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Harmonic-gauge plane-wave amplitudes split uniquely into a pure plane-wave gauge part and a transverse-traceless representative, with a two-dimensional space of polarizations

Statement

Let (M,g,N)=(R4,η,∂0) be the flat model with its inertial chart and let k≠0 be a null covector of the flat metric (The flat model spacetime: the Minkowski metric on R^4 and its inertial chart, Plane-wave perturbations of the flat linearization: planar profiles, wave covectors, amplitudes, TT form and the linearized field equations). Let X be the real vector space of symmetric 4×4 matrices (amplitudes), with trace tr⁡X=ηabXab and trace reversal Xˉab=Xab−12ηabtr⁡X. Define the three linear subspaces

V0:={X∈X:kaXˉab=0 for b=0,1,2,3},G:={X∈X:Xab=kaZb+kbZa for some Z∈R4},

and, for an observer n and propagation direction s with k=ω (η(n,⋅)+η(s,⋅)), ω≠0, the space

T:=Tn,s={X∈X:X(n,⋅)=0, X(s,⋅)=0, tr⁡X=0}

of transverse-traceless amplitudes of The wave screen of an observer and propagation direction, and the transverse-traceless projection of a symmetric two-tensor clause (d). Then:

(a) Adapted frames exist. There is a future-directed unit timelike n with k(n)≠0; putting ω:=−k(n) and s:=η−1(k)/ω−n (with η−1(k) the vector metrically dual to k) gives η(s,s)=1, η(n,s)=0 and k=ω(η(n,⋅)+η(s,⋅)), and (n,s) extends to an η-orthonormal basis (e0,e1,e2,e3) of R4 with e0=n, e3=s. In frame components kA=k(eA)=ω(−1,0,0,1) and kA=ω(1,0,0,1).

(b) The two subspaces lie in V0 and meet trivially. G⊆V0 and T⊆V0; the map R4→G, Z↦(kaZb+kbZa), is a linear isomorphism, so dim⁡G=4; dim⁡T=2; and T∩G={0}. Consequently dim⁡V0=6 and V0=T⊕G.

(c) Unique TT representative. For every X∈V0 there is exactly one Z∈R4 such that Xab′:=Xab−kaZb−kbZa is TT; in the frame of (a) with XAB the frame components of X, the solution is

Z0=−X002ω,Z1=−X01ω,Z2=−X02ω,Z3=Z0−X03ω.

Moreover the map π:V0→T, π(X):=X′, is linear and satisfies π∣T=id⁡T, so the quotient V0/G is isomorphic to T; with a screen basis of T as in The screen and spatial projectors are orthogonal projections of rank two and three, and the TT projection is the orthogonal projection onto the two-dimensional transverse-traceless space clause (d), the pair (A+,A×)=(X11′,X12′) is a linear isomorphism V0/G→R2.

(d) Differential form of the gauge condition and the gauge transformation. For a single-frequency plane wave hab=Xabcos⁡(k⋅x) with amplitude X∈X, the harmonic-gauge condition ∂ahˉab=0 of Flat linearized perturbations: families, trace reversal, gauge transformation and harmonic gauge clause (d) holds exactly when X∈V0. If X∈V0 and Z is as in (c), the covector field ξb:=Zbsin⁡(k⋅x) satisfies ∂aξb+∂bξa=(kaZb+kbZa)cos⁡(k⋅x), so that hab′:=hab−∂aξb−∂bξa is the plane wave with amplitude X′ and is again in harmonic gauge.

Facts & Assumptions

Given: The flat model with inertial chart, a null covector k≠0, and the spaces V0, G, T defined above.

[L1]

The flat metric is nondegenerate of signature (−,+,+,+); for every null k≠0 there is a future-directed unit timelike n with k(n)≠0, and (n,s) with the stated properties extends to an η-orthonormal basis (The flat model spacetime: the Minkowski metric on R^4 and its inertial chart, Every Lorentz form admits an ordered basis with matrix diag(-1,1,1,1), Timelike, null, spacelike and causal vectors of a Lorentz vector space, eta-orthogonality and orthogonal complements in a Lorentz vector space, Rational powers ar of a positive base).

