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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 x and take for Ω the open unit ball of R4 (identified with its image under x). Take the flat linearized family of Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge with normalized remainder q≡0 and first-order perturbation

h00=−2φ,hij=−2φ δij,h0i=0,φ(x):=12((x1)2+(x2)2+(x3)2),

so that g(λ)ab=ηab+λ hab. Then (ε1,h,q) with ε1:=1/8 and q≡0 is a flat linearized family over Ω, and with all indices raised and lowered by η:

  1. Γ(1)i00=xi, Γ(1)i0j=Γ(1)ij0=0 and Γ(1)ijk=−δki xj−δji xk+δjk xi, while Γ(1)000=Γ(1)0ij=0 and Γ(1)00i=Γ(1)0i0=xi; here xj:=δjmxm, and i,j,k range over 1,2,3.
  2. Ric⁡00(1)=3, Ric⁡0i(1)=0, Ric⁡ij(1)=3δij and S(1)=6.
  3. The trace-reversed perturbation is hˉ00=−4φ, hˉ0i=0, hˉij=0, and the closed formula of First-order curvature of a flat linearized family, gauge transformations and the quadratic remainder clause (c) gives G00(1)=2Δφ=6 and G0i(1)=Gij(1)=0; these values satisfy Gab(1)=Ric⁡ab(1)−12ηabS(1) with the tensors of clause 2, as the first-order expansion of G=Ric⁡−12Sg (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors) requires.

Facts & Assumptions

Given: The flat model (M,g,N) with inertial chart x, the open unit ball Ω⊆M, the potential φ above, and the flat linearized family (ε1,h,q) with ε1=1/8, q≡0 and the component fields h00=−2φ, h0i=0, hij=−2φδij.

[L1]

A flat linearized family over Ω consists of ε1>0 and smooth fields h, q such that for 0<∣λ∣<ε1 the field gab(λ,p)=ηab+λhab(p)+λ2qab(λ,p) is the component field of a smooth Lorentzian metric of signature (−,+,+,+) on Ω (Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge clause (a)).

[L2]

Indices on first-order quantities are raised and lowered with η: ∂a=ηab∂b, hab=ηacηbdhcd, □=ηab∂a∂b, h=ηabhab, hˉab=hab−12ηabh (Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge clause (c), The inverse metric, musical isomorphisms and index raising).

[L3]

First-order formulas (First-order curvature of a flat linearized family, gauge transformations and the quadratic remainder clauses (a)-(c)): Γ(1)abc=12ηad(∂bhcd+∂chbd−∂dhbc); Ric⁡ab(1)=12(∂c∂ahcb+∂c∂bhca−□hab−∂a∂bh); S(1)=∂a∂bhab−□h; Gab(1)=−12□hˉab+∂c∂(ahˉb)c−12ηab∂c∂dhˉcd; here hcb=ηcahab.

[L4]

For φ=12((x1)2+(x2)2+(x3)2) on Ω: ∂iφ=xi, ∂i∂jφ=δij and Δφ=3 (The Laplacian of a C2 function and of a C2 vector field). The field φ has x0-independent components, so for every component field f that is stationary (independent of x0) the d'Alembertian reduces to the Laplacian, □f=Δf; in particular □φ=3 and □xi=0. The components of h are stationary.

[L5]

If a symmetric bilinear form on a four-dimensional real vector space has, in some basis, the matrix diag⁡(−1,1,1,1)+E with ∣Eij∣<1/8 for all i,j, then it has inertia (3,1,0) (Lorentzian metrics are stable under small compactly supported symmetric perturbations clause (a)).

Verification

technique · direct; verify that the family is admissible, insert the explicit components into the first-order formulas of [L3], and cross-check the Einstein tensor through the trace-reversed closed formula of [L3] and through the first-order expansion of $G=\operatorname{Ric}-\tfrac12Sg$
1.1L1L5algebra

(Admissibility.) In the coordinate frame the components of λh are λh00=−2λφ, λhij=−2λφδij and 0 otherwise, so the matrix of g(λ)=η+λh in the coordinate basis is diag⁡(−1,1,1,1)+E(λ) with E(λ)=−2λφ I4, the entries of which satisfy ∣E(λ)ij∣=2∣λ∣ φ<2⋅18⋅12=18 on Ω, because φ<12 there; all components are stationary and smooth, so g(λ) is a smooth symmetric component field. By [L5] g(λ) has inertia (3,1,0) for every 0<∣λ∣<ε1, and q≡0 is smooth; hence (ε1,h,q) satisfies clause (a) of [L1].

