A (Running) Bolt for New Reasons
Iosif Bena, Stefano Giusto, Clement Ruef, Nicholas P. Warner
TL;DR
The paper constructs explicit non-BPS, horizonless five-dimensional geometries—running Bolt and running Taub-Bolt—by magnetizing Euclidean Schwarzschild and Kerr-Taub-Bolt bases within ungauged STU-like supergravity. These solutions share the same charges and mass as corresponding non-extremal black holes and exhibit a mixed time/Kaluza-Klein fiber at infinity; the base can be ambi-polar, enlarging the allowed parameter space and yielding multiple branches. A key finding is that the rest mass can either increase or decrease with added M2 charge, depending on the self-duality of the flux, with anti-self-dual cases even lowering mass without violating energy conservation due to the non-supersymmetric setting. The results provide concrete horizonless microstate geometries that support a fuzzball-like resolution of spacelike singularities for non-extremal black holes and point toward avenues for constructing large multi-bubble non-extremal configurations.
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.
