On the evolution of the momentarily static radiation free data in the Apostolatos - Thorne cylindrical shell model
Reinaldo J. Gleiser, Daniel E. Barraco

TL;DR
This paper investigates the evolution of momentarily static, radiation-free initial data in a cylindrical shell model, demonstrating stability, slow approach to equilibrium, and compatibility with static configurations through analytical and numerical methods.
Contribution
It provides a detailed analysis of the evolution and stability of MSRF data in the Apostolatos-Thorne model, including a new numerical procedure and a proof of solution existence for related wave equations.
Findings
Evolution is stable in all cases.
Approach to final state is very slow, logarithmic in time.
Numerical visualization confirms qualitative behavior.
Abstract
We study the evolution of the "Momentarily Static and Radiation Free" (MSRF) initial data for the Apostolatos - Thorne cylindrical shell model. We analyze the relation between the parameters characterizing the MSRF data those for the corresponding final static configuration, and show that there is a priori no conflict for any choice of initial MSRF data, in contrast with some recent results of Nakao, Ida and Kurita. We also consider the problem in the linear approximation, and show that the evolution is stable in all cases. We find that the approach to the final state is very slow, with an inverse logarithmic dependence on time at fixed radius. To complement these results we introduce a numerical computation procedure that allows us to visualize the explicit form of the evolution of the shell and of the gravitational field up to large times. The results are in agreement with the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
