Testing numerical relativity with the shifted gauge wave
Maria C. Babiuc, Bela Szilagyi, Jeffrey Winicour

TL;DR
This paper introduces a shifted gauge wave test for numerical relativity, revealing an exponential instability caused by shift, and discusses techniques to suppress it, aiding black hole simulations.
Contribution
It presents a new shifted gauge wave test with boundary conditions that expose instabilities, and proposes methods to suppress these in harmonic evolution codes.
Findings
Shift introduces exponential growth in the gauge wave test.
Certain techniques can suppress instabilities caused by shift.
The methods are applicable to black hole simulations.
Abstract
Computational methods are essential to provide waveforms from coalescing black holes, which are expected to produce strong signals for the gravitational wave observatories being developed. Although partial simulations of the coalescence have been reported, scientifically useful waveforms have so far not been delivered. The goal of the AppleswithApples (AwA) Alliance is to design, coordinate and document standardized code tests for comparing numerical relativity codes. The first round of AwA tests have now being completed and the results are being analyzed. These initial tests are based upon periodic boundary conditions designed to isolate performance of the main evolution code. Here we describe and carry out an additional test with periodic boundary conditions which deals with an essential feature of the black hole excision problem, namely a non-vanishing shift. The test is a shifted…
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