Hod–Piran charged massless scalar decay conjecture

Let H+\mathcal{H}^+ be the event horizon, let vv be the standard advanced time null coordinate, let ee be the asymptotic charge at timelike infinity, and define

δ(q0e)=1Re14(q0e)2[0,1).\delta(q_0e)=1-\operatorname{Re}\sqrt{1-4(q_0e)^2}\in[0,1).

Charged massless scalar decay conjecture. For smooth, regular, generic admissible data with a non-empty black hole and m2=0m^2=0,

ϕH+(v)v2+δ(q0e),DvϕH+(v)v2+δ(q0e).|\phi|_{\mathcal{H}^+}(v)\sim v^{-2+\delta(q_0e)},\qquad |D_v\phi|_{\mathcal{H}^+}(v)\sim v^{-2+\delta(q_0e)}.

The conjecture is supported by heuristic and numerical work; an upper bound is proved on a fixed Reissner–Nordström background for small charge, but the full nonlinear asymptotic remains open.

Sources & referencesView supporting material

Primary source

Maxime Van de Moortel, “Mass inflation and the C^2-inextendibility of spherically symmetric charged scalar field dynamical black holes”, arXiv:2001.11156 (2020).

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