[L2]

In an η-orthonormal basis (e0,e1,e2,e3), the matrix of the screen projector of the pair (e0,e3) is diag⁡(0,1,1,0) and the TT subspace T consists of the symmetric matrices with X11=−X22, X12=X21 and all other components zero; it is two-dimensional, and the map X↦(X11,X12) is a linear isomorphism onto R2 (The screen and spatial projectors are orthogonal projections of rank two and three, and the TT projection is the orthogonal projection onto the two-dimensional transverse-traceless space clauses (c)-(d), The wave screen of an observer and propagation direction, and the transverse-traceless projection of a symmetric two-tensor).

Proof

technique · direct; construct an adapted orthonormal frame from the null covector, evaluate the amplitude conditions in that frame, and solve the resulting finite linear system
1.1L1L5algebra

(Existence of the adapted frame.) A vector n with k(n)≠0 and the required properties exists: choose any future unit timelike v; if k(v)≠0 take n:=v; if k(v)=0, nondegeneracy of η and k≠0 give a vector w with k(w)≠0, and for small t≠0 the vector v+tw is future timelike and has k(v+tw)=tk(w)≠0; rescaling it to unit length gives n by [L1]. Put ω:=−k(n)≠0 and s:=η−1(k)/ω−n, where η−1(k) is the vector with components ηabkb. Then η(n,s)=k(n)/ω−η(n,n)=(−ω)/ω+1=0 and η(s,s)=η−1(k,k)/ω2−2k(n)/ω+η(n,n)=0−2(−ω)/ω−1=1, so s is a unit spacelike vector orthogonal to n; moreover k=ω(η(n,⋅)+η(s,⋅)) by construction. By [L5] the pair extends to an η-orthonormal basis with e0=n, e3=s; in that basis the frame components of the covector are kA=k(eA)=ω(η(n,eA)+η(s,eA))=ω(−1,0,0,1) and the raised components are kA=ηABkB=ω(1,0,0,1). This proves (a).

2.1L3algebra

(The pure gauge amplitudes.) Let Hab=kaZb+kbZa. Its trace is tr⁡H=2kaZa=:2κZ, so Hˉab=kaZb+kbZa−ηabκZ; hence kaHˉab=kakaZb+kakbZa−kbκZ=kbκZ−kbκZ=0 because kaka=0 and kakbZa=kbκZ. Thus G⊆V0. If H=0, then testing in the frame of step 1.1 on e0 gives 0=H(e0,⋅)=−ωZ∙+Z0k∙; evaluating on e0 gives 0=−2ωZ0, so Z0=0, and substituting back gives ωZb=0 for every b, so Z=0. Hence Z↦(kaZb+kbZa) is injective, and its image G is isomorphic to R4, so dim⁡G=4 by [L3].

3.1L2L3step 2.1algebra

(The TT amplitudes.) If X∈T, then tr⁡X=0, so Xˉ=X, and X(e0,⋅)=X(e3,⋅)=0; in frame components kaXˉab=ω(X0b+X3b)=0 for every b. Hence T⊆V0. By [L2], dim⁡T=2. If X∈T∩G with X=kaZb+kbZa, then testing on e0 as in step 2.1 gives Z0=0 and then Z=0, so X=0: T∩G={0}.

