2009/12/31 by Bernard Kelly, Bernard J. Kelly, Wolfgang Tichy +4 · 2 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics #Binary number #Black Holes and Theoretical Physics #Classical mechanics #Conformal map #Constraint (computer-aided design) #Cosmology #Flatness (cosmology) #General relativity #Geometry #Gravitational wave #Mathematical analysis #Metric (unit) #Newtonian fluid #Numerical relativity #Physics #Pulsars and Gravitational Waves Research #Theoretical physics #gr-qc
paper · pdf · doi:10.1088/0264-9381/27/11/114005
published as Class.Quant.Grav.27:114005,2010 · 13 pages, 9 figures. Invited paper from Numerical Relativity and Data Analysis (NRDA) 2009, Albert Einstein Institute, Potsdam. Corrected to match published version.
arxiv created 2010/05/11 · openalex publication_date 2010/05/11 · arxiv updated 2010/05/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In Kelly et al. [Phys. Rev. D, 76:024008, 2007], we presented new binary black-hole initial data adapted to puncture evolutions in numerical relativity. This data satisfies the constraint equations to 2.5 post-Newtonian order, and contains a transverse-traceless "wavy" metric contribution, violating the standard assumption of conformal flatness. We report on progress in evolving this data with a modern moving-puncture implementation of the BSSN equations in several numerical codes. We discuss the effect of the new metric terms on junk radiation and continuity of physical radiation extracted.