The characteristic initial-boundary value problem for the Einstein--massless Vlasov system in spherical symmetry
Georgios Moschidis

TL;DR
This paper develops the mathematical framework for analyzing the Einstein-massless Vlasov system in spherical symmetry with negative cosmological constant, establishing existence, uniqueness, and stability results for solutions with specific boundary conditions.
Contribution
It introduces the initial-boundary value problem for the Einstein-massless Vlasov system in AdS spacetime, proving key existence, continuation, and stability results under spherical symmetry.
Findings
Existence and uniqueness of maximal future development.
Continuation criteria based on the ratio 2m/r.
Cauchy stability of Anti-de Sitter spacetime.
Abstract
In this paper, we initiate the study of the asymptotically AdS initial-boundary value problem for the Einstein-massless Vlasov system with in spherical symmetry. We will establish the existence and uniqueness of a maximal future development for the characteristic initial-boundary value problem in the case when smooth initial data are prescribed on a future light cone emanating from a point at and a reflecting boundary condition is imposed on conformal infinity . We will then prove a number of continuation criteria for smooth solutions of the spherically symmetric Einstein-massless Vlasov system, under the condition that the ratio remains small in a neighborhood of . Finally, we will establish a Cauchy stability statement for Anti-de Sitter spacetime as a solution of the spherically symmetric Einstein-massless Vlasov…
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Taxonomy
TopicsCosmology and Gravitation Theories · Gas Dynamics and Kinetic Theory · Advanced Mathematical Physics Problems
