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Post-Newtonian initial data with waves: progress in evolution. (English) Zbl 1190.83035
Summary: In [B. J. Kelly et al., Phys. Rev. D 76 024008 (2007)], we presented new binary black-hole initial data adapted to puncture evolutions in numerical relativity. These data satisfy the constraint equations to 2.5 post-Newtonian order, and contain a transverse-traceless ‘wavy’ metric contribution, violating the standard assumption of conformal flatness. We report on progress in evolving these 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.
Reviewer: Reviewer (Berlin)

MSC:
83C35 Gravitational waves
83C25 Approximation procedures, weak fields in general relativity and gravitational theory
83C05 Einstein’s equations (general structure, canonical formalism, Cauchy problems)
83C57 Black holes
85A25 Radiative transfer in astronomy and astrophysics
83-08 Computational methods for problems pertaining to relativity and gravitational theory
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