We review some recent results concerning non-extremal and extremal stationary, asymptotically flat black hole solutions in extended D = 4 supergravities, and their properties with respect to the global symmetries of the theory. More specifically we refer to the effective three-dimensional description of these solutions and their classification within orbits with respect to the action of the global symmetry group, illustrating, for single-center solutions, the general mathematical relation between the orbits of non-extremal and extremal black holes.

On D=4 Stationary Black Holes / Andrianopoli, Laura Maria; D'Auria, Riccardo; Gallerati, Antonio; Trigiante, Mario. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6588. - STAMPA. - 474:(2013). (Intervento presentato al convegno XXIst International Conference on Integrable Systems and Quantum Symmetries (ISQS21) 12–16 June 2013, Prague, Czech Republic tenutosi a Prague, Czech Republic nel 12–16 June 2013) [10.1088/1742-6596/474/1/012002].

On D=4 Stationary Black Holes

ANDRIANOPOLI, Laura Maria;D'AURIA, RICCARDO;GALLERATI, ANTONIO;TRIGIANTE, MARIO
2013

Abstract

We review some recent results concerning non-extremal and extremal stationary, asymptotically flat black hole solutions in extended D = 4 supergravities, and their properties with respect to the global symmetries of the theory. More specifically we refer to the effective three-dimensional description of these solutions and their classification within orbits with respect to the action of the global symmetry group, illustrating, for single-center solutions, the general mathematical relation between the orbits of non-extremal and extremal black holes.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11583/2556748
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