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Momentum Fractionation on Superstrata

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Superstrata are bound states in string theory that carry D1, D5, and momentum charges, and whose supergravity descriptions are parameterized by arbitrary functions of (at least) two variables. In the D1-D5 CFT, typical three-charge states reside in high-degree twisted sectors, and their momentum charge is carried by modes that individually have fractional momentum. Understanding this momentum fractionation holographically is crucial for understanding typical black-hole microstates in this system. We use solution-generating techniques to add momentum to a multi-wound supertube and thereby construct the first examples of asymptotically-flat superstrata. The resulting supergravity solutions are horizonless and smooth up to well-understood orbifold singularities. Upon taking the AdS3 decoupling limit, our solutions are dual to CFT states with momentum fractionation. We give a precise proposal for these dual CFT states. Our construction establishes the very nontrivial fact that large classes of CFT states with momentum fractionation can be realized in the bulk as smooth horizonless supergravity solutions.

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citation-polarity summary

fields

gr-qc 1 hep-th 1

years

2026 1 2025 1

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UNVERDICTED 2

roles

background 1

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representative citing papers

Chaos of Berry curvature for BPS microstates

hep-th · 2026-04-25 · unverdicted · novelty 7.0

Berry curvature of BPS states is random-matrix-like for supersymmetric black hole microstates but non-random and often zero for horizonless geometries, offering a chaos diagnostic in degenerate sectors.

Gravitational Atoms from Topological Stars

gr-qc · 2025-11-13 · unverdicted · novelty 5.0

Bound states of a massive scalar field around topological stars form strictly normal modes, producing a hydrogen-like spectrum when the Compton wavelength exceeds the star size and localized states otherwise.

citing papers explorer

Showing 2 of 2 citing papers.

  • Chaos of Berry curvature for BPS microstates hep-th · 2026-04-25 · unverdicted · none · ref 80

    Berry curvature of BPS states is random-matrix-like for supersymmetric black hole microstates but non-random and often zero for horizonless geometries, offering a chaos diagnostic in degenerate sectors.

  • Gravitational Atoms from Topological Stars gr-qc · 2025-11-13 · unverdicted · none · ref 15 · internal anchor

    Bound states of a massive scalar field around topological stars form strictly normal modes, producing a hydrogen-like spectrum when the Compton wavelength exceeds the star size and localized states otherwise.