Polarization of Light: Astrophysical Processes & Mechanisms

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    Light Polarization
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Discussion Overview

The discussion centers on the astrophysical processes that can lead to the polarization of light, encompassing various mechanisms across the electromagnetic spectrum, from gamma rays to radio waves.

Discussion Character

  • Exploratory, Technical explanation

Main Points Raised

  • Some participants mention scattering, synchrotron emission, and Kerr rotation as processes that can result in light polarization.
  • One participant elaborates that polarization occurs whenever there is anisotropy in matter-radiation interactions, suggesting that ideal spherical symmetry is required to avoid polarization.
  • Basic processes leading to polarization include elastic scattering on free electrons and inelastic scattering on atoms, with the polarization state changing unless scattering occurs in specific directions.
  • The presence of magnetic or electric fields can complicate the polarization state, which can be utilized for diagnostics through effects like the Zeeman and Hanle effects.
  • Impact atomic polarization is introduced as a phenomenon where the polarization state of atoms changes due to anisotropic collisions, affecting the emitted radiation.
  • Bremsstrahlung is mentioned as a general result of charged particle acceleration contributing to polarization.

Areas of Agreement / Disagreement

Participants present multiple competing views on the processes and mechanisms of light polarization, with no consensus reached on a definitive list or explanation.

Contextual Notes

Some limitations include the dependence on specific definitions of polarization and the complexity of interactions that may not be fully resolved in the discussion.

RJ Emery
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What astrophysical processes can result in the polarization of light, and by what mechanisms is that accomplished? (By light, I mean any form of EM waves, from gamma to radio.)
 
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Scattering, synchrotron emission, Kerr rotation, ... no doubt there are more as well.
 
There are many sources of polarization in the universe. Roughly speaking, photons polarization emerges whenever any kind of anisotropy in matter-radiation interaction appears. It is easier to find an answer to the question of what processes do not lead to the light polarization: You need an ideal spherical symmetry of the interaction to avoid light polarization. Even in this case, photons are polarized, but the total polarization is zero due to cancellations of large number of observed photons (distant spherical star free of magnetic fields would produce unpolarized radiation).
Basic processes which lead to polarization include elastic scattering on free electrons (atoms, molecules, ...) (the polarization state of a scattered photon is always changed unless it scatters in the forward/backward direction), inelastic scattering on atoms. In the presence of magnetic or electric fields the polarization state can be modified in a very complicated manner and it can be used for detailed diagnostics of the state of the distant object - Zeeman and Hanle effect. Another phenomenon is so-called impact atomic polarization (polarization state of atoms is changed by anisotropical collisions with charged perturbers hence the emitted radiation is also polarized), bremsstrahlung (in a general sense as a result of charged particle acceleration)
 
Nereid and kocour,

I greatly appreciate the listing of the various processes and their elaboration.
 

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