Einstein-Vlasov system in spherical symmetry. II. Spherical perturbations of static solutions

Aug 23, 2017
13 pages
Published in:
  • Phys.Rev.D 96 (2017) 8, 084008
  • Published: Oct 4, 2017
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Abstract: (APS)
We reduce the equations governing the spherically symmetric perturbations of static spherically symmetric solutions of the Einstein-Vlasov system (with either massive or massless particles) to a single stratified wave equation -ψ,tt=Hψ, with H containing second derivatives in radius, and integrals over energy and angular momentum. We identify an inner product with respect to which H is symmetric, and use the Ritz method to approximate the lowest eigenvalues of H numerically. For two representative background solutions with massless particles we find a single unstable mode with a growth rate consistent with the universal one found by Akbarian and Choptuik in nonlinear numerical time evolutions.