4.1step 2.1step 3.1algebra

(Solving for the TT representative.) Let X∈V0 and let Z be any vector. Define Xab′:=Xab−kaZb−kbZa. In frame components with k0=−ω, k3=ω, the four equations X0b′=0 read X0b+ωZb−kbZ0=0, that is b=0: X00+2ωZ0=0;b=1: X01+ωZ1=0;b=2: X02+ωZ2=0;b=3: X03+ωZ3−ωZ0=0, whose unique solution is the displayed Z (the matrix of the system is triangular with diagonal entries 2ω,ω,ω,ω, all nonzero). Set X′ accordingly; then X′∈V0 because V0 is a subspace containing X and G (steps 2.1, 3.1). We show X′∈T. First, the harmonic-gauge condition kaXˉab′=0 in frame components reads ω(Xˉ0b′+Xˉ3b′)=0. For b=1,2 this is X31′+X01′=0 and X32′+X02′=0, because η31=η32=0; since X01′=X02′=0 by construction, X31′=X32′=0. For b=0 it gives Xˉ00′+Xˉ30′=0; here Xˉ30′=X30′−12η30tr⁡X′=X03′=0 and Xˉ00′=X00′−12η00tr⁡X′=12tr⁡X′, so tr⁡X′=0. For b=3 it gives Xˉ03′+Xˉ33′=0 with Xˉ03′=X03′=0 and Xˉ33′=X33′−12tr⁡X′=X33′, so X33′=0. Substituting tr⁡X′=X11′+X22′ (which holds because X00′=X33′=0) gives X11′+X22′=0. Therefore X′(e0,⋅)=0, X′(e3,⋅)=0 and tr⁡X′=0: X′∈T.

5.1L2L3step 2.1step 3.1step 4.1algebra

(Uniqueness and the projection.) If X′′,X′ are two TT representatives of the same X, their difference lies in T∩G={0} by step 3.1 and the definition of G; so the representative is unique. Writing π(X):=X′, the assignment is the composition of the linear maps X↦(X,Z(X)) and (X,Z)↦X−kZ−kZ with Z the linear solution of step 4.1, hence linear; and π(X)=X for X∈T because then Z=0 solves X0b′=X0b=0 (uniqueness of the solution). Consequently every X∈V0 is X=π(X)+(X−π(X)) with π(X)∈T and X−π(X)∈G, so V0=T+G; combined with T∩G={0} this is an internal direct sum, and by [L3] dim⁡V0=dim⁡T+dim⁡G=6. The map V0/G→T, X+G↦π(X), is a linear isomorphism, and by [L2] the map T→R2, X↦(X11,X12), is a linear isomorphism. This proves (b) and (c).

6.1L4step 4.1step 5.1algebra

(Differential form and the gauge transformation.) For hab=Xabcos⁡(k⋅x) we have hˉab=Xˉabcos⁡(k⋅x) and, by [L4], ∂ahˉab=kaXˉab(−sin⁡(k⋅x)); this vanishes identically exactly when kaXˉab=0 for every b, that is, exactly when X∈V0. With Z as in step 4.1 and ξb=Zbsin⁡(k⋅x), the product rule and [L4] give ∂aξb=kaZbcos⁡(k⋅x), hence ∂aξb+∂bξa=(kaZb+kbZa)cos⁡(k⋅x) and hab′=(Xab−kaZb−kbZa)cos⁡(k⋅x)=Xab′cos⁡(k⋅x) with X′∈T⊆V0, so h′ is in harmonic gauge. This proves (d).

7.1step 1.1step 2.1step 3.1step 4.1step 5.1step 6.1∎

(Conclusion.) Steps 1.1, 2.1, 3.1, 4.1, 5.1 and 6.1 prove the four clauses; the arguments use finite linear algebra in an adapted orthonormal frame and the coordinate calculus of the flat model only. No field equation and no physical assumption enters, and no choice beyond the inherited countable choice of the cited finite-dimensional suppliers is used.

Remarks

  • Frame dependence of the representative. The subspace T=Tn,s and hence the pair (A+,A×) of a class depend on the chosen observer n with k(n)≠0; the quotient V0/G and its dimension two do not. Clause (a) records that an adapted observer always exists, and the identity of two classes is tested by their TT representatives in any one admissible frame.

  • Residual gauge freedom. Harmonic gauge is preserved by the plane-wave gauges of G; that is the plane-wave instance of the residual freedom □ξ=0 after harmonic gauge, since □ξb=−kakaZbsin⁡(k⋅x)=0 for null k by [L4]. The lemma states this only in the form needed for the amplitude classification; the existence of a harmonic-gauge representative for a general (non-plane-wave) perturbation is a different statement, proved for the smooth all-space regime in All-space smooth wave equation with zero data, and harmonic gauge on flat space.

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