The International Pulsar Timing Array: A Galactic Scale Gravitational Wave Observatory

TL;DR

This paper discusses the use of a global array of millisecond pulsars as a gravitational wave detector, highlighting recent progress and future prospects for detecting low-frequency gravitational waves.

Contribution

It provides an overview of the pulsar timing array efforts and discusses how advancements will enhance gravitational wave detection capabilities.

Findings

Growing number of pulsars improves sensitivity

Expected detection or constraints within next several years

Enhanced instrumentation and longer observations drive progress

Abstract

The phenomenal rotational stability of millisecond pulsars allows them to be used as precise celestial clocks. An array of these pulsars can be exploited to search for correlated perturbations in their pulse times of arrival due to gravitational waves. Here, I describe the observations and analysis necessary to accomplish this goal and present an overview of the efforts of the worldwide pulsar timing community. Due to a growing number of millisecond pulsar discoveries, improved instrumentation, and growing timespans of observation, the sensitivity of our pulsar timing array experiments is expected to dramatically increase over the next several years, leading to either a gravitational wave detection or very stringent constraints on low-frequency gravitational wave source populations before the end of the decade.