Polarized synchrotron and self-absorption
Research context
research method · conditional · As of 2026-10-10
For isotropic power-law electrons in a uniform field, optically thin synchrotron has a conditional spectral slope and maximum linear polarization.
Key knowledge
For isotropic power-law electrons in a uniform field, optically thin synchrotron has a conditional spectral slope and maximum linear polarization. A homogeneous self-absorbed power-law source approaches a ν^(5/2) spectrum, while field disorder, Faraday rotation, cooling and cutoffs change observations.
Values and equations
jν∝ν^[-(p-1)/2]; Π_max=(p+1)/(p+7/3); Iν=Sν(1-exp[-τν])
- jν
- Synchrotron emissivity
- ν
- Frequency Hz
- p
- Electron power-law index 1
- Π_max
- Optically thin maximum linear polarization 1
- Iν,Sν
- Specific intensity and source function
- τν
- Optical depth 1
Conditions and scope
- Electron index p and spectral-frequency support must be declared; optically thick polarization differs.
- An observed polarization fraction does not uniquely determine field topology or jet geometry.
- Homogeneous power-law support, uniform field and isotropic pitch angles for the slope/polarization; slab transfer has constant source function and no incident background.
Sources · 2
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
High energy astrophysics: synchrotron radiation I: Power-law radiation and polarization (selected source body inspected). High energy astrophysics: synchrotron radiation: Power-law electrons, spectra and self-absorption (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
Permanent link to this entry ↗- Record identity
- research-earth-synchrotron-polarization
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference