Abstract
The role of Regge calculus as a tool for numerical relativity is discussed,
and a parallelizable implicit evolution scheme described. Because of the
structure of the Regge equations, it is possible to advance the vertices of a
triangulated spacelike hypersurface in isolation, solving at each vertex a
purely local system of implicit equations for the new edge-lengths involved.
(In particular, equations of global ``elliptic-type'' do not arise.)
Consequently, there exists a parallel evolution scheme which divides the
vertices into families of non-adjacent elements and advances all the vertices
of a family simultaneously. The relation between the structure of the equations
of motion and the Bianchi identities is also considered. The method is
illustrated by a preliminary application to a 600--cell Friedmann cosmology.
The parallelizable evolution algorithm described in this paper should enable
Regge calculus to be a viable discretization technique in numerical relativity.
Users
Please
log in to take part in the discussion (add own reviews or comments).