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Pulsar timing for gravitational wave detection

Nature Astronomy volume 1, pages 809–811 (2017)Cite this article

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Pulsar timing arrays may well be the next type of experiment to detect gravitational waves. Sensitive to lower frequencies than LIGO–Virgo, they will detect the stochastic background of massive binary black hole mergers.

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Fig. 1

Reproduced from ref. 12, IOP.

Fig. 2: Side-by-side comparison of how LIGO–Virgo (left) detects a gravitational wave source and how PTAs (right) detect a source.

Mark Garlick/Science Photo Library/Alamy Stock Photo.

Fig. 3: Partners in the International Pulsar Timing Array.

References

  1. Abbott, B. P. et al. (LIGO Scientific Collaboration and Virgo Collaboration) Phys. Rev. Lett. 116, 061102 (2016).

    Article  ADS  MathSciNet  Google Scholar 

  2. Abbott, B. P. et al. (LIGO Scientific Collaboration and Virgo Collaboration) Phys. Rev. Lett. 119, 141101 (2017).

    Article  ADS  Google Scholar 

  3. Verbiest, J. P. W. et al. Mon. Not. R. Astron. Soc. 458, 1267–1288 (2016).

    Article  ADS  Google Scholar 

  4. Lommen, A. N. Rep. Prog. Phys. 78, 124901 (2015).

    Article  ADS  Google Scholar 

  5. Merritt, D. & Ferrarese, L. Mon. Not. R. Astron. Soc. 320, L30–L34 (2001).

    Article  ADS  Google Scholar 

  6. Shannon, R. M. et al. Science 342, 334–337 (2013).

    Article  ADS  Google Scholar 

  7. Lentati, L. et al. Mon. Not. R. Astron. Soc. 453, 2576–2598 (2015).

    Article  ADS  Google Scholar 

  8. Arzoumanian, Z. et al. Astrophys. J. 821, 13–23 (2016).

    Article  ADS  Google Scholar 

  9. Taylor, S. R. et al. Astrophys. J. 819, L6–L11 (2016).

    Article  Google Scholar 

  10. Madison, D. R., Cordes, J. M. & Chatterjee, S. Astrophys. J. 788, 141–154 (2014).

    Article  ADS  Google Scholar 

  11. Mingarelli, C. M. F. et al. Nat. Astron. https://doi.org/10.1038/S41550-017-0299-6 (2017).

  12. Moore, C. J., Cole, R. H. & Berry, C. P. L. Class. Quantum. Grav 32, 015014 (2015).

    Article  ADS  Google Scholar 

Download references

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  1. Department of Physics and Astronomy, Haverford College, Haverford, PA, USA

    Andrea N. Lommen

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  1. Andrea N. Lommen
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Correspondence to Andrea N. Lommen.

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Lommen, A. Pulsar timing for gravitational wave detection. Nat Astron 1, 809–811 (2017). https://doi.org/10.1038/s41550-017-0324-9

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