Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing
arXiv:0706.0740 · doi:10.1088/0264-9381/25/10/105006
Abstract
We describe a modification of a fourth-order accurate ``moving puncture'' evolution code, where by replacing spatial fourth-order accurate differencing operators in the bulk of the grid by a specific choice of sixth-order accurate stencils we gain significant improvements in accuracy. We illustrate the performance of the modified algorithm with an equal-mass simulation covering nine orbits.
13 pages, 6 figures
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- Gravitational waves from black-hole mergers