Pulsar Timing Array Experiments

Abstract

Pulsar timing is a technique that uses the highly stable spin periods of neutron stars to investigate a wide range of topics in physics and astrophysics. Pulsar timing arrays (PTAs) use sets of extremely well-timed pulsars as a Galaxy-scale detector with arms extending between Earth and each pulsar in the array. These challenging experiments look for correlated deviations in the pulsars' timing that are caused by low-frequency gravitational waves (GWs) traversing our Galaxy. PTAs are particularly sensitive to GWs at nanohertz frequencies, which makes them complementary to other space- and ground-based detectors. In this chapter, we will describe the methodology behind pulsar timing; provide an overview of the potential uses of PTAs; and summarise where current PTA-based detection efforts stand. Most predictions expect PTAs to successfully detect a cosmological background of GWs emitted by supermassive black-hole binaries and also potentially detect continuous-wave emission from binary supermassive black holes, within the next several years.

49 pages, 6 figures, published in the "Handbook of Gravitational Wave Astronomy" Eds. Bambi, Katsanevas & Kokkotas (Springer, Singapore, 2021)

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Cited by in corpus (8)

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• Primordial black holes and gravitational waves induced by exponential-tailed perturbations
• Gravitational Wave Timing Array
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• The Statistics of the Cross-Spectrum and the Spectrum Average: Generalization to Multiple Instruments
• Gravitational wave astronomy: astrophysical and cosmological inferences
• Non canonical polarizations of Gravitational Waves