Two families of elliptical plasma lenses
arXiv:1907.10787 · doi:10.1093/mnras/stz2073
Abstract
Plasma lensing is the refraction of low-frequency electromagnetic rays due to free electrons in the interstellar medium. Although the phenomenon has a distinct similarity to gravitational lensing, particularly in its mathematical description, plasma lensing introduces other additional features, such as wavelength dependence, radial rather than tangential image distortions, and strong demagnification of background sources. Axisymmetrical models of plasma lenses have been well-studied in the literature, but density distributions with more complicated shapes can provide new and exotic image configurations and increase the richness of the magnification properties. As a first step towards non-axisymmetrical distributions, we study two families of elliptical plasma lens, softened power-law and exponential plasma distributions. We perform numerical studies on each lens model, and present them over a parameter space. In addition to deriving elliptical plasma lens formulae, we also investigate the number of critical curves that the lens can produce by studying the lens parameter space, in particular the dependence on the lensing ellipticity. We find that the introduction of ellipticity into the plasma distribution can enhance the lensing effects as well as the complexity of the magnification map.
14 pages, comments welcome
References in corpus (21)
- A direct empirical proof of the existence of dark matter
- A bright millisecond radio burst of extragalactic origin
- The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius
- Baryon effects on the internal structure of LCDM halos in the EAGLE simulations
- Vertical structure of a supernova-driven turbulent magnetized ISM
- Three-dimensional Features of the Outer Heliosphere Due to Coupling between the Interstellar and Heliospheric Magnetic Field. V. The Bow Wave, Heliospheric Boundary Layer, Instabilities, and Magnetic Reconnection
- Two families of astrophysical diverging lens models
- Gravitational radiospectrometer
- Folded Fields as the Source of Extreme Radio-Wave Scattering in the Galactic Center
- Escape and Trapping of Low-Frequency Gravitationally Lensed Rays by Compact Objects within Plasma
- Extreme Scattering Events Towards Two Young Pulsars
- Modelling and mitigating refractive propagation effects in precision pulsar timing observations
- SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
- Constraining small scale magnetic fields through plasma lensing: Application to the Black widow eclipsing pulsar binary
- Noodle Model for Scintillation Arcs
- The nature of fast radio bursts
- Extreme scattering events from axisymmetric plasma lenses
- First assessment of the binary lens OGLE-2015_BLG-0232
- Dual-Component Plasma Lens Models
- Wave asymptotics and their application to astrophysical plasma lensing
- Scintillation kinks, bumps and wiggles in the radio spectrum of the quasar PMN J1106-3647
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