Hostname: page-component-745bb68f8f-g4j75 Total loading time: 0 Render date: 2025-01-12T14:05:34.234Z Has data issue: false hasContentIssue false
  • English
  • Français

Electromagnetic Waves in the Exterior of a Schwarzschild Black Hole

Published online by Cambridge University Press:  07 February 2017

H. Stephani  and
E. Herlt
H. Stephani
Affiliation:
Sektion Physik, Universität Jena, G.D.R.
E. Herlt
Affiliation:
Sektion Physik, Universität Jena, G.D.R.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using the technique of Debye potentials, the regular (nonstatic) EM fields are found to behave at r = M either as purely ingoing or as purely outgoing waves. After separation the radial equation is treated in the short wavelength approximation.

Type
Part II: Stability and Collapse
Information
Symposium - International Astronomical Union , Volume 64: Gravitational Radiation and Gravitational Collapse , 1974 , pp. 96
Copyright
Copyright © Reidel 1974