activity
19972026
most citedNumerical evolution of axisymmetric, isolated systems in General Relativity

22 citations · 69 across the 10 of their papers we have counts for

collaborators

10 papers

gr-qc2026

Fully global numerical evolutions of the linearised spin-2 equation

Merlyn Barrer, Jörg Frauendiener, Jörg Hennig +3

We study the linearised spin-2 field on conformally compactified Minkowski spacetime. Initial data are prescribed on past null infinity , and the system is evolved t…

gr-qc2026

A note on the conformal geometry of the 2-sphere

Jörg Frauendiener

We discuss the geometry of the two-dimensional sphere. Our perspective focuses on the set of conformal factors that rescale a given metric to a round metric. We find that there exi…

gr-qc2025

Fully non-linear gravitational wave simulations from past to future null-infinity

Jörg Frauendiener, Chris Stevens, Sebenele Thwala

We present the first numerical simulations of asymptotically flat space-times whose computational domain includes past and future null-infinity. As an application, we explore the s…

gr-qc2025

A numerical framework for studying asymptotic quantities

Breanna Camden, Jörg Frauendiener, Joseph Galinski +3

In this contribution we present an overview of our work on the numerical simulation of the perturbation of a black hole space-time by incoming gravitational waves. The formulation…

gr-qc2023

The non-linear perturbation of a black hole by gravitational waves. III. Newman-Penrose constants

Jörg Frauendiener, Alex Goodenbour, Chris Stevens

In this paper we continue our study of the non-linear response of a Schwarzschild black hole to an ingoing gravitational wave by computing the Newman-Penrose (NP) constants. The NP…

gr-qc2022★ 15 cited

The non-linear perturbation of a black hole by gravitational waves. II. Quasinormal modes and the compactification problem

Jörg Frauendiener, Chris Stevens

Recently, Friedrich's Generalized Conformal Field Equations (GCFE) have been implemented numerically and global quantities such as the Bondi energy and the Bondi-Sachs mass loss ha…