Prospects for detecting asteroid-mass primordial black holes in extreme-mass-ratio inspirals with continuous gravitational wavesJan 1, 2025·Andrew L. Miller· 0 min read PDF Cite DOIPublicationPhys. Rev. D 112(10) 103027Last updated on Jan 1, 2025 AuthorsAndrew L. MillerAssociate Professor ← Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes Jan 1, 2025Searching for continuous gravitational waves from highly deformed compact objects with DECIGO Jan 1, 2025 →