Late-time asymptotics conjecture for the linear charged wave equation on sub-extremal Reissner–Nordström spacetime

Let gRNg_{RN} be the sub-extremal Reissner–Nordström exterior metric with mass MM and charge ee, where 0e<M0\leq |e|<M, and let r+(M,e)=M+M2e2r_+(M,e)=M+\sqrt{M^2-e^2}. In an appropriate gauge, consider the linear charged wave equation

(gRN1)μνμνϕ=(iqer22Mr3+2e2r4)ϕ+2iqer(tϕ+rϕ).(g_{RN}^{-1})^{\mu\nu}\partial_\mu\partial_\nu\phi=\left(\frac{iqe}{r^2}-\frac{2M}{r^3}+\frac{2e^2}{r^4}\right)\phi+\frac{2iqe}{r}(\partial_t\phi+\partial_r\phi).

Late-time asymptotics conjecture. If 0<qe<120<|qe|<\frac{1}{2}, then a solution ϕ\phi with generic, regular initial data obeys the asymptotics stated in the paper's sharp asymptotic results for the uncharged models, for every rr+(M,e)r\geq r_+(M,e).

The claim proposes that the simplified linear charged wave model, the Maxwell–Klein–Gordon system, and the related charged scalar field model share the same late-time asymptotics. The supplied text does not establish this assertion or provide evidence resolving it.

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Primary source

Dejan Gajic and Maxime Van de Moortel, “Late-time tails for scale-invariant wave equations with a potential and the near-horizon geometry of null infinity”, arXiv:2401.13047 (2024).

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