricci curvature can be summarized as saying:

Let U be an open subset of ℝ

^{n}. Given a smooth mapping g on U which is valued in the space of invertible symmetricn×nmatrices, one can define (by a complicated formula involving various partial derivatives of the components of g) the Ricci curvature of g to be a smooth mapping from U into the space of symmetricn×nmatrices.

The remarkable and unexpected property of Ricci curvature can be summarized as:

Let J denote the Jacobian matrix of a diffeomorphism y from some other open set V to U. The Ricci curvature of the matrix-valued function given by the matrix product

J^{T}(g∘y)Jis given by the matrix productJ^{T}(R∘y)J, where R denotes the Ricci curvature of g.

In mathematics, this property is referred to by saying that the Ricci curvature is a "tensorial quantity", and marks the formula defining Ricci curvature, complicated though it may be, as of outstanding significance in the field of differential geometry.^{ [3] } In physical terms, this property is a manifestation of "general covariance" and is a primary reason that Albert Einstein made use of the formula defining *R*_{ij} when formulating general relativity. In this context, the possibility of choosing the mapping y amounts to the possibility of choosing between reference frames; the "unexpected property" of the Ricci curvature is a reflection of the broad principle that the equations of physics do not depend on reference frame.

This is discussed from the perspective of differentiable manifolds in the following subsection, although the underlying content is virtually identical to that of this subsection.

Let (*M*, *g*) be a smooth Riemannian or pseudo-Riemannian n-manifold. Given a smooth chart (*U*, * *) one then has functions *g*_{ij} : (*U*) → ℝ and *g*^{ij} : (*U*) → ℝ for each i and j between 1 and n which satisfy

for all x in (*U*). The functions *g*_{ij} are defined by evaluating g on coordinate vector fields, while the functions *g*^{ij} are defined so that, as a matrix-valued function, they provide an inverse to the matrix-valued function *x* ↦ *g*_{ij}(*x*).

Now define, for each a, b, c, i, and j between 1 and n, the functions

Now let (*U*, * *) and (*V*, ψ) be two smooth charts for which U and V have nonempty intersection. Let *R*_{ij} : (*U*) → ℝ be the functions computed as above via the chart (*U*, * *) and let *r*_{ij} : ψ(*V*) → ℝ be the functions computed as above via the chart (*V*, ψ). Then one can check by a calculation with the chain rule and the product rule that

This shows that the following definition does not depend on the choice of (*U*, * *). For any p in U, define a bilinear map Ric_{p} : *T _{p}M* ×

where *X*^{1}, ..., *X*^{n} and *Y*^{1}, ..., *Y*^{n} are the components of X and Y relative to the coordinate vector fields of (*U*, * *).

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

Let M be a smooth manifold, and let g be a Riemannian or pseudo-Riemannian metric. In local smooth coordinates, define the Christoffel symbols

It can be directly checked that

so that

R_{ij}define a (0,2)-tensor field on M. In particular, if X and Y are vector fields on M then relative to any smooth coordinates one has

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.

Suppose that (*M*, *g*) is an n-dimensional Riemannian or pseudo-Riemannian manifold, equipped with its Levi-Civita connection ∇. The Riemann curvature of M is a map which takes smooth vector fields X, Y, and Z, and returns the vector field

on vector fields *X*, *Y*, *Z*. The crucial property of this mapping is that if X, Y, Z and X', Y', and Z' are smooth vector fields such that X and X' define the same element of some tangent space *T*_{p}*M*, and Y and Y' also define the same element of *T*_{p}*M*, and Z and Z' also define the same element of *T*_{p}*M*, then the vector fields *R*(*X*,*Y*)*Z* and *R*(*X*′,*Y*′)*Z*′ also define the same element of *T*_{p}*M*.

The implication is that the Riemann curvature, which is a priori a mapping with vector field inputs and a vector field output, can actually be viewed as a mapping with tangent vector inputs and a tangent vector output. That is, it defines for each p in M a (multilinear) map

Define for each p in M the map by

That is, having fixed Y and Z, then for any basis *v*_{1}, ..., *v*_{n} of the vector space *T*_{p}*M*, one defines

where for any fixed i the numbers *c*_{i1}, ..., *c*_{in} are the coordinates of Rm_{p}(*v*_{i},*Y*,*Z*) relative to the basis *v*_{1}, ..., *v*_{n}. 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}.

**Sign conventions.** Note that some sources define to be what would here be called they would then define as Although sign conventions differ about the Riemann tensor, they do not differ about the Ricci tensor.