1.2L2L3L4algebra

(First-order connection.) By [L2] and [L3], Γ(1)i00=12ηia(2∂0ha0−∂ah00). The time derivatives vanish and ∂ah00=−2∂aφ, so Γ(1)i00=ηia∂aφ=∂iφ=xi. Similarly Γ(1)i0j=12ηia(∂0haj+∂jha0−∂ah0j)=0 and Γ(1)ij0=0 because the spatial components hk0=h0k vanish and ηi0=0. For the spatial pairs Γ(1)ijk=12ηia(∂jhak+∂khaj−∂ahjk)=12δia(−2∂jφ δak−2∂kφ δaj+2∂aφ δjk)=−δkixj−δjixk+δjkxi. For the components with upper index 0, Γ(1)0bc=12η0a(∂bhca+∂chba−∂ahbc)=−12(∂bhc0+∂chb0−∂0hbc), since η0a is nonzero only at a=0: for (b,c)=(0,0) and for b,c both spatial this vanishes (hi0=0 for spatial i and all component time derivatives vanish), while Γ(1)00i=Γ(1)0i0=−12∂ih00=∂iφ=xi.

1.3L2algebra

(Trace data.) By [L2], h=ηabhab=η00h00+ηijhij=2φ−6φ=−4φ, and the mixed components hcb=ηcahab are h00=η00h00=2φ, hij=ηikhkj=−2φδji, h0i=η0ahai=0 and hi0=ηikhk0=0.

2.1step 1.3L2L3L4algebra

(First-order Ricci tensor.) By [L3] and step 1.3: for the (00) component, ∂c∂0hc0=0 because all components of hc0 are stationary, and −□h00−∂0∂0h=2□φ=2Δφ=6 (the field h is stationary), so Ric⁡00(1)=12(0+0+6+0)=3. For the (0i) component, ∂c∂0hci=0 and ∂c∂ihc0=0 because the fields hci are stationary and hc0 vanishes for c≠0 and is stationary for c=0; and □h0i=∂0∂ih=0 because h0i=0 and h is stationary; so Ric⁡0i(1)=0. For the (ij) component, ∂c∂ihcj=∂k∂i(−2φδjk)=−2δij, likewise ∂c∂jhci=−2δij, −□hij=2δijΔφ=6δij and −∂i∂jh=4∂i∂jφ=4δij, so Ric⁡ij(1)=12(−2−2+6+4)δij=3δij.

3.1step 2.1L2L3L4algebra

(Scalar curvature.) By [L3] and [L2], ∂a∂bhab=∂i∂jhij=∂i∂j(−2φδij)=−2Δφ=−6, since h00=−2φ, h0i=0, hij=−2φδij and all time derivatives vanish; and □h=□(−4φ)=−4Δφ=−12. Hence S(1)=−6+12=6. As an arithmetic check on the defining relation S=gabRic⁡ab of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, whose first-order expansion at λ=0 is S(1)=ηabRic⁡ab(1) because Ric⁡(0)=0: the values of step 2.1 give −Ric⁡00(1)+δijRic⁡ij(1)=−3+9=6, in agreement.

4.1step 1.3step 2.1step 3.1L2L3L4algebra∎

(Einstein tensor and cross-check.) By [L2] the trace reversal of step 1.3 is hˉ00=h00−12η00h=−2φ−12(−1)(−4φ)=−4φ, hˉij=−2φδij−12δij(−4φ)=0 and hˉ0i=0; that is, hˉab=−4φ δa0δb0. The closed formula of [L3] then gives: for (00), ∂c∂dhˉcd=η00η00∂0∂0hˉ00=0 and ∂c∂(0hˉ0)c=0 by stationarity, so G00(1)=−12□(−4φ)=2Δφ=6; for (0i) and (ij) every term of the closed formula involves a component hˉ0⋅ or a time derivative, hence vanishes, so G0i(1)=Gij(1)=0. Finally, the values satisfy Gab(1)=Ric⁡ab(1)−12ηabS(1): 3−12(−1)(6)=6 for (00), 3δij−12δij⋅6=0 for (ij) and 0−0=0 for (0i), which is the first-order expansion at λ=0 of the defining relation G=Ric⁡−12Sg of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, using S(0)=0 and g(0)=η.

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