Can environmental effects spoil precision gravitational-wave astrophysics?

TL;DR

This paper investigates how various environmental factors influence gravitational-wave signals from black holes and compact binaries, finding that such effects are generally negligible but can dominate in specific extreme cases, impacting tests of gravity.

Contribution

It provides a comprehensive analysis of environmental effects on gravitational-wave signals, highlighting their significance in different astrophysical scenarios and informing data analysis strategies.

Findings

Resonances due to external mass distributions affect late-time waveforms.

Environmental effects are negligible for most eLISA sources, except some extreme mass ratio inspirals.

Accretion and hydrodynamic drag dominate over self-force in thin disk environments.

Abstract

[abridged abstract] No, within a broad class of scenarios. With the advent of gravitational-wave (GW) astronomy, environmental effects on the GW signal will eventually have to be quantified. Here we present a wide survey of the corrections due to these effects in two situations of great interest for GW astronomy: the black hole (BH) ringdown emission and the inspiral of two compact objects. We take into account various effects such as: electric charges, magnetic fields, cosmological evolution, possible deviations from General Relativity, firewalls, and various forms of matter such as accretion disks and dark matter halos. Our analysis predicts the existence of resonances dictated by the external mass distribution, which dominate the very late-time behavior of merger/ringdown waveforms. The mode structure can drastically differ from the vacuum case, yet the BH response to external perturbations is unchanged at the time scales relevant for detectors. This is because although the vacuum Schwarzschild resonances are no longer quasinormal modes of the system, they still dominate the response at intermediate times. Our results strongly suggest that both parametrized and ringdown searches should use at least two-mode templates. Our analysis of compact binaries shows that environmental effects are typically negligible for most eLISA sources, with the exception of very few special extreme mass ratio inspirals. We show in particular that accretion and hydrodynamic drag generically dominate over self-force effects for geometrically thin disks, whereas they can be safely neglected for geometrically thick disk environments, which are the most relevant for eLISA. Finally, we discuss how our ignorance of the matter surrounding compact objects implies intrinsic limits on the ability to constrain strong-field deviations from General Relativity.