BibTex format
@article{Arav:2026:10.1007/jhep10(2026)214,
author = {Arav, I and Gauntlett, JP and Park, J and Roberts, MM and Rosen, C},
doi = {10.1007/jhep10(2026)214},
journal = {Journal of High Energy Physics},
title = {Spindle solutions with hyperscalars in D = 4 gauged supergravity},
url = {http://dx.doi.org/10.1007/jhep10(2026)214},
volume = {2026},
year = {2026}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - <jats:title> A <jats:sc>bstract</jats:sc> </jats:title> <jats:p> We construct new classes of supersymmetric <jats:italic>AdS</jats:italic> <jats:sub>2</jats:sub> × Σ solutions, where Σ = Σ( <jats:italic>n</jats:italic> <jats:sub> <jats:italic>N</jats:italic> </jats:sub> , <jats:italic>n</jats:italic> <jats:sub> <jats:italic>S</jats:italic> </jats:sub> ) is a spindle. Such solutions can arise as the near horizon limit of supersymmetric, accelerating black holes. The solutions are constructed using <jats:italic>D</jats:italic> = 4 STU <jats:italic>U</jats:italic> (1) <jats:sup>4</jats:sup> gauged supergravity theory coupled to a charged hyperscalar, and can be uplifted to obtain smooth, supersymmetric <jats:italic>AdS</jats:italic> <jats:sub>2</jats:sub> × <jats:italic>Y</jats:italic> <jats:sub>9</jats:sub> solutions of <jats:italic>D</jats:italic> = 11 supergravity. We allow ( <jats:italic>n</jats:italic> <jats:sub> <jats:italic>N</jats:italic> </jats:sub> , <jats:italic&
AU - Arav,I
AU - Gauntlett,JP
AU - Park,J
AU - Roberts,MM
AU - Rosen,C
DO - 10.1007/jhep10(2026)214
PY - 2026///
TI - Spindle solutions with hyperscalars in D = 4 gauged supergravity
T2 - Journal of High Energy Physics
UR - http://dx.doi.org/10.1007/jhep10(2026)214
UR - https://doi.org/10.1007/jhep10(2026)214
VL - 2026
ER -