We use zero angular momentum null geodesics in the Kerr–de Sitter spacetime to transform the metric in a generalised Bondi coordinate system. We write the metric components explicitly. Next, we… Click to show full abstract
We use zero angular momentum null geodesics in the Kerr–de Sitter spacetime to transform the metric in a generalised Bondi coordinate system. We write the metric components explicitly. Next, we choose the radial coordinate to be the areal coordinate and write the asymptotic metric in the Bondi–Sachs gauge.
               
Click one of the above tabs to view related content.