We argue that the main feature behind novel properties of higher-dimensional black holes, compared to four-dimensional ones, is that their horizons can have two characteristic lengths of very different size. We develop a long-distance world-volume effective theory that captures the black hole dynamics at scales much larger than the short scale. In this limit the black hole is regarded as a blackfold: a black brane (possibly boosted locally) whose world volume spans a curved submanifold of the spacetime. This approach reveals black objects with novel horizon geometries and topologies more complex than the black ring, but more generally it provides a new organizing framework for the dynamics of higher-dimensional black holes
In a companion paper [1], we have presented a cross-correlation approach to near-horizon physics in ...
The AdS/CFT correspondence provides a microscopic description of black hole thermodynamics. In this ...
A particle in four dimensions should behave like a classical black hole if the horizon radius is lar...
We argue that the main feature behind novel properties of higher-dimensional black holes, compared t...
We construct several classes of worldvolume effective actions for black holes by integrating out spa...
The application of the blackfold effective theory to the perturbative construction of black holes in...
We initiate a systematic scan of the landscape of black holes in any spacetime dimension using the r...
Abstract. In models with large extra dimensions that accommodate a TeV-scale gravity Einstein’s equa...
We argue that the effective theory describing the long-wavelength dynamics of black branes is the sa...
The scale at which quantum gravity becomes manifest, the species scale $\Lambda_s$, has recently bee...
We discuss the properties of black holes in brane-world scenarios where our universe is viewed as a ...
By investigating the critical behavior appearing at the extremal limit of the non-dilatonic, black p...
This thesis is divided into three Parts. In Part I the general theory of black holes in higher dimen...
We point out that in the limit of large number of dimensions a wide class of non-extremal neutral bl...
In this thesis we present a new aspect pertaining to the effective field theory of general relativity...
In a companion paper [1], we have presented a cross-correlation approach to near-horizon physics in ...
The AdS/CFT correspondence provides a microscopic description of black hole thermodynamics. In this ...
A particle in four dimensions should behave like a classical black hole if the horizon radius is lar...
We argue that the main feature behind novel properties of higher-dimensional black holes, compared t...
We construct several classes of worldvolume effective actions for black holes by integrating out spa...
The application of the blackfold effective theory to the perturbative construction of black holes in...
We initiate a systematic scan of the landscape of black holes in any spacetime dimension using the r...
Abstract. In models with large extra dimensions that accommodate a TeV-scale gravity Einstein’s equa...
We argue that the effective theory describing the long-wavelength dynamics of black branes is the sa...
The scale at which quantum gravity becomes manifest, the species scale $\Lambda_s$, has recently bee...
We discuss the properties of black holes in brane-world scenarios where our universe is viewed as a ...
By investigating the critical behavior appearing at the extremal limit of the non-dilatonic, black p...
This thesis is divided into three Parts. In Part I the general theory of black holes in higher dimen...
We point out that in the limit of large number of dimensions a wide class of non-extremal neutral bl...
In this thesis we present a new aspect pertaining to the effective field theory of general relativity...
In a companion paper [1], we have presented a cross-correlation approach to near-horizon physics in ...
The AdS/CFT correspondence provides a microscopic description of black hole thermodynamics. In this ...
A particle in four dimensions should behave like a classical black hole if the horizon radius is lar...