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REVIEW 2 major objections 4 minor 2 cited by

Integer dual dimensions in scale-separated AdS$_3$ from massive IIA

T0 review · 2 major / 4 minor · reviewed 2026-08-08 · deepseek-v4-flash

Pith's one-line read In the formal limit, all eight closed-string scalar dual dimensions are integers {8,4,4,4,4,2,2,2}.

desk verdict Solid EFT-level construction with genuinely new flux choices and a useful Joyce-orbifold idea; the smeared-backreaction caveat is real but openly acknowledged. read the letter →

arxiv 2502.08215 v2 pith:R6HYGEUO submitted 2025-02-12 hep-th

classification hep-th
keywords AdS3fluxvacuamassivetypeIIAG2orbifoldsscaleseparationintegerconformaldimensionsmodulistabilizationsmearedorientifoldsT^7/Z2^3
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper studies three-dimensional anti-de Sitter (AdS$_3$) flux vacua of massive type IIA string theory (the ten-dimensional supergravity with a nonzero $F_0$ flux) on G2 orbifolds, and asks whether the light closed-string scalar fields have operator dimensions in the conjectured dual CFT that are integers, a pattern seen in other scale-separated string vacua. The authors show that on two closely related $T^7/\mathbb{Z}_2^3$ orbifolds with the orientifold planes smeared rather than localized, specific flux choices make every untwisted scalar satisfy $\Delta_A = 1+\sqrt{1+m_A^2 L^2} = \{8,4,4,4,4,2,2,2\}$ in the formal limit where the string coupling vanishes and the internal volume is infinite. One of the two orbifolds admits a known desingularization into a smooth G2 manifold, and resolving the singularities may remove the intersecting orientifold planes that otherwise threaten the smeared-source approximation. The paper also exhibits a flux configuration with all moduli stabilized; its mass spectrum approaches these integers parametrically as a large integer $G$ tends to infinity, so the integer dimensions are statements about a limit rather than about finite flux values.

What carries the argument

The load-bearing object is the 3D $\mathcal{N}=1$ effective superpotential for G2 orientifold compactifications, $$P = \frac{m}{8}$e^{{\frac{y}}${2}-\frac{\sqrt{7}}{2}x}+\frac{h}{8}$e^{{y+\frac{x}}${\sqrt{7}}}\left(\frac{1}{\tilde{s}_1}+\frac{1}{\tilde{s}_2}+\frac{1}{\tilde{s}_3}\right)-\frac{f}{8}$e^{{y-\frac{x}}${\sqrt{7}}}\left(\tilde{s}_4+\tilde{s}_5+\tilde{s}_6+\frac{1}{\prod_{a=1}^6\tilde{s}_a}\right),$$ together with the harmonic 3-form and 4-form bases $\Phi_i,\Psi_i$ of the G2 orbifold and a shift parameter $c\in\{0,1/2\}$ distinguishing the two orbifold types. Extremizing $P$ fixes the eight scalar fields $\phi^A=(x,y,\tilde{s}_1,\ldots,\tilde{s}_6)$; the masses are the eigenvalues of the normalized Hessian $\langle K^{AB}\rangle^{-1}\langle V_{BC}\rangle/|\langle V\rangle|$, and the relation $\Delta_A = 1+\sqrt{1+m_A^2 L^2}$ converts those eigenvalues into dual conformal dimensions. The second key ingredient is a generalized $F_4$ flux with an integer parameter $G$ that breaks a shift symmetry, removes the flat direction, and reduces to the simpler integer-dimension flux as $G\to\infty$.

What would settle it

Compute the first-order backreaction of the localized O6-planes for these flux choices---for example, by finding localized profiles in the singular and desingularizable orbifolds---and recompute the normalized Hessian of the scalar potential. If the mass eigenvalues deviate from $\{48,8,8,8,8,0,0,0\}$ by a nonvanishing amount that does not vanish as $G\to\infty$, the integer spectrum is an artifact of the smeared approximation and fails as a statement about the actual vacuum.

