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Tensoriality of the curvature, its coordinate formula and its point-normal metric formula
Statement
Let be a time-oriented smooth Lorentzian four-manifold with metric-selected connection (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields), and let be the curvature operator of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, with components in a chart.
(a) Tensoriality. For all smooth functions on and smooth vector fields on a common domain, and Consequently, for every , the value depends only on , and is a smooth tensor field of type on whose components in every smooth chart are the functions of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (b).
(b) Coordinate formula. In every smooth chart with Christoffel symbols of (Christoffel symbols of an affine connection), on , for all .
(c) Point-normal formula. If the chart is point-normal at , that is , and (Point-normal and exponential coordinate charts of the metric-selected connection), then, writing , Equivalently, .
Facts & Assumptions
Given: A time-oriented smooth Lorentzian four-manifold with metric-selected connection , its curvature operator , a chart , and a point with a point-normal chart as in the claims.
All field calculations below are made on a common open domain , using the restriction of the connection to local fields there. The function-linearity identities are proved for every ; the Statement's global smooth functions are their restrictions, and step 3.1 uses these same local identities for its chart coefficient functions.
The curvature operator is for smooth fields, is a smooth field, and its components in a chart are defined by (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors).
On every common open domain , the restricted affine connection is real bilinear on local fields, function-linear in its first argument, satisfies for , and takes smooth local fields to smooth local fields (Affine connection on a smooth manifold).
On every common open domain , the Lie bracket satisfies and for , , and for coordinate fields (The Lie bracket of smooth vector fields, Coordinate formula for the Lie bracket).
In a chart, , and torsion freedom of gives (Christoffel symbols of an affine connection, Torsion freedom and metric compatibility in chart components clauses 1, Metric compatibility, torsion freedom and the metric-selected connection class).
The Christoffel symbols of the metric-selected connection satisfy in every chart, and (Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields clause (a), The inverse metric, musical isomorphisms and index raising).
For every there is a smooth chart with , and (Point-normal and exponential coordinate charts of the metric-selected connection clause (a)).
A smooth vector field on a chart domain is a finite sum with smooth coefficients , and vanishes at a point whenever every does (Coordinate derivations form a basis of the tangent space).
Mixed partial derivatives of a smooth function commute (Clairaut--Schwarz theorem for continuous second partial derivatives).
A smooth tensor field of type is a family of multilinear maps with components in every chart (Tensor fields of type (r,s) on a Lorentzian four-manifold and their components clauses (a)-(b)).
Proof
(Function-linearity in the first slot.) Let be smooth. Using [L3] for the bracket and [L2] for the connection, , the two terms cancelling.
(Function-linearity in the third slot.) Expanding with [L2] and [L3], , while , and . Subtracting the second and third displays from the first, the , and -coefficient terms cancel in pairs and the remaining scalar coefficient is by definition of the bracket, so .
(Skew-symmetry and the second slot.) Directly from [L1] and , ; combining this with step 1.1, .
(Pointwise dependence.) Let and let be a chart around . By [L7], fields with , , have the form , , on a possibly smaller chart neighborhood, with . By additivity of in each field argument and the three function-linearity steps, expanding yields plus a finite sum of terms each carrying at least one of the smooth coefficients (a term with such factors expands, by steps 1.1, 2.1 and 1.2, into -fold products of coefficients times evaluated on coordinate fields). Every such term vanishes at because all coefficients do, so : the value depends only on the pointwise data.
(Smooth tensor field.) By step 3.1 the assignment descends to a map , for any smooth local extensions, which is -multilinear because the field-level assignment is additive over and function-linear. In a chart, is a smooth field by [L1], so its coefficients in the coordinate frame are functions on the chart domain. By [L9] these data constitute a smooth tensor field of type whose components are exactly . This proves (a).
(Coordinate formula.) In the chart, [L3] gives , so [L1] gives . By [L4], , so [L2] gives ; exchanging and subtracting yields . This proves (b).
(Point-normal derivative of the Christoffel symbols.) In the point-normal chart of [L6], differentiate the Christoffel formula of [L5]. The derivative of the factor multiplies the bracket , which vanishes at because , so only the bracket's derivative survives: , and likewise . Since , formula (b) of step 5.1 reduces at to the difference of these two derivatives, in which the terms and agree by [L8] and cancel: .
(Lowering and final form.) Lowering the first index with [L5], . Using [L8] to commute the mixed partials and the symmetry , of the metric, this is , and raising back with recovers the equivalent raised display. This proves (c) and completes the proof.
Remarks
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What is used where. Clause (a) uses only the connection rules and the bracket identity; the coordinate formula (b) uses in addition the symmetry of the Christoffel symbols, which is torsion freedom; the point-normal formula (c) uses the Christoffel formula, that is metric compatibility and nondegeneracy. No positive-definite or Riemannian hypothesis is used anywhere. The result is stated for a Lorentzian metric only because that is the ambient framework; the computation is signature-independent.
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Tensoriality of is not claimed. The formula of (b) contains the non-tensorial chart functions , but its left-hand side is tensorial by (a); this is exactly why (b) cannot be used to conclude that vanishing of at a point implies vanishing of curvature. Clause (c) shows that curvature is precisely the second-order metric information that a point-normal chart cannot remove.
Depends on
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Metric compatibility, torsion freedom and the metric-selected connection class
Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
Affine connection on a smooth manifold
The Lie bracket of smooth vector fields
Coordinate formula for the Lie bracket
Christoffel symbols of an affine connection
Torsion freedom and metric compatibility in chart components
The inverse metric, musical isomorphisms and index raising
Point-normal and exponential coordinate charts of the metric-selected connection
Coordinate derivations form a basis of the tangent space
Clairaut--Schwarz theorem for continuous second partial derivatives
Tensor fields of type (r,s) on a Lorentzian four-manifold and their components
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 3: the commutator [nabla_mu,nabla_nu]V^rho, the Riemann tensor (3.65)-(3.67), and its evaluation in Riemann normal coordinates, printed pp. 75-77 and 79-80 (PDF pp. 82-84 and 86-87)
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision), section 4.4 and equation (4.29): the Riemann tensor in normal coordinates, R_{mu nu rho sigma} = (1/2)(g_{mu sigma,nu rho}+g_{nu rho,mu sigma}-g_{nu sigma,mu rho}-g_{mu rho,nu sigma}) at p, printed pp. 45-49 (PDF pp. 46-50)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), sections 3.3.2 and 3.4: the Riemann tensor (3.39) and its normal-coordinate form, printed pp. 119-121 and 130 (PDF pp. 126-128 and 137)