Abstract
The comoving-frame equations of radiative transfer and moment equations to accurate terms of all orders inv/c are derived in the modified Lagrangian form. The equations exactly describe the interaction of radiation with matter in a relativistically moving medium in flat or curved spacetime. Two specialized sets of equations are presented: (1) the equation of radiative transfer and moment equations accurate to terms of second order (v 2/c 2), and (2) the transfer equation and moment equations for a radial flow in curved spacetime with the Schwarzschild-type metric.
Similar content being viewed by others
References
Anderson, J. L. and Spiegel, E. A.: 1972,Astrophys. J. 171, 127.
Kaneko, N., Morita, K., and Maekawa, M.: 1984,Astrophys. Space Sci. 107, 333.
Lindquist, R. W.: 1966,Ann. Phys. 37, 487.
Mihalas, D.: 1980,Astrophys. J. 237, 574.
Misner, C. W., Thorne, K. S., and Wheeler, J. A.: 1973,Gravitation, W. H. Freeman Co., San Francisco.
Pomraning, G. C.: 1975,Radiation Hydrodynamics, Pergamon Press, Oxford.
Thorne, K. S.: 1981,Monthly Notices Roy. Astron. Soc. 194, 439.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Morita, K., Kaneko, N. The comoving-frame equation of radiative transfer in relativistic flows. Astrophys Space Sci 121, 105–125 (1986). https://doi.org/10.1007/BF00648265
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00648265