activity
20022012
most citedFirst-order flow equations for extremal and non-extremal black holes

68 citations · 435 across the 15 of their papers we have counts for

collaborators

15 papers

hep-th2012★ 7 cited

Black hole solutions of N=2, d=4 supergravity with a quantum correction, in the H-FGK formalism

Pietro Galli, Tomas Ortin, Jan Perz +1

We apply the H-FGK formalism to the study of some properties of the general class of black holes in N=2 supergravity in four dimensions that correspond to the harmonic and hyperbol…

hep-th2012★ 9 cited

On anharmonic stabilisation equations for black holes

Pietro Galli, Kevin Goldstein, Jan Perz

We investigate the stabilisation equations for sufficiently general, yet regular, extremal (supersymmetric and non-supersymmetric) and non-extremal black holes in four-dimensional…

hep-th2012★ 36 cited

Black holes and black strings of N=2, d=5 supergravity in the H-FGK formalism

Patrick Meessen, Tomas Ortín, Jan Perz +1

We study general classes and properties of extremal and non-extremal static black-hole solutions of N=2, d=5 supergravity coupled to vector multiplets using the recently proposed H…

hep-th2011★ 35 cited

H-FGK formalism for black-hole solutions of N=2, d=4 and d=5 supergravity

Patrick Meessen, Tomas Ortin, Jan Perz +1

We rewrite the Ferrara-Gibbons-Kallosh (FGK) black-hole effective action of N=2, d=4,5 supergravities coupled to vector multiplets, replacing the metric warp factor and the physica…

hep-th2011★ 28 cited

Non-Extremal Black Holes of N=2,d=5 Supergravity

P. Meessen, T. Ortin

We study the generalization of the Ansatz of Galli et al. for non-extremal black holes of N=2,d=4 supergravities for a simple model of N=2,d=5 supergravity with a vector multiplet…

hep-th2011★ 59 cited

Non-extremal black holes of N=2, d=4 supergravity

Pietro Galli, Tomas Ortin, Jan Perz +1

We propose a generic recipe for deforming extremal black holes into non-extremal black holes and we use it to find and study the non-extremal black-hole solutions of several N=2,d=…