2002/01/07 by Shahar Hod
Earth and Planetary Sciences · Physics and Astronomy · #Computational physics #Mechanics #Optics #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Scattering #Seismic Imaging and Inversion Techniques #Seismic Waves and Analysis #Statistical physics #Time evolution #gr-qc
paper · pdf · doi:10.1103/physrevd.66.024001
published as Phys.Rev. D66 (2002) 024001 · 4 pages, 2 figures
arxiv created 2002/01/07 · openalex publication_date 2002/06/26 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
It is well known that waves propagating under the influence of a scattering potential develop ``tails.'' However, the study of late-time tails has so far been restricted to time-independent backgrounds. In this paper, we explore the late-time evolution of spherical waves propagating under the influence of a time-dependent scattering potential. It is shown that the tail structure is modified due to the temporal dependence of the potential. The analytical results are confirmed by numerical calculations.