Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches

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Abbott, R. and Ben Yaala, M. and Talbot, C. J., The Virgo Collaboration, LIGO Scientific Collaboration, KAGRA Collaboration (2022) Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches. Physical Review D, 105 (6). 062008. ISSN 1550-2368 (https://doi.org/10.1103/PhysRevD.105.062008)

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Abstract

We present new constraints on the merging rates of planetary-mass and asteroid-mass primordial black hole binaries using limits on continuous waves (quasimonochromatic, quasi-infinite duration signals) derived from an all-sky search for isolated compact objects in the first six months of the third observing run (O3a) of LIGO/Virgo. We calculate the merging rates of these binaries in a model-independent way, and convert them to constraints on the primordial black hole abundance with minimal modeling assumptions. Our results show that all-sky searches are sensitive to sources at most O(10  pc) away for systems with chirp masses of O(10−5  M⊙) at gravitational-wave frequencies around 30 Hz–40 Hz. These results also show that continuous-wave searches could in the future directly probe the existence of planetary-mass and asteroid-mass primordial black holes, especially those in binaries with asymmetric mass ratios. Furthermore, they demonstrate that new methods accounting for the full nonlinear gravitational-wave frequency evolution are needed to improve constraints on primordial black holes.

ORCID iDs

Abbott, R., Ben Yaala, M. ORCID logoORCID: https://orcid.org/0000-0002-6754-0875 and Talbot, C. J.;
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