The two above definitions are identical. The formulas defining and 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 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.

Note also that the complicated formula defining 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

As can be seen from the Bianchi identities, the Ricci tensor of a Riemannian manifold is symmetric, in the sense that

for all It thus follows linear-algebraically that the Ricci tensor is completely determined by knowing the quantity Ric(*X*,*X*) for all vectors 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 is a vector of unit length on a Riemannian n-manifold, then Ric(*ξ*,*ξ*) is precisely (*n* − 1) times the average value of the sectional curvature, taken over all the 2-planes containing ξ. There is an (*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

where is the scalar curvature, defined in local coordinates as This is often called the contracted second Bianchi identity.

The Ricci curvature is sometimes thought of as (a negative multiple of) the Laplacian of the metric tensor ( Chow & Knopf 2004 , Lemma 3.32) . Specifically, in harmonic local coordinates the components satisfy

where is the Laplace–Beltrami operator, here regarded as acting on the locally-defined functions g_{ij}. This fact motivates, for instance, the introduction of the Ricci flow equation as a natural extension of the heat equation for the metric. Alternatively, in a normal coordinate system based at p, at the point p

Near any point p in a Riemannian manifold (*M*, *g*), one can define preferred local coordinates, called geodesic normal coordinates. These are adapted to the metric so that geodesics through p correspond to straight lines through the origin, in such a manner that the geodesic distance from 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

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

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

which follows by expanding the square root of the determinant of the metric.

Thus, if the Ricci curvature Ric(*ξ*,*ξ*) is positive in the direction of a vector ξ, the conical region in M swept out by a tightly focused family of geodesic segments of length emanating from p, with initial velocity inside a small cone about ξ, will have smaller volume than the corresponding conical region in Euclidean space, at least provided that is sufficiently small. Similarly, if the Ricci curvature is negative in the direction of a given vector ξ, 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. 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. 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.

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, where certain one-parameter families of Riemannian metrics are singled out as solutions of a geometrically-defined partial differential equation. This system of equations can be thought of as a geometric analog of the heat equation, and was first introduced by Richard S. Hamilton in 1982. 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 much 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.

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*) is positive on the set of non-zero tangent vectors ξ.) 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, then the manifold has diameter ≤ π/√*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. - The Bishop–Gromov inequality states that if a complete 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-space. Moreover, if
*v*(_{p}*R*) denotes the volume of the ball with center p and radius R in the manifold and*V*(*R*) =*c*denotes the volume of the ball of radius R in Euclidean n-space then the function_{n}R^{n}*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)*with Ric ≥ 0 contains a*line*, meaning a geodesic such that*d*(*γ*(*u*),*γ*(*v*)) = |*u*−*v*| for all*u*,*v*∈ ℝ, then it is isometric to a product space ℝ ×*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 (+ − − ...)) 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.

If the metric g is changed by multiplying it by a conformal factor *e*^{2f}, the Ricci tensor of the new, conformally-related metric *g̃* = *e*^{2f}*g* is given ( Besse 1987 , p. 59) by

where Δ = *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 in a Riemannian manifold, it is always possible to find metrics conformal to the given metric g for which the Ricci tensor vanishes at 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 is a harmonic function, then the conformal scaling *g* ↦ *e*^{2f}*g* does not change the Ricci tensor (although it still changes its trace with respect to the metric unless *f* = 0).

In Riemannian geometry and pseudo-Riemannian geometry, the **trace-free Ricci tensor** (also called **traceless Ricci tensor**) of a Riemannian or pseudo-Riemannian *n*-manifold (*M*, *g*) is the tensor defined by

where Ric and R denote the Ricci curvature and scalar curvature of g. The name of this object reflects the fact that its trace automatically vanishes: However, it is quite an important tensor since it reflects an "orthogonal decomposition" of the Ricci tensor.

Trivially, one has

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

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

By taking a divergence, and using the contracted Bianchi identity, one sees that implies So, provided that *n* ≥ 3 and is connected, the vanishing of implies that the scalar curvature is constant. One can then see that the following are equivalent:

- for some number

In the Riemannian setting, the above orthogonal decomposition shows that is also equivalent to these conditions. In the pseudo-Riemmannian setting, by contrast, the condition does not necessarily imply so the most that one can say is that these conditions imply

In particular, the vanishing of trace-free Ricci tensor characterizes Einstein manifolds, as defined by the condition for a number In general relativity, this equation states that (*M*, *g*) is a solution of Einstein's vacuum field equations with cosmological constant.

