Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves

TL;DR

This paper explores the potential to detect line-of-sight acceleration in gravitational wave signals from merging compact objects, providing the first observational constraints and projecting future detection capabilities with advanced detectors.

Contribution

It introduces the first observational constraints on line-of-sight acceleration in gravitational wave events and assesses future detection prospects with next-generation detectors.

Findings

No evidence of acceleration in GW170817 and GW190425 at 90% confidence.

Future detectors could constrain acceleration to as low as 10^{-16} s^{-1}.

Constraints can inform about mergers near supermassive black holes.

Abstract

Line-of-sight acceleration of a compact binary coalescence (CBC) event would modulate the shape of the gravitational waves (GWs) it produces with respect to the corresponding non-accelerated CBC. Such modulations could be indicative of its astrophysical environment. We investigate the prospects of detecting this acceleration in future observing runs of the LIGO-Virgo-KAGRA network, as well as in next-generation (XG) detectors and the proposed DECIGO. We place the first observational constraints on this acceleration, for putative binary neutron star mergers GW170817 and GW190425. We find no evidence of line-of-sight acceleration in these events at $90\%$ confidence. Prospective constraints for the fifth observing run of the LIGO at A+ sensitivity suggest that accelerations for typical BNSs could be constrained with a precision of $a/c \sim 10^{-7}~[\mathrm{s}^{-1}]$, assuming a signal-to-noise ratio of $10$. These improve to $a/c \sim 10^{-9}~[\mathrm{s}^{-1}]$ in XG detectors, and $a/c \sim 10^{-16}~[\mathrm{s}^{-1}]$ in DECIGO. We also interpret these constraints in the context of mergers around supermassive black holes.