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Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs

Tore Boybeyi ^1,*, Sebastien Clesse ^2,3,†, Sachiko Kuroyanagi ^4,5,‡, and Mairi Sakellariadou ^6,§

¹School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
²Service de Physique Théorique Brussels Laboratory of the Universe, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, 1050 Brussels, Belgium
³Brussels Laboratory of the Universe, Université Libre de Bruxelles, Boulevard du Triomphe, CP225, 1050 Brussels, Belgium
⁴Instituto de Física Teórica UAM-CSIC, Universidad Autónoma de Madrid, Cantoblanco 28049 Madrid, Spain
⁵Department of Physics and Astrophysics, Nagoya University, 464-8602, Nagoya, Japan
⁶Theoretical Particle Physics and Cosmology Group, Physics Department, King’s College London, University of London, Strand, London, WC2R 2LS, United Kingdom

^*Contact author: boybe001@umn.edu
^†Contact author: sebastien.clesse@ulb.be
^‡Contact author: sachiko.kuroyanagi@csic.es
^§Contact author: mairi.sakellariadou@kcl.ac.uk

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Articles Citing

Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs

Primordial black holes: constraints, potential evidence and prospects

Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences

In-depth analysis of the clustering of dark matter particles around primordial black holes. Part II. Analytical prescriptions for spikes

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No title available

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Extended mass distribution of PBHs during the QCD phase transition: Stochastic gravitational wave backgrounds and mini-extreme mass ratio inspirals

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Dark classification matters: searching for primordial black holes with LSST

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