On a Kähler manifold 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:

The Levi-Civita connection corresponding to the metric on X gives rise to a connection on κ. The curvature of this connection is the two form defined by

where 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 (for compact X) in the sense that it depends only on the topology of X and the homotopy class of the complex structure.

Conversely, the Ricci form determines the Ricci tensor by

In local holomorphic coordinates z^{α}, the Ricci form is given by

where ∂ is the Dolbeault operator and

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 SL(*n*,**C**). However, Kähler manifolds already possess holonomy in U(*n*), and so the (restricted) holonomy of a Ricci-flat Kähler manifold is contained in SU(*n*). Conversely, if the (restricted) holonomy of a 2*n*-dimensional Riemannian manifold is contained in SU(*n*), then the manifold is a Ricci-flat Kähler manifold ( Kobayashi & Nomizu 1996 , IX, §4).

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 ∇ denotes an affine connection, then the curvature tensor R is the (1,3)-tensor defined by

for any vector fields *X*, *Y*, *Z*. The Ricci tensor is defined to be the trace:

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

Notions of Ricci curvature on discrete manifolds have been defined on graphs and networks, where they quantify local divergence properties of edges. Olliver's Ricci curvature is defined using optimal transport theory.^{[ citation needed ]} A second notion, Forman's Ricci curvature, is based on topological arguments.^{[ citation needed ]}

- ↑ Here it is assumed that the manifold carries its unique Levi-Civita connection. For a general affine connection, the Ricci tensor need not be symmetric.
- ↑ Lott, John; Villani, Cedric (2006-06-23). "Ricci curvature for metric-measure spaces via optimal transport". arXiv: math/0412127 .
- ↑ To be precise, there are many tensorial quantities in differential geometry. What makes the Ricci curvature (as well as other curvature quantities such as the Riemann curvature tensor) special is not the collection of functions of functions
*R*_{ij}itself, which is in principle "just one of many tensors," but is rather the automatic passage from one tensorial quantity (the collection of functions g) to a new tensorial quantity (the collection of functions R).

In physics, **Kaluza–Klein theory** is a classical unified field theory of gravitation and electromagnetism built around the idea of a fifth dimension beyond the common 4D of space and time and considered an important precursor to string theory. Gunnar Nordström had an earlier, similar idea. But in that case, a fifth component was added to the electromagnetic vector potential, representing the Newtonian gravitational potential, and writing the Maxwell equations in five dimensions.

In the mathematical field of differential geometry, the **Riemann curvature tensor** or **Riemann–Christoffel tensor** is the most common way used to express the curvature of Riemannian manifolds. It assigns a tensor to each point of a Riemannian manifold. It is a local invariant of Riemannian metrics which measure the failure of second covariant derivatives to commute. A Riemannian manifold has zero curvature if and only if it is *flat*, i.e. locally isometric to the Euclidean space. The curvature tensor can also be defined for any pseudo-Riemannian manifold, or indeed any manifold equipped with an affine connection.

In differential geometry, a **Riemannian manifold** or **Riemannian space**(*M*, *g*) is a real, smooth manifold *M* equipped with a positive-definite inner product *g*_{p} on the tangent space *T*_{p}*M* at each point *p*. A common convention is to take *g* to be smooth, which means that for any smooth coordinate chart (*U*, *x*) on *M*, the *n*^{2} functions

In Riemannian geometry, the **sectional curvature** is one of the ways to describe the curvature of Riemannian manifolds with dimension greater than 2. The sectional curvature *K*(σ_{p}) depends on a two-dimensional linear subspace σ_{p} of the tangent space at a point *p* of the manifold. It can be defined geometrically as the Gaussian curvature of the surface which has the plane σ_{p} as a tangent plane at *p*, obtained from geodesics which start at *p* in the directions of σ_{p}. The sectional curvature is a real-valued function on the 2-Grassmannian bundle over the manifold.

In Riemannian geometry, the **scalar curvature** is the simplest curvature invariant of a Riemannian manifold. To each point on a Riemannian manifold, it assigns a single real number determined by the intrinsic geometry of the manifold near that point. Specifically, the scalar curvature represents the amount by which the volume of a small geodesic ball in a Riemannian manifold deviates from that of the standard ball in Euclidean space. In two dimensions, the scalar curvature is twice the Gaussian curvature, and completely characterizes the curvature of a surface. In more than two dimensions, however, the curvature of Riemannian manifolds involves more than one functionally independent quantity.

