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Evolution of the Einstein equations to future null infinity

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Rinne,  Oliver
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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フルテキスト (公開)

Rinne_Moncrief.pdf
(全文テキスト(全般)), 308KB

付随資料 (公開)

Rinne_Oliver.pdf
(付録資料), 299KB

引用

Rinne, O., & Moncrief, V. (2014). Evolution of the Einstein equations to future null infinity. In Relativity and Gravitation. Springer Proceedings in Physics (pp. 199-206). Springer.


引用: https://hdl.handle.net/11858/00-001M-0000-000E-7C68-C
要旨
We describe recent progress with a formulation of the Einstein equations on constant mean curvature surfaces extending to future null infinity. Long-time stable numerical evolutions of an axisymmetric gravitationally perturbed Schwarzschild black hole have been obtained. Here we show how matter can be included in our formulation. We study late-time tails for the spherically symmetric Einstein–Yang–Mills equations both for initial data that disperse and that collapse to a black hole.