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Extended reading notes

Core claim

The central claim is that the untwisted closed-string scalar sector of these scale-separated AdS$_3$ vacua can be arranged by choosing fluxes so that every scalar mass squared in units of the AdS scale matches the values $$$m_A^{2}$ $L^{2}$ = \{48,8,8,8,8,0,0,0\},$$ which through the AdS/CFT relation $\Delta_A = 1+\sqrt{1+m_A^2 L^2}$ gives the integer conformal dimensions $$\Delta_A = \{8,4,4,4,4,2,2,2\}.$$ This is shown for both the singular $c=0$ orbifold and the desingularizable $c=1/2$ orbifold, which admit the same flux ansatz and produce the same untwisted spectrum. The paper further shows that adding $F_4$ flux along the remaining harmonic four-forms lifts the flat direction of the simpler flux choice and stabilizes all eight moduli, with the normalized Hessian converging to the matrix that yields the integer spectrum as a single large integer flux $G\to\infty$; at any finite $G$ the dimensions are only parametrically close to integers, exactly as in all other known examples.

Load-bearing premise

The computation treats the orientifold planes as spread out uniformly rather than concentrated along their worldvolumes; if their true localized backreaction cannot be captured this way, or if it shifts the untwisted scalar masses, the integer conformal dimensions would not describe a real string vacuum.

Editorial extensions

If this is right

  • In the formal limit $G\to\infty$, the fully stabilized vacuum has $g_s\sim G^{-3/2}$, string-frame volume $\sim G^{7/2}$, and $L_{\mathrm{KK}}^2/L_{\mathrm{AdS}}^2\sim G^{-2}$, so weak coupling, large volume, and parametric scale separation coexist.
  • The singular $c=0$ and desingularizable $c=1/2$ orbifolds give the same untwisted closed-string spectrum and the same integer dual dimensions for the same flux choices.
  • The normalized mass eigenvalues $\{48,8,8,8,8,0,0,0\}$ translate to dual dimensions $\{8,4,4,4,4,2,2,2\}$; this equality is exact only in the asymptotic limit, with corrections of order $1/G$ at finite flux.
  • The simple flux choice of Section 3 leaves one flat direction that would be lifted by higher-order corrections; the more general flux of Section 4 stabilizes all eight moduli while preserving the asymptotic integer spectrum.
  • If the known desingularization of the $c=1/2$ orbifold removes orientifold intersections, the smeared-source approximation may be more defensible in this construction than in the singular case.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Beyond the paper: if the integer spectrum survives in the resolved orbifold, a first-order backreaction calculation in this construction would provide a concrete test of whether the smeared approximation is the leading-order description of a real vacuum.
  • Beyond the paper: the same $\Delta_A$ values appearing for both orbifolds and being independent of the anisotropy parameter $n$ suggests the integers are fixed by the G2 structure-form topology and the tadpole algebra, not by flux magnitudes; enumerating all flux vectors satisfying the same Bianchi identities could test this.
  • Beyond the paper: the pattern $\{8,4,4,4,4,2,2,2\}$ may reflect the arithmetic of the $\mathbb{Z}_2^3$ action on the seven-torus, with the $c=1/2$ shift making some involutions freely acting; a scan over $\mathbb{Z}_2^k$ orbifolds could reveal whether integer dimensions always accompany such shifts.
  • Beyond the paper: since only the untwisted sector is treated, computing twisted-sector masses after blowing up the singularities would show whether integer dimensions are a property of the putative dual CFT or an artifact of the truncation; the paper leaves this open.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

