Post-Newtonian freely specifiable initial data for binary black holes in numerical relativity
Post-Newtonian freely specifiable initial data for binary black holes in numerical relativity
Construction of astrophysically realistic initial data remains a central problem when modelling the merger and eventual coalescence of binary black holes in numerical relativity. The objective of this paper is to provide astrophysically realistic freely specifiable initial data for binary black hole systems in numerical relativity, which are in agreement …