We discuss the connection between the construction of Bogomol'nyi bounds and equations in three dimensional gravitational theories and the existence of an underlying N = 2 local supersymmetric structure. We show that, apart from matter self duality equations, a first order equation for the gravitational field (whose consistency condition gives the Einstein equation) can be written as a consequence of the local supersymmetry. Its solvability makes possible the evasion of the no-go scenario for the construction of Killing spinors in asymptotically conical spacetimes. In particular we show that the existence of non-trivial supercovariantly constant spinors is guaranteed whenever field configurations saturate the topological bound.Facultad de C...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
We discuss the 2 + 1 dimensional Abelian Higgs model coupled to N = 2 supergravity. We construct the...
We study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gau...
We initiate a systematic study of the solutions of three-dimensional matter-coupled half-maximal (N=...
The locally supersymmetric extension of the most general gravity theory in three dimensions leading ...
It is shown that, under certain conditions, the existence of a Killing spinor on a bosonic backgroun...
The asymptotic structure of three-dimensional hypergravity without cosmological constant is analyzed...
Bogomolnyi-type bound is constructed for the topological solitons in O(3) nonlinear $\sigma$ model c...
The asymptotic structure of three-dimensional hypergravity without cosmological constant is analyzed...
Witten has argued that in 2+1 dimensions local supersymmetry can ensure the vanishing of the cosmolo...
AbstractWe show how the Killing Spinor Identities (KSI) can be used to reduce the number of independ...
We give a brief overview of black-hole solutions in four-dimensional supergravity theories and their...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
We discuss the 2 + 1 dimensional Abelian Higgs model coupled to N = 2 supergravity. We construct the...
We study the cosmological constant problem in a three-dimensional N = 2 supergravity theory with gau...
We initiate a systematic study of the solutions of three-dimensional matter-coupled half-maximal (N=...
The locally supersymmetric extension of the most general gravity theory in three dimensions leading ...
It is shown that, under certain conditions, the existence of a Killing spinor on a bosonic backgroun...
The asymptotic structure of three-dimensional hypergravity without cosmological constant is analyzed...
Bogomolnyi-type bound is constructed for the topological solitons in O(3) nonlinear $\sigma$ model c...
The asymptotic structure of three-dimensional hypergravity without cosmological constant is analyzed...
Witten has argued that in 2+1 dimensions local supersymmetry can ensure the vanishing of the cosmolo...
AbstractWe show how the Killing Spinor Identities (KSI) can be used to reduce the number of independ...
We give a brief overview of black-hole solutions in four-dimensional supergravity theories and their...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...
There exists two distinct off-shell N = 2 supergravities in three dimensions. They are also referred...