POLARIZED SYNCHROTRON EMISSIVITIES and ABSORPTIVITIES for RELATIVISTIC THERMAL, POWER-LAW, and KAPPA DISTRIBUTION FUNCTIONS

Alex Pandya, Zhaowei Zhang, Mani Chandra, Charles F. Gammie

Research output: Contribution to journalArticlepeer-review

Abstract

Synchrotron emission and absorption determine the observational appearances of many astronomical systems. In this paper, we describe a numerical scheme for calculating synchrotron emissivities and absorptivities in all four Stokes parameters for arbitrary gyrotropic electron distribution functions, building on earlier work by Leung, Gammie, and Noble. We use this technique to evaluate the emissivities and the absorptivities for a thermal (Maxwell-Jü ttner), isotropic power-law, and an isotropic kappa distribution function. The latter contains a power-law tail at high particle energies that smoothly merges with a thermal core at low energies, as is characteristic of observed particle spectra in collisionless plasmas. We provide fitting formulae and error bounds on the fitting formulae for use in codes that solve the radiative transfer equation. The numerical method and the fitting formulae are implemented in a compact C library called symphony. We find that the kappa distribution has a source function that is indistinguishable from a thermal spectrum at low frequency and transitions to the characteristic self-absorbed synchrotron spectrum, , at high frequency; the linear polarization fraction for a thermal spectrum is near unity at high frequency; and all distributions produce O(10%) circular polarization at low frequency for lines of sight sufficiently close to the magnetic field vector.

Original languageEnglish (US)
Article number34
JournalAstrophysical Journal
Volume822
Issue number1
DOIs
StatePublished - May 1 2016

Keywords

  • plasmas
  • polarization
  • radiation mechanisms: general
  • radiative transfer
  • relativistic processes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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