A (Running) Bolt for New Reasons

Abstract

We construct a four-parameter family of smooth, horizonless, stationary solutions of ungauged five-dimensional supergravity by using the four-dimensional Euclidean Schwarzschild metric as a base space and "magnetizing" its bolt. We then generalize this to a five-parameter family based upon the Euclidean Kerr-Taub-Bolt. These "running Bolt" solutions are necessarily non-static. They also have the same charges and mass as a non-extremal black hole with a classically-large horizon area. Moreover, in a certain regime their mass can decrease as their charges increase. The existence of these solutions supports the idea that the singularities of non-extremal black holes are resolved by low-mass modes that correct the singularity of the classical black hole solution on large (horizon-sized) scales.

25 pages, 3 figures, LaTeX; v2: minor changes, references added

References in corpus (14)

• The fuzzball proposal for black holes
• Black Holes as Effective Geometries
• Fuzzballs with internal excitations
• Bicycling Black Rings
• Mergers and Typical Black Hole Microstates
• Radiation from the non-extremal fuzzball
• Plumbing the Abyss: Black Ring Microstates
• Almost BPS black holes
• Orthogonal black di-ring solution
• Non-supersymmetric microstates of the D1-D5-KK system
• Pair creation in non-extremal fuzzball geometries
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• Generating technique for $U(1{)}^{3}5D$ supergravity
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• Non-extremal Black Hole Microstates: Fuzzballs of Fire or Fuzzballs of Fuzz ?
• Deforming the D1D5 CFT away from the orbifold point
• Excitations in the deformed D1D5 CFT
• Supergravity Solutions from Floating Branes
• The information paradox and the infall problem
• Topological Stars and Black Holes
• Topological Stars, Black holes and Generalized Charged Weyl Solutions
• Fuzzballs and Observations
• Metastable Supertubes and non-extremal Black Hole Microstates
• Supersymmetric black lenses in five dimensions
• Integrability of Five Dimensional Minimal Supergravity and Charged Rotating Black Holes
• The Nuts and Bolts of Einstein-Maxwell Solutions
• Non-BPS multi-bubble microstate geometries
• First-order flows and stabilisation equations for non-BPS extremal black holes
• Black hole non-uniqueness via spacetime topology in five dimensions
• Structure of Six-Dimensional Microstate Geometries
• Analyzing the squeezed state generated by a twist deformation
• Floating JMaRT
• The Cheshire Cap
• Non-BPS Floating Branes and Bubbling Geometries
• Inverse Scattering and the Geroch Group
• Non-supersymmetric extremal multicenter black holes with superpotentials
• Hair in the Back of a Throat: Non-Supersymmetric Multi-Center Solutions from Kähler Manifolds
• Mind the Gap: Supersymmetry Breaking in Scaling, Microstate Geometries
• Duality covariant non-BPS first order systems
• Non-supersymmetric Microstates of the MSW System
• A bubbling bolt
• Insane Anti-Membranes?
• An Inverse Scattering Construction of the JMaRT Fuzzball
• Intertwining Relations for the Deformed D1D5 CFT
• New Supersymmetric Bubbles on AdS_3xS^3
• New instability of non-extremal black holes: spitting out supertubes
• Phases of non-extremal multi-centered bound states
• Hot Attractors
• Asymptotically flat multi-black lenses
• Non-Supersymmetric, Multi-Center Solutions with Topological Flux
• Soliton mechanics
• Imaginary Soaring Branes: A Hidden Feature of Non-Extremal Solutions
• Smooth non-extremal D1-D5-P solutions as charged gravitational instantons
• Instabilities of microstate geometries with antibranes
• Generalized Hot Attractors
• Unwinding of strings thrown into a fuzzball
• Topological Sources of Soliton Mass and Supersymmetry Breaking
• Brane Resolution Through Fibration
• The Hot Attractor Mechanism: Decoupling Without Deep Throats