Collisions of gravitational and electromagnetic waves that do not develop curvature singularities

DOI10.1063/1.528615zbMath0667.53063OpenAlexW1969916183MaRDI QIDQ3819675

Basilis C. Xanthopoulos, T. Papacostas

Publication date: 1989

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.528615

zbMATH Keywords

electromagnetic wavesgravitational wavesEinstein-Maxwell equations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of global differential geometry to the sciences (53C80) Electromagnetic fields in general relativity and gravitational theory (83C50)

Related Items (2)

Linear perturbations of plane polarized plane waves. I. The absence of purely incoming perturbations ⋮ EFFECT OF NUT PARAMETER ON THE ANALYTIC EXTENSION OF THE CAUCHY HORIZON THAT DEVELOP IN COLLIDING WAVE SPACE–TIMES

Cites Work

• A class of solutions of Einstein-Maxwell equations
• Rotating, charged, and uniformly accelerating mass in general relativity
• A new type of singularity created by colliding gravitational waves
• On the Nutku—Halil solution for colliding impulsive gravitational waves
• On colliding waves that develop time–like singularities: a new class of solutions of the Einstein–Maxwell equations
• A perturbation analysis of the Bell-Szekeres space-time
• Orthogonal transitivity, invertibility, and null geodesic separability in type D electrovac solutions of Einstein’s field equations with cosmological constant
• On colliding waves in the Einstein—Maxwell theory

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