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The international pulsar timing array: a galactic scale gravitational wave observatory

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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.

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Notes

  1. http://www.atnf.csiro.au/people/pulsar/psrcat/.

  2. There is no strict cutoff for MSPs, with the main criterion being that they are fully recycled. However, there are no MSPs with periods more than 20 ms included in PTAs.

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Acknowledgments

Thank you to all of my colleagues in NANOGrav and the IPTA for many conversations that have improved this paper. The comments from the anonymous referee were also immensely helpful.

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  1. Department of Physics and Astronomy, West Virginia University, Morgantown, WV, 26506, USA

    Maura McLaughlin

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Correspondence to Maura McLaughlin.

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This article belongs to the Topical Collection: The First Century of General Relativity: GR20/Amaldi10. Guest Editors: Jerzy Lewandowski, Bala Iyer, Sheila.

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McLaughlin, M. The international pulsar timing array: a galactic scale gravitational wave observatory. Gen Relativ Gravit 46, 1810 (2014). https://doi.org/10.1007/s10714-014-1810-3

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