4.4 Article

Light propagation in a plasma on an axially symmetric and stationary spacetime: Separability of the Hamilton-Jacobi equation and shadow

期刊

JOURNAL OF MATHEMATICAL PHYSICS
卷 63, 期 9, 页码 -

出版社

AIP Publishing
DOI: 10.1063/5.0106433

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资金

  1. Charles University Grant Agency [21/11268S]
  2. Czech Grant Agency
  3. Deutsche Forschungsgemeinschaft
  4. [317421]

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This paper investigates the properties of light rays around compact objects surrounded by a plasma, taking into account the effects of strong gravitational fields and dispersive and refractive medium. By using the relativistic Hamiltonian formalism, the authors derive analytical solutions for the light rays and calculate the photon region and shadow. Several specific examples are discussed, including Kerr black holes, Hartle-Thorne spacetime metrics, Melvin universe, and Teo rotating traversable wormhole.
The properties of light rays around compact objects surrounded by a plasma are affected by both strong gravitational fields described by a general-relativistic spacetime and by a dispersive and refractive medium, characterized by the density distribution of the plasma. We study these effects employing the relativistic Hamiltonian formalism under the assumption of stationarity and axisymmetry. The necessary and sufficient conditions on the metric and on the plasma frequency are formulated such that the rays can be analytically determined from a fully separated Hamilton-Jacobi equation. We demonstrate how these results allow us to analytically calculate the photon region and the shadow if they exist. Several specific examples are discussed in detail: the hairy Kerr black holes, the Hartle-Thorne spacetime metrics, the Melvin universe, and the Teo rotating traversable wormhole. In all of these cases, a plasma medium is present as well. Published under an exclusive license by AIP Publishing.

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