Mass inflation and the \(C^2\)-inextendibility of spherically symmetric charged scalar field dynamical black holes

DOI10.1007/s00220-020-03923-wzbMath1462.83009arXiv2001.11156OpenAlexW3120089543MaRDI QIDQ2662860

Maxime Van de Moortel

Publication date: 15 April 2021

Published in: Communications in Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2001.11156

zbMATH Keywords

spherical symmetryCauchy horizonHawking massdynamical black holeEinstein-Maxwell-Klein-Gordon equationmass inflation scenarioweak null singularity

Mathematics Subject Classification ID

Asymptotic behavior of solutions to PDEs (35B40) Black holes (83C57) Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Gravitational energy and conservation laws; groups of motions (83C40) Space-time singularities, cosmic censorship, etc. (83C75) Einstein-Maxwell equations (83C22) Einstein equations (35Q76)

Related Items (9)

Curvature blow-up and mass inflation in spherically symmetric collapse to a Schwarzschild black hole ⋮ Precise late-time asymptotics of scalar field in the interior of a subextreme Kerr black hole and its application in Strong Cosmic Censorship conjecture ⋮ The breakdown of weak null singularities inside black holes ⋮ Mathematical aspects of general relativity. Abstracts from the workshop held August 29 -- September 4, 2021 (hybrid meeting) ⋮ Blowup of the local energy of linear waves at the Reissner–Nordström–AdS Cauchy horizon ⋮ Numerical evolution of the interior geometry of charged black holes ⋮ On black hole thermodynamics, singularity, and gravitational entropy ⋮ Low regularity extensions beyond Cauchy horizons ⋮ Diophantine approximation as cosmic censor for Kerr-AdS black holes

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