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No-horizon theorem for spacetimes with spacelikeG1isometry groups
2003
Classical and quantum gravity
We consider four-dimensional spacetimes (M, g) which obey the Einstein equations G= T, and admit a global spacelike G_1= R isometry group. By means of dimensional reduction and local analyis on the reduced (2+1) spacetime, we obtain a sufficient condition on T which guarantees that (M, g) cannot contain apparent horizons. Given any (3+1) spacetime with spacelike translational isometry, the no-horizon condition can be readily tested without the need for dimensional reduction. This provides thus
doi:10.1088/0264-9381/20/24/012
fatcat:kdanpbvs7fah7bzx2xqwoyrt5u