no code implementations • 2 Oct 2020 • Sunil Choudhary, Nicolas Sanchis-Gual, Anshu Gupta, Juan Carlos Degollado, Sukanta Bose, José A. Font
We show how gravitational-wave observations of binary black hole (BBH) mergers can constrain the physical characteristics of a scalar field cloud parameterized by mass $\tilde{\mu}$ and strength $\phi_0$ that may surround them.
General Relativity and Quantum Cosmology
