Pulsar timing can constrain primordial black holes in the LIGO mass window
arXiv:1610.04234 · doi:10.1103/PhysRevD.95.023002
Abstract
The recent discovery of gravitational waves from merging black holes has generated interest in primordial black holes as a possible component of the dark matter. In this paper, we show that pulsar timing may soon have sufficient data to constrain - primordial black holes via the non-detection of a third-order Shapiro time delay as the black holes move around the Galactic halo. We present the results of a Monte Carlo simulation which suggests that future data from known pulsars may be capable of constraining the PBH density more stringently than other existing methods in the mass range ~1-30. We find that timing new pulsars discovered using the proposed Square Kilometre Array may constrain primordial black holes in this mass range to comprise less than ~1-10% of the dark matter.
arXiv comment6 pages, 2 figures; published in PRD with minor revision (no changes to results)
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