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Holographic correlators with multi-particle states,

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

3 Pith papers citing it

citation-role summary

background 1

citation-polarity summary

fields

hep-th 2 gr-qc 1

years

2026 2 2025 1

verdicts

UNVERDICTED 3

roles

background 1

polarities

background 1

representative citing papers

Fortuity beyond counting: an explicit construction

hep-th · 2026-06-18 · unverdicted · novelty 6.0

Explicit construction of BPS states in (h,j)=(1,0) sector of D1D5 CFT shows non-vanishing three-point coupling between monotone and fortuitous states, indicating the sectors are dynamically connected.

Towering Gravitons in AdS$_3$/CFT$_2$

hep-th · 2026-04-22 · unverdicted · novelty 5.0

A procedure dresses supergravitons with singletons to extend the BPS gravity-sector spectrum in AdS3/CFT2, yielding affine multiplets that match the D1-D5 CFT better after deformation up to higher levels.

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 3 of 3 citing papers.

  • Fortuity beyond counting: an explicit construction hep-th · 2026-06-18 · unverdicted · none · ref 57

    Explicit construction of BPS states in (h,j)=(1,0) sector of D1D5 CFT shows non-vanishing three-point coupling between monotone and fortuitous states, indicating the sectors are dynamically connected.

  • Towering Gravitons in AdS$_3$/CFT$_2$ hep-th · 2026-04-22 · unverdicted · none · ref 46

    A procedure dresses supergravitons with singletons to extend the BPS gravity-sector spectrum in AdS3/CFT2, yielding affine multiplets that match the D1-D5 CFT better after deformation up to higher levels.

  • Gravitational Atoms from Topological Stars gr-qc · 2025-11-13 · unverdicted · none · ref 24

    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.