Freely propagating polarized radiation in curved space-times

Details Freely propagating polarized radiation in curved space-times Freely propagating polarized radiation in curved space-times

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219...25b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. 25-28.

Statistics

Computation

5

Computational Astrophysics, Cosmology, Polarized Radiation, Radiative Transfer, Space-Time Functions, Angular Momentum, Gravitational Effects, Relativity, Schwarzschild Metric, Stokes Law Of Radiation

Scientific paper

The comoving frame transfer equations for the Stokes-parameters measured by an arbitrary observer in an arbitrary background metric are derived in an Eulerian coordinate system, which for a wide range of problems in radiation hydrodynamics is the most adequate to describe the motion of matter. Explicit expressions are given for a Bianchi type I cosmological model and a Kerr metric with small angular momentum.

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