A characterization of strong wave tails in curved spacetimes

DOI10.1088/0264-9381/14/5/030zbMath0873.53069arXivgr-qc/9703031OpenAlexW2066552824MaRDI QIDQ4341014

Brien C. Nolan

Publication date: 16 June 1997

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9703031

zbMATH Keywords

backscatteringelectromagnetic fieldsasymptotically flat spacetimespropagation of radiationwave tails

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Electromagnetic fields in general relativity and gravitational theory (83C50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (2)

Optical geometry analysis of the electromagnetic self-force ⋮ Scalar and vector tail radiation from the interior of the lightcone

This page was built for publication: A characterization of strong wave tails in curved spacetimes