Curvature Singularities: the Good, the Bad, and the Naked
Steven S. Gubser
TL;DR
The paper investigates which curvature singularities in five-dimensional gravity coupled to scalars are physically admissible within the AdS/CFT framework, focusing on 3+1D Poincaré-invariant geometries and the role of the scalar potential V.A central conjecture is proposed: large curvatures are allowed only when the scalar potential remains bounded above along the solution, a criterion motivated by the existence of near-extremal black-hole generalizations and supported by Coulomb-branch analyses.Through finite-temperature extensions, explicit examples (one, two, and three massive adjoint chirals), and fluctuations analyses, the work links infrared bulk behavior to dual field theory properties, such as Coulomb-branch dynamics and phase structure, and discusses implications for cosmological constant scenarios and brane-world models.
Abstract
Necessary conditions are proposed for the admissibility of singular classical solutions with 3+1-dimensional Poincare invariance to five-dimensional gravity coupled to scalars. Finite temperature considerations and examples from AdS/CFT support the conjecture that the scalar potential must remain bounded above for a solution to be physical. Having imposed some restrictions on naked singularities allows us to comment on a recent proposal for solving the cosmological constant problem.
