Interaction of Einstein-Maxwell radiation and a cosmic string: Special solutions with hypersurface-orthogonal Killing vectors
- Facultad de Matematica, Astronomia y Fisica, Universidad Nacional de Cordoba, Laprida 854, 5000 Cordoba, Argentina (AR)
We present several nontrivial limits of a new family of exact solutions of the Einstein-Maxwell equations for axisymmetric nonstationary spacetimes, obtained using Alekseev's inverse-scattering method, which we previously interpreted as describing the presence of a rotating cosmic string interacting with electromagnetic and gravitational radiation. The limit in which the {ital C} energy of the solutions goes to infinity is related to a change in their geometry, reminiscent of some results recently found for both gauge and global cosmic strings. The axisymmetry, i.e., the presence of a (quasiregular) symmetry axis,'' is in general lost, except in one case, which includes hypersurface-orthogonal Killing vectors. Its relation to Xanthopoulos's question as to whether the rotation'' can be stopped is discussed. This last case can also be interpreted as a collapsing Melvin electromagnetic universe. We also analyze a particular limit that leads to a vacuum solution with a curvature singularity on the symmetry axis, but asymptotically flat in the radial direction.
- OSTI ID:
- 5912102
- Journal Information:
- Physical Review, D (Particles Fields); (USA), Vol. 43:4; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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GENERAL PHYSICS
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COSMOLOGICAL MODELS
EINSTEIN-MAXWELL EQUATIONS
GEODESICS
GRAVITATIONAL RADIATION
INVERSE SCATTERING PROBLEM
MINKOWSKI SPACE
SOLITONS
SPACE-TIME
UNIVERSE
VACUUM STATES
EQUATIONS
FIELD EQUATIONS
MATHEMATICAL MODELS
MATHEMATICAL SPACE
QUASI PARTICLES
RADIATIONS
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640106* - Astrophysics & Cosmology- Cosmology
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