A hyperboloidal method for numerical simulations of multidimensional nonlinear wave equations: nonlinear tails
Oliver Rinne
TL;DR
The paper develops and implements a hyperboloidal, conformally compactified framework to numerically study the nonlinear wave equation $\Box \Phi = \mu |\Phi|^{p-1}\Phi$ in $n+1$ dimensions without full spherical symmetry for $n=3$ and with SO$(n-1)$ symmetry in higher dimensions. It derives a regular first-order system for the rescaled field $\tilde{\Phi}$ and its conjugate $\tilde{\Pi}$ on hyperboloidal slices, establishing regularity at future null infinity $\mathrsfs{I}^+$ and an energy balance that accounts for energy flux through $\mathrsfs{I}^+$. Numerically, the authors employ a hybrid discretisation (radial fourth-order finite differences with angular pseudo-spectral methods), RK4 time stepping, Kreiss-Oliger dissipation, and Orszag 2/3 filtering to evolve the system up to $\mathrsfs{I}^+$. They compute tail decay exponents $q_{lm}$ across subcritical, critical, and supercritical regimes in $n=3$ and $n=5$ with SO$(n-1)$ symmetry, finding mode-dependent exponents that are independent of the azimuthal index in 3D and that agree with conjectured finite-radius and $\mathrsfs{I}^+$ scaling relations, thereby extending previous radial results to nonradial settings and highlighting the method's capacity to probe nonlinear tails in multi-dimensional NLWs.
Abstract
We consider the scalar wave equation with power nonlinearity in n+1 dimensions. Unlike most previous numerical studies, we go beyond the radial case and do not assume any symmetries for n=3, and we only impose an SO(n-1) symmetry in higher dimensions. Our method is based on a hyperboloidal foliation of Minkowski spacetime and conformal compactification. We focus on the late-time power-law decay (tails) of the solutions and compute decay exponents for different spherical harmonic modes, for subcritical, critical and supercritical, focusing and defocusing nonlinear wave equations.
