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First-order curvature of the diagonal perturbation h_00 = -2 phi, h_ij = -2 phi delta_ij for the explicit potential phi = |x|^2/2
Example
Work on the flat model of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart with its inertial chart and take for the open unit ball of (identified with its image under ). Take the flat linearized family of Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge with normalized remainder and first-order perturbation
so that . Then with and is a flat linearized family over , and with all indices raised and lowered by :
- , and , while and ; here , and range over .
- , , and .
- The trace-reversed perturbation is , , , and the closed formula of First-order curvature of a flat linearized family, gauge transformations and the quadratic remainder clause (c) gives and ; these values satisfy with the tensors of clause 2, as the first-order expansion of (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors) requires.
Facts & Assumptions
Given: The flat model with inertial chart , the open unit ball , the potential above, and the flat linearized family with , and the component fields , , .
A flat linearized family over consists of and smooth fields , such that for the field is the component field of a smooth Lorentzian metric of signature on (Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge clause (a)).
Indices on first-order quantities are raised and lowered with : , , , , (Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge clause (c), The inverse metric, musical isomorphisms and index raising).
First-order formulas (First-order curvature of a flat linearized family, gauge transformations and the quadratic remainder clauses (a)-(c)): ; ; ; ; here .
For on : , and (The Laplacian of a function and of a vector field). The field has -independent components, so for every component field that is stationary (independent of ) the d'Alembertian reduces to the Laplacian, ; in particular and . The components of are stationary.
If a symmetric bilinear form on a four-dimensional real vector space has, in some basis, the matrix with for all , then it has inertia (Lorentzian metrics are stable under small compactly supported symmetric perturbations clause (a)).
Verification
(Admissibility.) In the coordinate frame the components of are , and otherwise, so the matrix of in the coordinate basis is with , the entries of which satisfy on , because there; all components are stationary and smooth, so is a smooth symmetric component field. By [L5] has inertia for every , and is smooth; hence satisfies clause (a) of [L1].
(First-order connection.) By [L2] and [L3], . The time derivatives vanish and , so . Similarly and because the spatial components vanish and . For the spatial pairs . For the components with upper index , , since is nonzero only at : for and for both spatial this vanishes ( for spatial and all component time derivatives vanish), while .
(Trace data.) By [L2], , and the mixed components are , , and .
(First-order Ricci tensor.) By [L3] and step 1.3: for the component, because all components of are stationary, and (the field is stationary), so . For the component, and because the fields are stationary and vanishes for and is stationary for ; and because and is stationary; so . For the component, , likewise , and , so .
(Scalar curvature.) By [L3] and [L2], , since , , and all time derivatives vanish; and . Hence . As an arithmetic check on the defining relation of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, whose first-order expansion at is because : the values of step 2.1 give , in agreement.
(Einstein tensor and cross-check.) By [L2] the trace reversal of step 1.3 is , and ; that is, . The closed formula of [L3] then gives: for , and by stationarity, so ; for and every term of the closed formula involves a component or a time derivative, hence vanishes, so . Finally, the values satisfy : for , for and for , which is the first-order expansion at of the defining relation of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, using and .
Depends on
The flat model spacetime: the Minkowski metric on R^4 and its inertial chart
Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge
First-order curvature of a flat linearized family, gauge transformations and the quadratic remainder
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
The inverse metric, musical isomorphisms and index raising
The Laplacian of a function and of a vector field
Lorentzian metrics are stable under small compactly supported symmetric perturbations
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 4 equations (4.12)-(4.21) and (4.48)-(4.52), printed pp. 105-112: Newtonian time-time potential and Poisson limit; Ch. 6 equations (6.4)-(6.8), (6.13)-(6.22) and (6.24)-(6.29), printed pp. 142-148: first-order curvature, gauge, trace reversal and diagonal weak-field metric
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 5.1.1: the first-order curvature of the stationary diagonal weak-field metric, printed pp. 205-208 (PDF pp. 212-215)