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Precise late-time asymptotics of scalar field in the interior of a subextreme Kerr black hole and its application in Strong Cosmic Censorship conjecture

Siyuan Ma, Lin Zhang

Abstract

In this work, we compute the precise late-time asymptotics for the scalar field in the interior of a non-static subextreme Kerr black hole, based on recent progress on deriving its precise asymptotics in the Kerr exterior region. This provides a new proof of the generic $H^1_{\text{loc}}$-inextendibility of the Kerr Cauchy horizon against scalar perturbations that is first shown by Luk--Sbierski (J. Func. Anal., 2016). The analogous results in Reissner--Nordström spacetimes are also discussed.

Precise late-time asymptotics of scalar field in the interior of a subextreme Kerr black hole and its application in Strong Cosmic Censorship conjecture

Abstract

In this work, we compute the precise late-time asymptotics for the scalar field in the interior of a non-static subextreme Kerr black hole, based on recent progress on deriving its precise asymptotics in the Kerr exterior region. This provides a new proof of the generic -inextendibility of the Kerr Cauchy horizon against scalar perturbations that is first shown by Luk--Sbierski (J. Func. Anal., 2016). The analogous results in Reissner--Nordström spacetimes are also discussed.
Paper Structure (21 sections, 11 theorems, 173 equations, 7 figures)

This paper contains 21 sections, 11 theorems, 173 equations, 7 figures.

Key Result

Theorem 1.1

Let $0<\lvert a\rvert<M$. Let $\psi$ be a solution to the scalar wave equation eq:wave arising from smooth, compactly supported initial data on $\Sigma_{\text{init}}$. Let $j_1\in \mathbb{N}$, $s_1>0$ be suitably largeBy examining the proof, we find that $j_1=4$ and $s_1=9$ are sufficient. The reaso Assume moreover that there are real constants $c_0$ and $c_0'$ and an $\epsilon>0$Without loss of g

Figures (7)

  • Figure 1: Kerr interior and Kerr exterior regions
  • Figure 2: Two-ended initial value problem
  • Figure 3: Region ${_{r}}\mathcal{D}^{+}_{\text{init}}$ and its subregions
  • Figure 4: Region ${_{l}}\mathcal{D}^{+}_{\text{init}}$ and its subregions
  • Figure 5: Different asymptotic regions in the exterior and interior of a Kerr black hole
  • ...and 2 more figures

Theorems & Definitions (24)

  • Theorem 1.1: Global precise late-time asymptotics for the scalar field and its derivatives in Kerr interior
  • Remark 1.2: Global late-time precise asymptotics in ${_{l}}\mathcal{D}^{+}_{\text{init}}\cup{_{r}}\mathcal{D}^{+}_{\text{init}}$
  • Remark 1.3: Global late-time precise asymptotics for $\psi$ and its principal null derivatives in $\mathcal{D}^+_{\text{init}}$
  • Remark 1.4: Precise late-time asymptotics for nondegenerate transverse derivative near event horizon
  • Theorem 1.5: Global precise late-time asymptotics for scalar field in the interior of a Reissner--Nordström spacetime
  • Theorem 1.6: Precise asymptotics for the scalar field on the Kerr event horizon hintz2022sharpangelopoulos2021lateMZ21PLKerr
  • Remark 1.7: Generic inextendibility for scalar field in Kerr interior
  • Theorem 3.1: Precise late-time asymptotics in the region $\mathcal{D}^+_{\text{init}}\cap\{r_{\mathfrak{b}}\leq r\leq r_+\}$
  • Proposition 3.2
  • proof
  • ...and 14 more