Gravitational-wave standard sirens and application in cosmology

TL;DR

Gravitational-wave standard sirens from binary mergers offer a novel, independent way to measure cosmic expansion and constrain cosmological parameters, especially with upcoming advanced detectors.

Contribution

This paper reviews the principles, methods, and future prospects of using gravitational-wave standard sirens for cosmology, highlighting recent developments and challenges.

Findings

Gravitational-wave sources can serve as standard sirens to measure the Universe's expansion.

Electromagnetic counterparts enable precise redshift measurements for binary neutron star mergers.

Future detectors will improve constraints on the Hubble constant and dark energy parameters.

Abstract

The discovery of the gravitational-wave event GW170817 from a binary neutron star merger, together with its multi-wavelength electromagnetic counterparts, marks the beginning of the era of multi-messenger gravitational wave astronomy. Observations of gravitational-wave signals from compact binary mergers enable an independent measurement of the luminosity distance to the source. This implies that gravitational-wave sources can serve as standard sirens to probe the expansion history of the Universe, providing a new approach to constrain cosmological parameters. In this paper, we review the basic principles of using gravitational-wave standard sirens to constrain cosmology. We discuss various methods for determining the source distance and redshift, as well as the capabilities of second and third generation ground-based detectors and space-based detectors in constraining cosmological parameters, especially the Hubble constant and dark energy parameters. By examining two types of standard sirens, binary neutron star mergers with electromagnetic counterparts as bright sirens and stellar-mass binary black hole mergers as dark sirens, we illustrate the methodology, challenges, and future prospects of the standard siren approach.