Numerical solution of the 2 + 1 Teukolsky equation on a hyperboloidal and horizon penetrating foliation of Kerr and application to late-time decays

DOI10.1088/0264-9381/30/11/115013zbMath1271.83006arXiv1301.1591OpenAlexW3105783201MaRDI QIDQ2841448

Sebastiano Bernuzzi, Enno Harms, Bernd Brügmann

Publication date: 25 July 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1301.1591

zbMATH Keywords

extremal black holes Kerr future null infinity Teukolsky equation power-law decay

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75) Analogues of general relativity in lower dimensions (83C80) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (8)

Axisymmetric fully spectral code for hyperbolic equations ⋮ Computing the quasinormal modes and eigenfunctions for the Teukolsky equation using horizon penetrating, hyperboloidally compactified coordinates ⋮ A GPU-accelerated mixed-precision WENO method for extremal black hole and gravitational wave physics computations ⋮ Intermediate behavior of Kerr tails ⋮ The evolution of hyperboloidal data with the dual foliation formalism: mathematical analysis and wave equation tests ⋮ Hyperboloidal framework for the Kerr spacetime ⋮ Discontinuous collocation methods and gravitational self-force applications ⋮ Noether currents for the Teukolsky master equation

Uses Software

Teukode

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