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Asymptotic time-translation flux of a charged scalar mode

Statement

Use the fixed subextremal electric Reissner–Nordström exterior, gauge, charged derivative, real normalized spherical harmonic Y, and mode conventions of Massless charged-scalar radial scattering data. Let ψ=Aine−iωtY(Ω)u(r∗)/r be any admitted real-frequency scattering mode with ω>0 and Ain≠0, and let R be its reflection coefficient. Form Tab[ψ;g,A,e] by the scalar stress-tensor definition. With ξ=∂t, define the outward radial flux through the sphere of radius r by

P(r):=−∫S2r2Trt[ψ;g,A,e] dωS2.

Let ψin:=Aine−iωtYe−iΘ/r and ψref:=Aine−iωtYReiΘ/r be the two leading asymptotic components. Define their nonnegative directional flux magnitudes by

Pin:=lim⁡r→∞∫S2r2Trt[ψin;g,A,e] dωS2,Pref:=−lim⁡r→∞∫S2r2Trt[ψref;g,A,e] dωS2.

Then

Pin=2ω2∣Ain∣2,Pref=2ω2∣Ain∣2∣R∣2,PrefPin=∣R∣2.

This is a conditional tensor calculation for the specified mode asymptotics; it asserts neither that such a mode exists nor that its flux has been observed.

Facts & Assumptions

Given: The exact static exterior and gauge of the scattering definition, a real normalized harmonic, an admitted mode with its stated two-term asymptotics and differentiated asymptotics at infinity, and the tensor assignment in the stress-tensor definition.

[F1]

Massless charged-scalar radial scattering data: At=−Q/r, Dt=∂t+ieQ/r, Dr=∂r, grr=f, ∂r∗=f∂r, and Θ′(r∗)=ω−eQf/r→ω; also ∫S2Y2 dωS2=1.

[F2]

Complex scalar stress tensor with a supplied potential: Tab=Daψ‾Dbψ+Dbψ‾Daψ−gabgcdDcψ‾Ddψ.

[A1]

The separated mode has the normalized asymptotics u=e−iΘ+ReiΘ+o(1) and u′=−iΘ′e−iΘ+iΘ′ReiΘ+o(1) as r→∞, with all parameters real and ω>0.

Proof

1.1givenF1A1algebra

Since At=−Q/r and ω>0, the time derivative satisfies Dtψ=−iωψ+o(r−1). Using Dr=f∂r=∂r∗ and ∂r∗(u/r)=u′/r−fu/r2, the differentiated asymptotics and Θ′→ω give ψ=Aine−iωtYr(e−iΘ+ReiΘ)+o(r−1),Drψ=Aine−iωtYr(−iωe−iΘ+iωReiΘ)+o(r−1).

2.1givenF1F2A1step 1.1algebra

Since grt=0, [F2] gives Trt=2Re⁡(Drψ‾Dtψ). Substitution of step 1.1 gives the diagonal terms ω2(1−∣R∣2); the cross terms are z−z‾ for z=ω2Re2iΘ and have zero real part. Integrating Y2 over the sphere and taking r→∞ therefore gives the net outward flux P(r)→2ω2∣Ain∣2(∣R∣2−1).

3.1givenF1F2A1step 1.1algebra∎

For the incoming component, Drψin=−iωψin+o(r−1) and Dtψin=−iωψin+o(r−1), so Trt[ψin]=2ω2∣ψin∣2+o(r−2); its positive inward magnitude is 2ω2∣Ain∣2 after sphere integration. For the reflected component, Drψref=iωψref+o(r−1) while Dtψref=−iωψref+o(r−1), so its nonnegative outward magnitude is 2ω2∣Ain∣2∣R∣2. Their ratio is ∣R∣2 because ω>0 and Ain≠0.

Remarks

The Coulomb phase in the scattering definition is retained; only its derivative limit Θ′→ω enters the asymptotic stress calculation. The result concerns the prescribed geometric normalization and supplies no scattering-solution existence claim.

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