Abstract
The exact two-parameter solution of Einsteins equations described below represents ingoing and outgoing cylindrical gravitational waves with two degrees of polarization. It has been obtained from the Kerr metric by applying a well-known trick but, unlike the Kerr metric, it has no singularities.
| Original language | English |
|---|---|
| Pages (from-to) | 331-332 |
| Number of pages | 2 |
| Journal | Physical Review D |
| Volume | 34 |
| Issue number | 2 |
| DOIs | |
| State | Published - 1986 |