Gravitational Wave Constraints on Planetary-Mass Primordial Black Holes Using LIGO O3a DataSep 1, 2024·Andrew L. Miller,Nancy Aggarwal,Others· 0 min read PDF Cite DOIPublicationPhys. Rev. Lett. 133(11) 111401Last updated on Sep 1, 2024 AuthorsAndrew L. MillerPostdoctoral Researcher ← Prospects for detecting asteroid-mass primordial black holes in extreme-mass-ratio inspirals with continuous gravitational waves Oct 1, 2024Continuous gravitational waves: A new window to look for heavy nonannihilating dark matter Aug 1, 2024 →