PREPRINT
35DBFE2B-D9E1-410C-94B8-25951E18D576

Priorities in gravitational waveform modelling for future space-borne detectors: vacuum accuracy or environment?

Lorenz Zwick, Pedro R. Capelo, Lucio Mayer

Submitted on 8 September 2022

Abstract

In preparation for future space-borne gravitational-wave (GW) detectors, should the modelling effort focus on high-precision vacuum templates or on the the astrophysical environment of the sources? We perform a systematic comparison of the phase contributions caused by 1) known environmental effects in both gaseous and stellar matter backgrounds, or 2) high-order post-Newtonian terms in the evolution of mHz GW sources. We use the accuracy of currently available analytical waveform models as a benchmark and find the following trends: the largest unmodelled contributions are likely environmental for binaries lighter than 107/(1+z)2~M, where z is the redshift. Binaries heavier than 108/(1+z)~M do not require more accurate waveforms due to low signal-to-noise ratios (SNRs). For high-SNR sources, environmental influences are relevant at low redshift, while high-order vacuum templates are required at z>4. Led by these findings, we argue that including environmental effects in waveform models should be prioritised in order to maximize the science yield of mHz detectors.

Preprint

Comment: Submitted to MNRAS

Subjects: General Relativity and Quantum Cosmology; Astrophysics - High Energy Astrophysical Phenomena

URL: https://arxiv.org/abs/2209.04060