Abstract
The 3+1 split of general relativity has been used to investigate the dispersion relation for certain plasma waves, together with the two stream instability, in the vicinity of a Schwarzschild black hole horizon. In contrast to the special relativistic results, the dispersion relations discussed here contain additional terms involving the gravitational acceleration, a, and the lapse function {alpha}. Some of these terms are imaginary and should correspond to gravitational damping effects. 5 refs.
Buzzi, V;
Hines, K C;
[1]
Treumann, R A
[2]
- Melbourne Univ., Parkville (Australia). School of Physics
- Max-Planck-Institut fuer Extraterrestrische Physik, Garching (Germany)
Citation Formats
Buzzi, V, Hines, K C, and Treumann, R A.
Two fluid plasmas in the vicinity of a Schwarzschild black hole.
Australia: N. p.,
1992.
Web.
Buzzi, V, Hines, K C, & Treumann, R A.
Two fluid plasmas in the vicinity of a Schwarzschild black hole.
Australia.
Buzzi, V, Hines, K C, and Treumann, R A.
1992.
"Two fluid plasmas in the vicinity of a Schwarzschild black hole."
Australia.
@misc{etde_10109296,
title = {Two fluid plasmas in the vicinity of a Schwarzschild black hole}
author = {Buzzi, V, Hines, K C, and Treumann, R A}
abstractNote = {The 3+1 split of general relativity has been used to investigate the dispersion relation for certain plasma waves, together with the two stream instability, in the vicinity of a Schwarzschild black hole horizon. In contrast to the special relativistic results, the dispersion relations discussed here contain additional terms involving the gravitational acceleration, a, and the lapse function {alpha}. Some of these terms are imaginary and should correspond to gravitational damping effects. 5 refs.}
place = {Australia}
year = {1992}
month = {Dec}
}
title = {Two fluid plasmas in the vicinity of a Schwarzschild black hole}
author = {Buzzi, V, Hines, K C, and Treumann, R A}
abstractNote = {The 3+1 split of general relativity has been used to investigate the dispersion relation for certain plasma waves, together with the two stream instability, in the vicinity of a Schwarzschild black hole horizon. In contrast to the special relativistic results, the dispersion relations discussed here contain additional terms involving the gravitational acceleration, a, and the lapse function {alpha}. Some of these terms are imaginary and should correspond to gravitational damping effects. 5 refs.}
place = {Australia}
year = {1992}
month = {Dec}
}