2 major / 4 minor

Summary. The manuscript studies supersymmetric, scale-separated AdS3 flux vacua of massive IIA on T7/Z2^3 G2 orbifolds with smeared O2/O6 planes, comparing a 'singular' orbifold with c=0 and a Joyce-type orbifold with c=1/2. Using the 3D N=1 superpotential of [43], the authors specialize to H3 parallel to the O6 currents, Romans mass F0, and specific F4 components, solve the F-term equations analytically, and verify weak coupling, large internal volume, and parametric scale separation. The normalized Hessian gives m^2 L^2 = {48,8,8,8,8,0,0,0}, hence conformal dimensions Delta = {8,4,4,4,4,2,2,2} in the classical smeared untwisted sector. An anisotropic F4 variant is shown to preserve these dimensions. In Section 4, the authors add extra F4 components and adjust the D2-brane/tadpole contribution, breaking the flat direction of the simpler solution; with N = (2/5)G^2 and n = 5/G they find an analytic one-parameter family that stabilizes the eight scalars of the truncation. As G tends to infinity, the kinetic and mass matrices approach those of the integer-dimensional solution, so the dual dimensions are parametrically close to integers while g_s tends to zero and the volume diverges. The paper explicitly states that the backreaction of localized intersecting O6-planes and the twisted sector are not addressed.

Significance. The algebraic core of the paper is coherent: no free parameter is fitted to obtain the integer spectrum, the flux quantization conditions are made explicit, the Section 4 solution is fully analytic, and the parametric scalings are consistent with the stated limits. If the smeared orientifold approximation is a reliable leading-order description, or if the Joyce blow-up removes the O6 intersections as suggested by [24], the paper would be a distinctive addition to the AdS3 scale-separation literature, extending the known integer-conformal-dimension pattern to minimal-supersymmetry AdS3 vacua. The paper is also commendably transparent about its main weaknesses, namely the unresolved backreaction of intersecting smeared O6-planes and the restriction to the untwisted sector. The significance is therefore conditional on a physical assumption that is not established in the manuscript.

major comments (2)
  1. [Sec. 2.1, eqs. (2.8)-(2.10); Sec. 5] The load-bearing physical assumption is the existence of the localized 10D background. Equations (2.8)-(2.10) impose tadpole cancellation with smeared source currents, and the entire mass spectrum is computed in the effective theory built from this smeared configuration. Sections 2.1 and 5 acknowledge that the backreaction of the mutually intersecting O6-planes remains open, and reference [23] shows that localized intersecting sources can fail to admit a supergravity solution. Since the title and abstract present these as scale-separated AdS3 vacua of massive IIA, the manuscript should either provide evidence that the smeared limit is a controlled leading-order approximation, for example through a first-order backreaction analysis along the lines of [44] or through an explicit blow-up of the Joyce orbifold showing that the sources cease to intersect, or it should rescope the conclusions to the smeared classical truncation and state clearly that the string-vacuum realization is an open assumption. As it stands, the existence of the vacuum is an assumption rather than a result.
  2. [Sec. 4.2, eqs. (4.14)-(4.20)] The exact integer values are recovered only in the limit G -> infinity, and this is the same limit in which the determinant in (4.14) vanishes; the fully stabilized solution therefore degenerates at the point where the spectrum is exactly integer. For every finite G the stabilized vacuum has dimensions that are only parametrically close to integers. The paper is transparent about this, but the logical structure should be made explicit in the abstract and introduction: the exactly integer spectrum (3.17) is a property of the simpler, classically unstabilized vacuum of Section 3, while the fully stabilized vacuum of Section 4 has approximate integers and tends to that unstabilized solution only as G -> infinity. As written, the reader may infer that a single fully stabilized AdS3 vacuum has exactly integer conformal dimensions.
minor comments (4)
  1. [Abstract] The first sentence says the flux choices 'yield integer dual dimensions,' while the last sentence says the dimensions are 'only parametrically close to integer values.' This is consistent once the formal limit is specified, but the phrasing invites confusion; the abstract should state explicitly that exact integers occur only in the classical smeared truncation or in the formal G -> infinity limit.
  2. [Sec. 4.2, eq. (4.18)] The object displayed in (4.18) is called the 'normalized Hessian,' but it appears to be the second-derivative matrix divided by |V|; the physical mass eigenvalues require multiplication by K^{-1} as in (3.16). Since the kinetic matrix is given separately in (4.19), the text should clarify that the physical mass matrix is K^{-1} V / |V| in the G -> infinity limit.
  3. [Sec. 3.3, eq. (3.24)] The radii r_i in (3.24) are introduced without a definition; the text should state whether they are string-frame or Einstein-frame radii and to which torus coordinates they refer.
  4. [References and notation] Reference [29] is incomplete, as it lacks a title. In addition, the symbol N is used both for the flux quantum in (2.15) and for the large F4 flux in Section 4; please disambiguate these two uses.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the integer conformal dimensions are outputs of an algebraic Hessian computation for chosen quantized fluxes, not inputs or fitted parameters.

