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Ricci, scalar and Einstein tensors of the FLRW metric in product charts
Statement
Let be an FLRW model datum with conversion constant , with spacetime and metric (FLRW model data: warped product metric, cosmic time, comoving congruence, scale factor and Hubble parameter, The constant-curvature spatial model of a homogeneous cosmology), let be its metric-selected connection, and let , , and be the curvature components, Ricci tensor, scalar curvature and Einstein tensor of (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, Tensoriality of the curvature, its coordinate formula and its point-normal metric formula, Metric compatibility, torsion freedom and the metric-selected connection class). In a product chart with , with the derivative of the scale factor and :
(a) , , and for ;
(b) ;
(c) , , and for .
All displayed component functions are smooth on the chart domain; the identities are equalities of the components of the respective tensor fields in the product chart and hold at every point.
Facts & Assumptions
Given: An FLRW model datum with , its spacetime, metric, connection , curvature data and a product chart with .
In the product chart the Christoffel symbols are , , and , where are the symbols of the spatial metric (Christoffel symbols of the FLRW metric in product charts).
The curvature components are given by , and is a smooth -tensor whose curvature data are independent of the chart used (Tensoriality of the curvature, its coordinate formula and its point-normal metric formula clause (b), The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors).
with ; equivalently, in every orthonormal frame , which is the trace of the curvature endomorphism (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (c), Ricci curvature, Ricci curvature is symmetric and basis independent, The inverse metric, musical isomorphisms and index raising). Moreover and (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (c)).
The remaining components of the inverse metric in the product chart are and , and (Christoffel symbols of the FLRW metric in product charts [L2], The inverse metric, musical isomorphisms and index raising).
The spatial metric has constant sectional curvature , so its three-dimensional Ricci tensor is ; in the component convention shared with [L2] this reads , where are the curvature components of computed from the symbols (Constant-curvature three-manifolds: equivalence of constant sectional curvature, the tensor identity and the Ricci condition, Ricci curvature, Riemannian metric and riemannian manifold).
is the derivative of the smooth function of , , its second derivative, and for in the product chart (FLRW model data: warped product metric, cosmic time, comoving congruence, scale factor and Hubble parameter, The derivative of at a point that is a limit point of , and differentiability on a set).
Proof
(The component.) By [L3], . In the sum, the term is because every term of [L2] contains a symbol or , all of which vanish by [L1]. For the same formula gives , using and from [L1]; the remaining quadratic term is , because the terms with contain the vanishing symbol . Summing over gives , where by [L6].
(The spatial components.) By [L3], . For the term , [L2] and [L1] give , since and for ; with and this is . For the spatial terms, substituting [L1] into [L2] and summing over separates the -symbols from the time-dependent symbols exactly as in the third family of Christoffel symbols of the FLRW metric in product charts: the terms with some index contribute the total , and the remaining terms are by [L5]. Adding the two contributions gives , which is claim (a).
(The mixed components vanish.) By [L3], . The term vanishes as in step 1.1. For , [L2] and [L1] give , since the terms with contain and the spatial derivatives of the functions vanish; substituting and and summing over gives by the symmetry of the spatial symbols. Hence .
(Scalar curvature.) By [L3] and [L4], . Using by [L4], , since and by [L6]. This is claim (b).
(Einstein tensor and conclusion.) By [L3] and [L4], by step 2.2; by step 2.1; and by steps 1.2 and 2.2. This is claim (c), and it completes the proof of all three claims.
Remarks
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Conventions. The curvature sign convention is the one fixed by The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors and Tensoriality of the curvature, its coordinate formula and its point-normal metric formula: and . With this convention the round unit two-sphere has positive Ricci curvature and the spatial constant gives , as recorded in Constant-curvature three-manifolds: equivalence of constant sectional curvature, the tensor identity and the Ricci condition. Other sources order the loop indices differently; no formula of another source is used here without checking it against this convention.
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Flat check. For and the Euclidean metric the spatial symbols vanish, so steps 1.1-1.3 reduce to the textbook flat-slice expressions; the derivation covers this case without extra hypotheses and displays the -dependence explicitly.
Depends on
FLRW model data: warped product metric, cosmic time, comoving congruence, scale factor and Hubble parameter
The constant-curvature spatial model of a homogeneous cosmology
Christoffel symbols of the FLRW metric in product charts
The FLRW metric is smooth Lorentzian; the comoving field is unit timelike and cosmic time parametrizes comoving curves by proper time; the slices carry the scaled spatial metric
Constant-curvature three-manifolds: equivalence of constant sectional curvature, the tensor identity and the Ricci condition
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Tensoriality of the curvature, its coordinate formula and its point-normal metric formula
The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors
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
Christoffel symbols of an affine connection
The inverse metric, musical isomorphisms and index raising
Smooth covariant 2-tensor fields on a smooth manifold
Ricci curvature
Ricci curvature is symmetric and basis independent
Riemannian metric and riemannian manifold
The derivative of at a point that is a limit point of , and differentiability on a set
The Axiom of Countable Choice ()
Dependency tree · 2 levels
Sources
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 4.6.1: R_00 = -3 a-double-dot/a, R_0i = 0, R_ij = (a-double-dot/a + 2(a-dot/a)^2 + 2k/a^2)g_ij, the Ricci scalar and the Einstein tensor components, printed pp. 200-201 (PDF pp. 207-208); section 4.6.2: the Friedmann and acceleration equations (4.66)-(4.67), printed pp. 202-203 (PDF pp. 209-210)
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 8 (8.32)-(8.36): the 00 and ij Einstein equations for the FRW metric and the resulting Friedmann equations, printed pp. 222-223 (PDF pp. 229-230)
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 3 (3.90)-(3.95): the Ricci tensor, Ricci scalar and Einstein tensor in a chart, printed pp. 81-82 (PDF pp. 88-89)