2011/12/16 by James Healy, Tanja Bode, Roland Haas +5 · 4 citations
Physics and Astronomy · #Binary black hole #Binary number #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #General relativity #Gravitation #Gravitational wave #Numerical relativity #Pulsars and Gravitational Waves Research #Scalar (mathematics) #Scalar field #astro-ph.CO #gr-qc #hep-ph
paper · pdf · doi:10.1088/0264-9381/29/23/232002
4 pages, 5 figures, 1 table
arxiv created 2011/12/16 · openalex publication_date 2012/10/22 · arxiv updated 2015/06/03 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Gravitational wave observations will probe nonlinear gravitational interactions and thus enable strong tests of Einstein’s theory of general relativity. We present a numerical relativity study of the late inspiral and merger of binary black holes in scalar–tensor theories of gravity. We consider binaries inside a scalar field bubble, including in some cases a potential. We demonstrate how an evolving scalar field is able to trigger detectable differences between gravitational waves in scalar–tensor gravity and the corresponding waves in general relativity.