An axisymmetric evolution code for the Einstein equations on hyperboloidal slices

Oliver Rinne (1, 2)

1 Centre for Mathematical Sciences
2 King‘s College London

We present the first stable dynamical numerical evolutions of the Einstein equations in terms of a conformally rescaled metric on hyperboloidal hypersurfaces extending to future null infinity. Axisymmetry is imposed in order to reduce the computational cost. The formulation is based on an earlier axisymmetric evolution scheme, adapted to time slices of constant mean curvature. Ideas from a previous study by Moncrief and the author are applied in order to regularize the formally singular evolution equations at future null infinity. Longterm stable and convergent evolutions of Schwarzschild spacetime are obtained, including a gravitational perturbation. The Bondi news function is evaluated at future null infinity.

Mots clés: 04.20.Cv; 04.20.Ha; 04.25.D-; 04.30.-w

Oliver Rinne. An axisymmetric evolution code for the Einstein equations on hyperboloidal slices. Classical and Quantum Gravity, 2010, 27 (3), pp.35014. ⟨10.1088/0264-9381/27/3/035014⟩. ⟨hal-00569776⟩