Equations of general relativistic radiation hydrodynamics in Kerr space-time

@inproceedings{Takahashi2007EquationsOG,
  title={Equations of general relativistic radiation hydrodynamics in Kerr space-time},
  author={Ryoji Takahashi},
  year={2007}
}
Equations of fully general relativistic radiation hydrodynamics in Kerr space-time are derived. While the interactions between matter and radiation are introduced in the comoving frame, the derivatives used when describing the global evolutions of both the matter and the radiation are given in the Boyer-Lindquist frame (BLF) which is a frame fixed to the coordinate describing the central black hole. Around a rotating black hole, both the matter and the radiation are influenced by the frame… CONTINUE READING
BETA

Citations

Publications citing this paper.

References

Publications referenced by this paper.
SHOWING 1-4 OF 4 REFERENCES

The Equations of Radiation Hydrodynamics (Oxford; New York: Pergamon

Park M.-G
  • Schinder P. J.,
  • 2006
VIEW 4 EXCERPTS
HIGHLY INFLUENTIAL

Black-Hole Accretion Disks (Kyoto

C. Gammie, R. Popham
  • Ann. Phys.,
  • 1998
VIEW 1 EXCERPT

The Physics of Astrophysics Vol. 1: Radiation (California: University Science Books

J. Schmid-Burgk
  • Ap& SS,
  • 1978
VIEW 1 EXCERPT

Similar Papers

Loading similar papers…