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arXiv · 2202.01835

Static solutions to the spherically symmetric Einstein-Vlasov system: a particle-number-Casimir approach

Håkan Andréasson·Markus Kunze
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Abstract

Existence of spherically symmetric solutions to the Einstein-Vlasov system is well-known. However, it is an open problem whether or not static solutions arise as minimizers of a variational problem. Apart from being of interest in its own right, it is the connection to non-linear stability that gives this topic its importance. This problem was considered in \cite{Wol}, but as has been pointed out in \cite{AK}, the paper \cite{Wol} contained serious flaws. In this work we construct static solutions by solving the Euler-Lagrange equation for the energy density $\rho$ as a fixed point problem. The Euler-Lagrange equation originates from the particle number-Casimir functional introduced in \cite{Wol}. We then define a density function $f$ on phase space which induces the energy density $\rho$ and we show that it constitutes a static solution of the Einstein-Vlasov system. Hence we settle rigorously parts of what the author of \cite{Wol} attempted to prove.

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Håkan Andréasson, Markus Kunze. 2022-02-03. Static solutions to the spherically symmetric Einstein-Vlasov system: a particle-number-Casimir approach. https://doi.org/10.1137/22m1522887

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