full rationale

The derivation chain is self-contained at the level of the effective theory. The superpotential (3.4) is imported from the authors' earlier work [43], but that citation is independent support: [43] derives the N=1 superpotential for general G2-orientifold flux choices under stated smeared-source and untwisted-sector assumptions, and its derivation does not assume the target integer spectrum. Given that superpotential, the fluxes in (2.13)-(2.14) are fixed by the O6 tadpole structure (2.10), the vacuum moduli are solved algebraically in (3.11), and the normalized Hessian (3.16) is computed directly; the dimensions (3.17) follow from the standard AdS/CFT relation Delta = 1 + sqrt(1 + m^2 L^2). No parameter is fitted to make the eigenvalues {48,8,8,8,8,0,0,0} integer; the integers emerge from the coefficients 1,3,4 in the flux-aligned superpotential (3.10). The anisotropic example (3.18)-(3.20) and the full-moduli-stabilization example of Section 4 are likewise explicit flux choices solved analytically; eqs. (4.20)-(4.22) show the large-G limit tends to the earlier integer-dimension solution, and the paper is transparent that exact integer values are only attained in the formal limit g_s to 0 with corrections eliminated. The open backreaction question for smeared intersecting O6-planes (Sections 2.1 and 5) is a physical validity risk, not a circularity: it concerns whether the effective vacuum lifts to a 10D string background, not whether the claimed spectrum was used as an input.

Assumptions & free parameters 0 free parameters · 5 assumptions · 0 invented entities

The central claim rests on the effective supergravity derived in [43], the smeared-source approximation, and the standard AdS/CFT dictionary. No continuous free parameters are fitted: the flux integers are quantized inputs, and the integer-dimension spectrum is independent of their values in the formal limit.

assumptions (5)
  • domain assumption The 3D N=1 superpotential (3.4) from [43] correctly describes the untwisted closed-string scalar dynamics of massive IIA on the G2 orientifolds considered here.
    This is the starting point of the whole analysis; if the dimensional reduction is corrected by additional terms, the mass spectrum and hence the operator dimensions would change. Entered in Section 3.1.
  • domain assumption Smeared orientifold sources provide a valid leading-order description of the O2/O6-plane backreaction.
    The tadpole conditions (2.8)-(2.10) are imposed with smeared currents, and localized backreaction is not computed; acknowledged as open in Section 5.
  • domain assumption The standard AdS3/CFT2 mass-dimension relation Delta = 1 + sqrt(1 + m^2 L^2) applies to these scalar operators.
    Used in eq. (3.17) to convert the normalized Hessian eigenvalues to conformal dimensions; assumes the scalars are dual to scalar operators in a standard unitary CFT.
  • domain assumption Flux quantization rules h=(2pi)^2 K, m=(2pi)^{-1} M, f=(2pi)^3 N with KM=16 (eq. (2.15)) are the correct quantization conditions in this background.
    Used to justify integrality of the flux parameters and the analytic solution in Section 4.
  • domain assumption The untwisted cohomology basis Phi_i, Psi_i with the intersection property int Phi_i ^ Psi_j = delta_ij is complete for the fields retained in the truncation.
    Underlies the superpotential (3.10) and the orthogonality used in Section 2; twisted-sector forms are ignored.

