Gravitational waves from binary supermassive black holes missing in pulsar observations

R.M. Shannon, V. Ravi, L.T. Lentati, P.D. Lasky, G. Hobbs, M. Kerr, R.N. Manchester, W.A. Coles, Y. Levin, M. Bailes, N.D.R. Bhat, S. Burke-Spolaor, S. Dai, M.J. Keith, S. Osłowski, D.J. Reardon, W. Van Straten, L. Toomey, J.B. Wang, Linqing WenJ.S.B. Wyithe, Xingjiang Zhu

    Research output: Contribution to journalArticle

    231 Citations (Scopus)

    Abstract

    Gravitational waves are expected to be radiated by supermassive black hole binaries formed during galaxy mergers. A stochastic superposition of gravitational waves from all such binary systems would modulate the arrival times of pulses from radio pulsars. Using observations of millisecond pulsars obtained with the Parkes radio telescope, we constrained the characteristic amplitude of this background, Acyr, to be -15 with 95% confidence.This limit excludes predicted ranges for Acyr from current models with 91 to 99.7% probability. We conclude that binary evolution is either stalled or dramatically accelerated by galactic-center environments and that higher-cadence and shorterwavelength observations would be more sensitive to gravitational waves.
    Original languageEnglish
    Pages (from-to)1522-1525
    JournalScience
    Volume349
    Issue number6255
    DOIs
    Publication statusPublished - 2015

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