Towards a Singularity-Proof Scheme in Numerical Relativity
arXiv:gr-qc/9210016 · doi:10.1103/PhysRevLett.69.1845
Abstract
Progress in numerical relativity has been hindered for 30 years because of the difficulties of avoiding spacetime singularities in numerical evolution. We propose a scheme which excises a region inside an apparent horizon containing the singularity. Two major ingredients of the scheme are the use of a horizon-locking coordinate and a finite differencing which respects the causal structure of the spacetime. Encouraging results of the scheme in the spherical collapse case are given.
9 pages
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