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June 4, 2026Journal of High Energy Physics0 citationsOpen Access

Spindle solutions, hyperscalars and smooth uplifts

IAIgal AravJGJerome P. GauntlettMRMatthew M. Roberts

Key Points

  • This research aims to construct and investigate AdS 3 × Y 7 solutions in type IIB supergravity with new hyperscalar characteristics.
  • Solutions are constructed using D = 5 STU U(1)3 gauged supergravity.
  • Exploration includes spindle solutions with non-coprime integers (nN, nS).
  • The hyperscalar behavior at the poles is analyzed for impact on U(1)B flux.
  • New hyperscalar AdS 3 solutions can arise from RG flows triggered by relevant hyperscalar deformations.
  • Findings reveal non-unique uplifts distinguished by hyperscalar spectra for magnetic flux through the spindle.
  • Investigating orbifolds of round S2 has led to the discovery of inequivalent solutions.

Abstract

A bstract We construct AdS 3 × Y 7 solutions of type IIB supergravity, where Y 7 is a smooth S 5 bundle over a spindle Σ( n N , n S ), which are dual to 𝒩 = (0, 2) SCFTs in d = 2. The solutions are constructed using the D = 5 STU U (1) 3 gauged supergravity theory coupled to a hyperscalar charged under U (1) B . We investigate spindle solutions with two new features: first, we allow ( n N , n S ) to be non-coprime integers, including orbifolds of the round S 2 , which can lead to non-unique, inequivalent uplifts, distinguished by the hyperscalar spectra, for given magnetic flux through the spindle. Second, we also allow the hyperscalar to vanish at the poles leading to solutions carrying non-vanishing U (1) B flux. The new hyperscalar AdS 3 solutions can naturally arise as the endpoint of RG flows, triggered by relevant hyperscalar deformations of the AdS 3 solutions of the STU model.

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Cite This Study

Arav et al. (2026) studied this question.

synapsesocial.com/papers/6a2115f6d499ed480b16ef52https://doi.org/10.1007/jhep06(2026)010
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