Generic Schwarzschild Arnold-diffusion conjecture near the photon sphere

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Let NεN_\varepsilon denote the perturbed normally hyperbolic invariant manifold associated with the photon sphere, and let LL and LzL_z be the angular-momentum quantities used in the Schwarzschild dynamics. Generic Schwarzschild diffusion conjecture near the photon sphere. For a generic stationary perturbation of the Schwarzschild metric, for every δ>0\delta>0 there is an ε0\varepsilon_0 such that, whenever ∣ε∣<ε0|\varepsilon|<\varepsilon_0, an orbit on NεN_\varepsilon and times T,T′T,T' exist with

∣Lz(T)−L(0)∣<δ,∣Lz(T′)+L(0)∣<δ.|L_z(T)-L(0)|<\delta,\qquad |L_z(T')+L(0)|<\delta.

For a generic perturbation that is 11-periodic in τ\tau, for every δ>0\delta>0 there is an orbit visiting every δ\delta-ball centered on N×T1×(4/9,1/2)N\times\mathbb T^1\times(4/9,1/2), with the center written (Ξ,τ,E)(\Xi,\tau,E), provided ε\varepsilon is sufficiently small. These are explicitly presented as part of a conjectural picture based on normal hyperbolicity and the scattering mechanism.

References

Primary source

Jinxin Xue, “Arnold diffusion and geodesic dynamics of blackholes”, arXiv:2012.03047 (2020).

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