The geometry of null rotation identifications
Joan Simon
TL;DR
This work analyzes Minkowski space quotiented by a null rotation, creating a Lorentzian orbifold that preserves half of the supersymmetry while avoiding closed timelike curves away from a lightlike singular locus. It establishes a geometric picture of the null-rotation quotient, shows that closed causal curves are absent for $x^- eq 0$, and reveals a deep link to the BTZ black hole via a double-scaling limit. In string/M-theory, the quotient can be embedded, yielding dilatonic waves and offering a resolution of the singularity through nullbranes, with a broader extension to curved backgrounds possessing SO$(1,2)$ isometries. The results point to a universal, supersymmetric sector of time-dependent backgrounds with potential applications to cosmological and brane dynamics in string theory.
Abstract
The geometry of flat spacetime modded out by a null rotation (boost+rotation) is analysed. When embedding this quotient spacetime in String/M-theory, it still preserves one half of the original supersymmetries. Its connection with the BTZ black hole, supersymmetric dilatonic waves and one possible resolution of its singularity in terms of nullbranes are also discussed.
