0000000000605352

AUTHOR

Pietro Galli

showing 6 related works from this author

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

2011

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=4 supergravity models (SL(2,R)/U(1), CPn and STU with four charges). In all the cases considered, the non-extremal family of solutions smoothly interpolates between all the different extremal limits, supersymmetric and not supersymmetric. This fact can be used to find explicitly extremal non-supersymmetric solutions in the cases in which the attractor mechanism does not completely fix the values of the scalars on the event horizon and they still depend on the boundary conditions at spatial infinity. We compare (su…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsEvent horizonSupergravitySuperpotentialFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyModuli spaceBlack holeCombinatoricsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)AttractorCentral chargeSymplectic geometryJournal of High Energy Physics
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Non-supersymmetric Extremal Black Holes: First-Order Flows and Stabilisation Equations

2013

We review the results of [1, 2] on reducing the second-order equations of motion for stationary extremal black holes in four-dimensional \({\textit{N}}\,=\,2\) supergravity to first-order flow equations and further to non-differential stabilisation equations.

Black holePhysicsGeneral Relativity and Quantum CosmologyHarmonic functionFlow (mathematics)SupergravityExtremal black holeEquations of motionFirst orderMathematical physics
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Black hole solutions of N=2, d=4 supergravity with a quantum correction, in the H-FGK formalism

2012

We apply the H-FGK formalism to the study of some properties of a general class of black holes in N = 2 supergravity in four dimensions that correspond to the harmonic and hyperbolic ansatze and we obtain explicit extremal and non-extremal solutions for the t(3) model with and without a quantum correction. Not all solutions of the corrected model (quantum black holes), including in particular a solution with a single q(1) charge, have a regular classical limit.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsBlack holes010308 nuclear & particles physicsSupergravityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBlack holes in string theoryGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesClassical limitGeneral Relativity and Quantum CosmologyBlack holeFormalism (philosophy of mathematics)General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesSupersymmetry and DualityQuantum correction010306 general physicsQuantumMathematical physics
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From supersymmetric to non-supersymmetric black holes

2012

Methods similar to those used for obtaining supersymmetric black hole solutions can be employed to find also non-supersymmetric solutions. We briefly review some of them, with the emphasis on the non-extremal deformation ansatz of [1].

PhysicsBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryTheoretical physicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaSupergravityHigh Energy Physics::PhenomenologyExtremal black holeGeneral Physics and AstronomyDeformation (meteorology)AnsatzFortschritte der Physik
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First-order flows and stabilisation equations for non-BPS extremal black holes

2011

28 páginas.-- This article is distributed under the terms of the Creative Commons Attribution Noncommercial License.

PhysicsHigh Energy Physics - TheorySupergravity modelsNuclear and High Energy Physics010308 nuclear & particles physicsSupergravityFOS: Physical sciencesCharge (physics)Black holes in string theoryFirst order01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Flow (mathematics)Harmonic functionPhysics::Plasma Physics0103 physical sciences010306 general physicsMathematical physicsAnsatzJournal of High Energy Physics
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Non-supersymmetric black-hole solutions in N=2,D=4 supergravity

2013

254 páginas. Tesis Doctoral del Departamento de Física Teórica, de la Universidad de Valencia.

General Relativity and Quantum CosmologyUNESCO::FÍSICA::Física Teórica::Teoría cuántica de camposkahler geometry:FÍSICA::Física Teórica::Gravitación [UNESCO]supergravityUNESCO::FÍSICA::Física Teórica::Gravitación:FÍSICA::Física Teórica::Teoría cuántica de campos [UNESCO]black holes
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