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Ray-tracing and polarized radiative transfer in General Relativity
Published online by Cambridge University Press: 23 June 2017
Abstract
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We discuss the problem of polarized radiative transfer in general relativity. We present a set of equations suitable for solving the problem numerically for the case of an arbitrary space-time metric, and show numerical solutions to example problems. The solutions are computed with a new ray-tracing code, Arcmancer, developed by the authors.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 347 - 350
- Copyright
- Copyright © International Astronomical Union 2017
References
Novikov, I. D. & Thorne, K. S.
1973, in: DeWitt, C. & DeWitt, B. S. (eds.) Astrophysics of Black Holes, Black Holes (New York: Gordon and Breach), p. 343
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