In the mathematical field of differential geometry, the **Ricci flow**, sometimes also referred to as **Hamilton's Ricci flow**, is a certain partial differential equation for a Riemannian metric. It is often said to be analogous to the diffusion of heat and the heat equation, due to formal similarities in the mathematical structure of the equation; however, it exhibits many phenomena not present in the study of the heat equation. Many results for Ricci flow have also been shown for the mean curvature flow of hypersurfaces.

In mathematics and especially differential geometry, a **Kähler manifold** is a manifold with three mutually compatible structures: a complex structure, a Riemannian structure, and a symplectic structure. The concept was first studied by Jan Arnoldus Schouten and David van Dantzig in 1930, and then introduced by Erich Kähler in 1933. The terminology has been fixed by André Weil.

In mathematics, specifically differential geometry, the infinitesimal geometry of Riemannian manifolds with dimension greater than 2 is too complicated to be described by a single number at a given point. Riemann introduced an abstract and rigorous way to define curvature for these manifolds, now known as the Riemann curvature tensor. Similar notions have found applications everywhere in differential geometry.

In differential geometry, the **Weyl curvature tensor**, named after Hermann Weyl, is a measure of the curvature of spacetime or, more generally, a pseudo-Riemannian manifold. Like the Riemann curvature tensor, the Weyl tensor expresses the tidal force that a body feels when moving along a geodesic. The Weyl tensor differs from the Riemann curvature tensor in that it does not convey information on how the volume of the body changes, but rather only how the shape of the body is distorted by the tidal force. The Ricci curvature, or trace component of the Riemann tensor contains precisely the information about how volumes change in the presence of tidal forces, so the Weyl tensor is the traceless component of the Riemann tensor. It is a tensor that has the same symmetries as the Riemann tensor with the extra condition that it be trace-free: metric contraction on any pair of indices yields zero.

In differential geometry, the **Cotton tensor** on a (pseudo)-Riemannian manifold of dimension *n* is a third-order tensor concomitant of the metric, like the Weyl tensor. The vanishing of the Cotton tensor for *n* = 3 is necessary and sufficient condition for the manifold to be conformally flat, as with the Weyl tensor for *n* ≥ 4. For *n* < 3 the Cotton tensor is identically zero. The concept is named after Émile Cotton.

In differential geometry, the **Laplace–Beltrami operator** is a generalization of the Laplace operator to functions defined on submanifolds in Euclidean space and, even more generally, on Riemannian and pseudo-Riemannian manifolds. It is named after Pierre-Simon Laplace and Eugenio Beltrami.

In the mathematical fields of Riemannian and pseudo-Riemannian geometry, the **Ricci decomposition** is a way of breaking up the Riemann curvature tensor of a Riemannian or pseudo-Riemannian manifold into pieces with special algebraic properties. This decomposition is of fundamental importance in Riemannian and pseudo-Riemannian geometry.

In mathematics, the **Fubini–Study metric** is a Kähler metric on projective Hilbert space, that is, on a complex projective space **CP**^{n} endowed with a Hermitian form. This metric was originally described in 1904 and 1905 by Guido Fubini and Eduard Study.

In the mathematical field of differential geometry, the **Kulkarni–Nomizu product** is defined for two (0, 2)-tensors and gives as a result a (0, 4)-tensor.

In the mathematical field of differential geometry, a smooth map from one Riemannian manifold to another Riemannian manifold is called **harmonic** if its coordinate representatives satisfy a certain nonlinear partial differential equation. This partial differential equation for a mapping also arises as the Euler-Lagrange equation of a functional generalizing the Dirichlet energy. As such, the theory of harmonic maps encompasses both the theory of unit-speed geodesics in Riemannian geometry, and the theory of harmonic functions on open subsets of Euclidean space and on Riemannian manifolds.

In Riemannian geometry, the **Schouten tensor** is a second-order tensor introduced by Jan Arnoldus Schouten. It is defined for *n* ≥ 3 by:

In Riemannian geometry, a branch of mathematics, **harmonic coordinates** are a certain kind of coordinate chart on a smooth manifold, determined by a Riemannian metric on the manifold. They are useful in many problems of geometric analysis due to their regularity properties.

The **Yamabe problem** refers to a conjecture in the mathematical field of differential geometry, which was resolved in the 1980s. It is a statement about the scalar curvature of Riemannian manifolds:

Let (

M,g) be a closed smooth Riemannian manifold. Then there exists a positive and smooth function f on M such that the Riemannian metricfghas constant scalar curvature.

In Riemannian geometry, **Schur's lemma** is a result that says, heuristically, whenever certain curvatures are pointwise constant then they are forced to be globally constant. The proof is essentially a one-step calculation, which has only one input: the second Bianchi identity.

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