Spindle solutions with hyperscalars in D = 4 gauged supergravity
4 affiliations
- 1KU Leuven
- 2Imperial College
- 3University of Iceland
- 4University of Crete
Abstract
A bstract : We construct new classes of supersymmetric AdS ₂ × Σ solutions, where Σ = Σ( n N , n S ) is a spindle. Such solutions can arise as the near horizon limit of supersymmetric, accelerating black holes. The solutions are constructed using D = 4 STU U (1) ⁴ gauged supergravity theory coupled to a charged hyperscalar, and can be uplifted to obtain smooth, supersymmetric AdS ₂ × Y ₉ solutions of D = 11 supergravity. We allow ( n N , n S ) to be non-coprime integers, including orbifolds of the round S ² . We also allow the hyperscalar to vanish at the poles. The AdS ₂ solutions with non-vanishing hyperscalar can naturally arise as the endpoint of holographic RG flows, triggered by relevant hyperscalar deformations of the AdS ₂ solutions of the STU model.
Related
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BibTeX
@article{arav2026spindle,
title = {{Spindle solutions with hyperscalars in D = 4 gauged supergravity}},
author = {Igal Arav and Jerome P. Gauntlett and Jaeha Park and Matthew M. Roberts and Christopher Rosen},
journal = {Journal of High Energy Physics},
year = {2026},
month = oct,
doi = {10.1007/jhep10(2026)214},
url = {https://link.springer.com/article/10.1007/JHEP10(2026)214},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Spindle solutions with hyperscalars in D = 4 gauged supergravity
AU - Igal Arav
AU - Jerome P. Gauntlett
AU - Jaeha Park
AU - Matthew M. Roberts
AU - Christopher Rosen
PY - 2026
DA - 2026/10/21
JO - Journal of High Energy Physics
DO - 10.1007/jhep10(2026)214
UR - https://link.springer.com/article/10.1007/JHEP10(2026)214
AB - A bstract : We construct new classes of supersymmetric AdS ₂ × Σ solutions, where Σ = Σ( n N , n S ) is a spindle. Such solutions can arise as the near horizon limit of supersymmetric, accelerating black holes. The solutions are constructed using D = 4 STU U (1) ⁴ gauged supergravity theory coupled to a charged hyperscalar, and can be uplifted to obtain smooth, supersymmetric AdS ₂ × Y ₉ solutions of D = 11 supergravity. We allow ( n N , n S ) to be non-coprime integers, including orbifolds of the round S ² . We also allow the hyperscalar to vanish at the poles. The AdS ₂ solutions with non-vanishing hyperscalar can naturally arise as the endpoint of holographic RG flows, triggered by relevant hyperscalar deformations of the AdS ₂ solutions of the STU model.
SN - 1029-8479
ER -