Analytic extension in colliding waves with NUT parameter, Yang-Mills fields and extra dimen.pdf
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Analytic extension in colliding waves with NUT parameter, Yang-Mills fields and extra dimen
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Analytic extension in colliding waves with NUT parameter,
Yang-Mills fields and extra dimensions
Ozay Gurtug? and Mustafa Halilsoy?
Department of Physics, Eastern Mediterranean University,
G. Magusa, north Cyprus, via Mersin 10, Turkey.
Abstract
The Cauchy horizon forming colliding wave solution due to Chandrasekhar and Xanthopoulos
(CX) has been generalized by inclusion of the NUT ( Newman - Unti - Tamburino) parameter.
This is done by transforming the part of the inner horizon region of a Kerr-Newman-NUT black
hole into the space of colliding waves. By taking appropriate combination of Killing vectors and
analytically extending beyond the Cauchy horizon the time-like hyperbolic sigularities are resolved
as well. This provides another example of its kind among the type - D metrics with special emphasis
on the role of the NUT parameter. By applying a non-Abelian gauge transformation we show that
the same CX metric describes also collision of Einstein-Yang-Mills (EYM) plane waves with cross
polarization. Finally, it is shown that horizons of colliding higher dimensional plane waves obtained
from the black p-branes undergoes a similar procedure of analytic extension.
?Electronic address: ozay.gurtug@emu.edu.tr
?Electronic address: mustafa.halilsoy@emu.edu.tr
1
I. INTRODUCTION
Colliding gravitational waves (CGW) in general relativity constitutes one of the out-
standing subjects that nonlinear effects of the Einstein’s theory of relativity are manifestly
displayed. The prototype exact solutions suggested that when two plane gravitational waves
collide, they focus each other in a way that after a finite time from the instant of the collision,
a space-time singularity develops [1]. In contrast to this view, exceptional solutions were
found which do not exhibit curvature singularities; instead, they develop Killing - Cauchy
horizons [2]. Under what conditions the collision of waves produce a space-ti
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