Models for Self-Gravitating Photon Shells and Geons
arXiv:1511.01290 · doi:10.1007/s00023-016-0531-4
Abstract
We prove existence of spherically symmetric, static, self-gravitating photon shells as solutions to the massless Einstein-Vlasov system. The solutions are highly relativistic in the sense that the ratio is close to , where is the Hawking mass and is the area radius. In 1955 Wheeler constructed, by numerical means, so called idealized spherically symmetric geons, i.e. solutions of the Einstein-Maxwell equations for which the energy momentum tensor is spherically symmetric on a time average. The structure of these solutions is such that the electromagnetic field is confined to a thin shell for which the ratio is close to , i.e., the solutions are highly relativistic photon shells. The solutions presented in this work provide an alternative model for photon shells or idealized spherically symmetric geons.
References in corpus (4)
- A numerical investigation of the stability of steady states and critical phenomena for the spherically symmetric Einstein-Vlasov system
- On the steady states of the spherically symmetric Einstein-Vlasov system
- Critical collapse in the spherically-symmetric Einstein-Vlasov model
- A class of dust-like self-similar solutions of the massless Einstein-Vlasov system
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