Extended black holes in strong gravitational waves

Details Extended black holes in strong gravitational waves Extended black holes in strong gravitational waves

2011-01-24

arxiv.org/abs/1101.4455v3

JHEP 1104:105,2011

Physics

High Energy Physics

High Energy Physics - Theory

14 pages; v3: commentary and references extended, published version

Scientific paper

10.1007/JHEP04(2011)105

We describe a large class of solutions in pure gravity, dilaton gravity and supergravity corresponding to extended higher-dimensional black holes with strong (non-linear) gravitational waves propagating along their worldvolume. For pure gravity, the extended black holes are higher-dimensional analogs of the point-like Schwarzschild black hole in four dimensions. For supergravity, they are non-extremal p-branes. The gravitational waves can be both space-filling and localized around the worldvolume of the extended black holes. The solutions we present contain a large number of arbitrary functions of the light-cone time describing the amplitudes of different non-linear gravitational wave modes.

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