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Pith. "Pith review of Integer dual dimensions in scale-separated AdS$_3$ from massive IIA." pith.science (2026). https://pith.science/paper/R6HYGEUO

@misc{pith2026250208215,
  author       = {Pith},
  title        = {Pith review of: Integer dual dimensions in scale-separated AdS$_3$ from massive IIA},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/R6HYGEUO}},
  note         = {Machine review of arXiv:2502.08215}
}
abstract

We study supersymmetric scale-separated AdS$_3$ flux vacua of massive IIA on G2 orbifolds with smeared orientifold planes. We consider two types of $T^7/Z_2^3$ orbifolds which, with appropriate flux choices, yield integer dual dimensions for the operators corresponding to the closed string scalar fields in the dual CFT. As with all other known examples, the dual conformal dimensions are only parametrically close to integer values.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On the branes behind scale-separated AdS$_{3}$ flux vacua

    hep-th 2026-06 conditional novelty 6.5 of 10

    Scale-separated supersymmetric AdS3 flux vacua of type IIB G2-orientifolds arise as the near-horizon region of codimension-one smeared D1-D5-KK5 intersections.

  2. Warped G$_2$-throats in IIA and uplift dSillusions

    hep-th 2025-05 conditional novelty 6.0 of 10

    Anti-D2 brane uplifting of classical AdS3 vacua in IIA on G2 orientifolds is forbidden by O6 tadpole constraints, so dS3 must rely on quantum corrections to no-scale Minkowski vacua.

Reference graph

Works this paper leans on

51 extracted references · 7 canonical work pages · cited by 2 Pith papers

  1. [43]

    No-scale and sca le-separated flux vacua from IIA on G2 orientifolds

    F. Farakos, G. Tringas and T. Van Riet, “No-scale and sca le-separated flux vacua from IIA on G2 orientifolds”, Eur. Phys. J. C 80, no.7, 659 (2020) [arXiv:2005.05246 [hep-th]]

  2. [23]

    On the absence of supergravity solutions for localized, intersecting sources

    J. Bardzell, K. Federico, D. Smith and T. Wrase, “On the a bsence of su- pergravity solutions for localized, intersecting sources ,” JHEP 06, 083 (2024) [arXiv:2403.09873 [hep-th]]

  3. [24]

    A note on O6 intersections in AdS flux vacua ,

    D. Junghans, “A note on O6 intersections in AdS flux vacua ,” JHEP 02 (2024), 126 [arXiv:2310.17695 [hep-th]]

  4. [44]

    O6-plane backrea ction on scale-separated Type IIA AdS 3 vacua,

    M. Emelin, F. Farakos and G. Tringas, “O6-plane backrea ction on scale-separated Type IIA AdS 3 vacua,” JHEP 07, 133 (2022) [arXiv:2202.13431 [hep-th]]

  5. [1]

    AdS and the Swampland

    D. Lüst, E. Palti and C. Vafa, “AdS and the Swampland”, Phy s. Lett. B 797 (2019) 134867 [arXiv:1906.05225 [hep-th]]

  6. [2]

    Beginners lectures on flux c ompactifications and related Swampland topics,

    T. Van Riet and G. Zoccarato, “Beginners lectures on flux c ompactifications and related Swampland topics,” Phys. Rept. 1049, 1-51 (2024) [arXiv:2305.01722 [hep- th]]

  7. [3]

    Hiding the extra dimensions: A review on scale separation in string theory,

    T. Coudarchet, “Hiding the extra dimensions: A review on scale separation in string theory,” Phys. Rept. 1064, 1-28 (2024) [arXiv:2311.12105 [hep-th]]

  8. [4]

    Type I IA moduli stabiliza- tion

    O. DeWolfe, A. Giryavets, S. Kachru and W. Taylor, “Type I IA moduli stabiliza- tion”, JHEP 07 (2005), 066 [arXiv:hep-th/0505160 [hep-th]]

Show all 51 references
  1. [5]

    Fluxes, moduli fixi ng and MSSM-like vacua in a simple IIA orientifold,

    P. G. Camara, A. Font and L. E. Ibanez, “Fluxes, moduli fixi ng and MSSM-like vacua in a simple IIA orientifold,” JHEP 09, 013 (2005) [arXiv:hep-th/0506066 [hep-th]]

  2. [6]

    General N = 1 supersymmetric flu x vacua of (massive) type IIA string theory,

    K. Behrndt and M. Cvetic, “General N = 1 supersymmetric flu x vacua of (massive) type IIA string theory,” Phys. Rev. Lett. 95, 021601 (2005) [arXiv:hep-th/0403049 [hep-th]]

