Extrapolating gravitational-wave data from numerical simulations

TL;DR

This paper introduces two new algorithms to accurately extrapolate gravitational-wave data from numerical simulations, reducing near-field errors that can impact LIGO data analysis.

Contribution

It presents two novel extrapolation techniques for gravitational-wave data, demonstrating their effectiveness and agreement in a specific black-hole binary simulation.

Findings

Extrapolation reduces errors in waveform extraction.

The two methods produce consistent results within error margins.

Improves the reliability of gravitational-wave data analysis.

Abstract

Two complementary techniques are developed for obtaining the asymptotic form of gravitational-wave data at large radii from numerical simulations, in the form of easily implemented algorithms. It is shown that, without extrapolation, near-field effects produce errors in extracted waveforms that can significantly affect LIGO data analysis. The extrapolation techniques are discussed in the context of Newman--Penrose data applied to extrapolation of waveforms from an equal-mass, nonspinning black-hole binary simulation. The results of the two methods are shown to agree within error estimates. The various benefits and deficiencies of the methods are discussed.