EFFECT OF NUT PARAMETER ON THE ANALYTIC EXTENSION OF THE CAUCHY HORIZON THAT DEVELOP IN COLLIDING WAVE SPACE–TIMES

DOI10.1142/S0217751X09044243zbMath1168.83307arXiv0707.1945OpenAlexW2031635275MaRDI QIDQ3395446

Mustafa Halilsoy, Ozay Gurtug

Publication date: 1 September 2009

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0707.1945

zbMATH Keywords

colliding gravitational wavesKilling-Cauchy horizons

Mathematics Subject Classification ID

String and superstring theories in gravitational theory (83E30) Gravitational waves (83C35)

Related Items (1)

RESTRICTED CLASS OF COLLIDING EINSTEIN–YANG–MILLS PLANE WAVES

Cites Work

• Kerr-de Sitter black holes with NUT charges
• On the physical meaning of the NUT parameter
• On the collision of gravitational plane waves: A class of soliton solutions
• Quantum singularity in quasiregular spacetimes, as indicated by Klein-Gordon, Maxwell and Dirac fields
• A new type of singularity created by colliding gravitational waves
• A note on the parameters of the Kerr–NUT–(anti-)de Sitter spacetime
• Colliding wave solutions from five-dimensional black holes and black p-branes
• Collisions of gravitational and electromagnetic waves that do not develop curvature singularities
• Comments on the instability of black-hole inner horizons
• The most general axially symmetric electrovac spacetime admitting separable equations of motion
• Higher-dimensional resolution of dilatonic black-hole singularities
• Test particle motion in a gravitational plane wave collision background
• Scalar and spinor perturbation to the Kerr–NUT spacetime
• General Kerr–NUT–AdS metrics in all dimensions

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