2012/11/18 by A. Loinger, Loinger, A., Tiziana Marsico +2
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Physics (physics.gen-ph) #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #physics.gen-ph
paper · pdf · doi:10.48550/arxiv.1211.6152
8 pages
arxiv created 2012/11/18 · openalex publication_date 2012/11/18 · arxiv updated 2012/11/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
The computations of numerical relativity make use of (3+1)- decompositions of Einstein field equations. We examine the conceptual characteristics of this method; instances of compact-star binaries are considered. The preeminent role of the geodesic motions is emphasized.