vix.ing · top · new · best · stats · spec

Spatial dispersion of light rays propagating through a plasma in Kerr space–time

2019/01/14 by Tom Kimpson, Kinwah Wu, Silvia Zane
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Computational physics #Dispersion (optics) #Dispersion relation #Gravitational wave #Optics #Physics #Plasma #Pulsar #Pulsars and Gravitational Waves Research #Quantum mechanics #Spacetime #astro-ph.HE #gr-qc

paper · pdf · doi:10.1093/mnras/stz138

9 pages, 6 figures. Accepted for publication in MNRAS

openalex publication_date 2019/01/14 · arxiv created 2019/02/05 · arxiv updated 2019/02/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We investigate the propagation of light through a plasma on a background Kerr space–time via a Hamiltonian formulation. The behaviour of light when propagating through a vacuum and through a plasma is not the same; the convolution of gravitational and plasma effects gives rise to a dispersion in both space and time. The magnitude of the dispersion is a strong function of both the ray frequency and impact parameter. We discuss implications for the detection of gravitationally bent pulsar beams near the Galactic centre.

Citations