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Perturbative and numerical approach to plasma strong lensing

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arxiv 2212.14297 v2 pith:QRPPM4CV submitted 2022-12-29 gr-qc

classification gr-qc
keywords approachassociatedlensgalaxyimagesnumericalperturbativeplasma
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{Using two different approaches, we study imaging in the strong lens regime taking into account the effects of plasmatic environments on light propagation. First, we extend the use of a perturbative approach that allows us to quickly and analytically calculate the position and shape of the images of a circular source lensed by a galaxy. Such approach will be compared with that obtained from the numerical solution of the lens equations. Secondly, we introduce a 3-dimensional spheroidal model to describe the spacetime associated with the dark matter halo around the lens galaxy and an associated optical metric to incorporate the presence of the plasma medium. The (chromatic) deformation on caustic and critical curves and associated multiplicity of images is also analyzed for particular configurations.

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  1. Gravitational shadow and emission spectrum of thin accretion disks in a plasma medium

    gr-qc 2025-05 conditional novelty 6.0 of 10

    A blackbody accretion disk viewed through transparent, rotating plasma produces frequency-dependent shadows and emission maps, with the frequency of the brightest total flux controlled mainly by viewing angle.

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