An interpretation of Robinson-Trautmann type N solutions
The Robinson-Trautmann type N solutions, which describe expanding gravitational waves, are investigated for all possible values of the cosmological constant A and the curvature parameter E. The wave surfaces are always (hemi-)spherical, with successive surfaces displaced in a way which depends on E....
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| Main Authors: | , , |
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| Format: | Default Preprint |
| Published: |
2002
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| Subjects: | |
| Online Access: | https://hdl.handle.net/2134/460 |
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