We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensional Einstein equations. Using combined numerical and analytical methods we give evidence that within this model the Schwarzschild-Tangherlini black hole is asymptotically stable. In addition, we briefly discuss the critical behavior at the threshold of black-hole formation
We summarise recent results about the gravitational collapse to black holes in higher dimensions. W...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We present results of numerical simulations of the formation of black holes from the gravitational c...
We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensiona...
We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensiona...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
We show that the 4+1 dimensional vacuum Einstein equations admit gravitational waves with radial sym...
We consider the critical behavior at the threshold of black hole formation for the five dimensional ...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We consider the critical behavior at the threshold of black hole formation for the five dimensional ...
While in general relativity black holes can be freely embedded into a cosmological background, the s...
AbstractIn the context of gravitational collapse and black hole formation, we reconsider the problem...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We summarise recent results about the gravitational collapse to black holes in higher dimensions. W...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We present results of numerical simulations of the formation of black holes from the gravitational c...
We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensiona...
We consider the vacuum gravitational collapse for cohomogeneity-two solutions of the nine dimensiona...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
We show that the 4+1 dimensional vacuum Einstein equations admit gravitational waves with radial sym...
We consider the critical behavior at the threshold of black hole formation for the five dimensional ...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
It is fair to say that our current mathematical understanding of the dynamics of gravitational colla...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We consider the critical behavior at the threshold of black hole formation for the five dimensional ...
While in general relativity black holes can be freely embedded into a cosmological background, the s...
AbstractIn the context of gravitational collapse and black hole formation, we reconsider the problem...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We summarise recent results about the gravitational collapse to black holes in higher dimensions. W...
In the gravitational collapse of matter beyond spherical symmetry, gravitational waves are necessari...
We present results of numerical simulations of the formation of black holes from the gravitational c...