The polarization of strongly lensed point-like radio sources
Fuente:
arXiv
Saved in:
| Main Author: | |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866916781937917952 |
|---|---|
| author | Er, Xinzhong |
| author_facet | Er, Xinzhong |
| contents | Aims. The magnetized medium induces birefringence, splitting the light into two distinct wave modes. The differing propagation speeds of the two modes result in different trajectories. Strong gravitational lensing amplifies the birefringence and introduces an additional geometric rotation on top of the Faraday rotation. We compare the geometric rotation with the Faraday rotation. Methods. We construct the lens equation for massive objects in a magnetized plasma environment, and calculate the time delay difference between the two modes using two toy examples. We present that in the strong lensed radio sources, birefringence causes geometric rotation, which is a non-negligible effect, even with a weak magnetic field. Results. In both examples, the geometric delay causes a comparable or stronger rotation than the Faraday rotation and show a similar dependence on the wavelength of the signal. For a point lens with a strong magnetic field, the two wave modes exhibit distinct behaviours. The polarization of lensed sources can provide additional insights into the magnetic field and plasma environment. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_05772 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The polarization of strongly lensed point-like radio sources Er, Xinzhong Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena Aims. The magnetized medium induces birefringence, splitting the light into two distinct wave modes. The differing propagation speeds of the two modes result in different trajectories. Strong gravitational lensing amplifies the birefringence and introduces an additional geometric rotation on top of the Faraday rotation. We compare the geometric rotation with the Faraday rotation. Methods. We construct the lens equation for massive objects in a magnetized plasma environment, and calculate the time delay difference between the two modes using two toy examples. We present that in the strong lensed radio sources, birefringence causes geometric rotation, which is a non-negligible effect, even with a weak magnetic field. Results. In both examples, the geometric delay causes a comparable or stronger rotation than the Faraday rotation and show a similar dependence on the wavelength of the signal. For a point lens with a strong magnetic field, the two wave modes exhibit distinct behaviours. The polarization of lensed sources can provide additional insights into the magnetic field and plasma environment. |
| title | The polarization of strongly lensed point-like radio sources |
| topic | Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2506.05772 |