Re-formulating the Einstein equations for stable numerical simulations: Formulation Problem in Numerical Relativity
Authors:
Hisa-aki Shinkai, Gen Yoneda
Updated:
2002/12/2
Comments:
50 pages, 18 figs, 98 references, LaTeX.
A review for a part of the book "Progress in Astronomy and Astrophysics" (Nova Science Publ.,
2003?).
Abstract:
We review recent efforts to re-formulate the Einstein equations for fully relativistic numerical simulations. The so-called
numerical relativity (computational simulations in general relativity) is a promising research field matching with ongoing
astrophysical observations such as gravitational wave astronomy. Many trials for longterm stable and accurate simulations of
binary compact objects have revealed that mathematically equivalent sets of evolution equations show different numerical
stability in free evolution schemes. In this article, we first review the efforts of the community, categorizing them into the
following three directions: (1) modifications of the standard Arnowitt-Deser-Misner equations initiated by the Kyoto group, (2)
rewriting of the evolution equations in hyperbolic form, and (3) construction of an ``asymptotically constrained" system. We
next introduce our idea for explaining these evolution behaviors in a unified way using eigenvalue analysis of the constraint
propagation equations. The modifications of (or adjustments to) the evolution equations change the character of constraint
propagation, and several particular adjustments using constraints are expected to diminish the constraint-violating modes. We
propose several new adjusted evolution equations, and include some numerical demonstrations. We conclude by discussing some
directions for future research.
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