  3. [7]

    General N=1 supersymmetric flu xes in massive type IIA string theory,

    K. Behrndt and M. Cvetic, “General N=1 supersymmetric flu xes in massive type IIA string theory,” Nucl. Phys. B 708, 45-71 (2005) [arXiv:hep-th/0407263 [hep- th]]

  4. [8]

    Superpotentials in IIA compactifications with general fluxes,

    J. P. Derendinger, C. Kounnas, P. M. Petropoulos and F. Zw irner, “Superpotentials in IIA compactifications with general fluxes,” Nucl. Phys. B 715, 211-233 (2005) [arXiv:hep-th/0411276 [hep-th]]

  5. [9]

    N=1 effective potential fro m dual type-IIA D6/O6 orientifolds with general fluxes,

    G. Villadoro and F. Zwirner, “N=1 effective potential fro m dual type-IIA D6/O6 orientifolds with general fluxes,” JHEP 06, 047 (2005) [arXiv:hep-th/0503169 [hep- th]]

  6. [10]

    A Landscape of AdS Flux Va cua,

    F. Marchesano and J. Quirant, “A Landscape of AdS Flux Va cua,” JHEP 12, 110 (2019) [arXiv:1908.11386 [hep-th]]

  7. [11]

    Scale- separated AdS4 vacua of IIA orientifolds and M-theory,

    N. Cribiori, D. Junghans, V. Van Hemelryck, T. Van Riet a nd T. Wrase, “Scale- separated AdS4 vacua of IIA orientifolds and M-theory,” Phy s. Rev. D 104, no.12, 126014 (2021) [arXiv:2107.00019 [hep-th]]

  8. [12]

    Weak G2 manifolds and scale separati on in M-theory from type IIA backgrounds,

    V. Van Hemelryck, “Weak G2 manifolds and scale separati on in M-theory from type IIA backgrounds,” Phys. Rev. D 110, no.10, 10 (2024) [arXiv:2408.16609 [hep-th]]. 16

  9. [13]

    M-theory and Type IIA Flux Comp actifications,

    J. McOrist and S. Sethi, “M-theory and Type IIA Flux Comp actifications,” JHEP 12, 122 (2012) [arXiv:1208.0261 [hep-th]]

  10. [14]

    Remarks on scale separation in flux vacua

    F. F. Gautason, M. Schillo, T. Van Riet and M. Williams, “ Remarks on scale separation in flux vacua”, JHEP 03 (2016), 061 [arXiv:1512.00457 [hep-th]]

  11. [15]

    On scale separatio n in type II AdS flux vacua

    A. Font, A. Herráez and L. E. Ibáñez, “On scale separatio n in type II AdS flux vacua”, JHEP 03, 013 (2020) [arXiv:1912.03317 [hep-th]]

  12. [16]

    Quantum corrections to D GKT and the Weak Gravity Conjecture,

    M. Montero and I. Valenzuela, “Quantum corrections to D GKT and the Weak Gravity Conjecture,” [arXiv:2412.00189 [hep-th]]

  13. [17]

    O-Plane Backreaction and Scale Separati on in Type IIA Flux Vacua

    D. Junghans, “O-Plane Backreaction and Scale Separati on in Type IIA Flux Vacua”, Fortsch. Phys. 68 (2020) 6, 2000040 [arXiv:2003.06274 [hep-th]]

  14. [18]

    On supersymmetric AdS 4 orientifold vacua

    F. Marchesano, E. Palti, J. Quirant and A. Tomasiello, “ On supersymmetric AdS 4 orientifold vacua”, JHEP 08 (2020), 087 [arXiv:2003.13578 [hep-th]]

  15. [19]

    Extensions of a scale-separ ated AdS 4 solution and their mass spectrum,

    D. Andriot and G. Tringas, “Extensions of a scale-separ ated AdS 4 solution and their mass spectrum,” JHEP 01, 008 (2024) [arXiv:2310.06115 [hep-th]]

  16. [20]

    Consistency conditions for O-plane unsmea ring from second-order per- turbation theory,

    M. Emelin, “Consistency conditions for O-plane unsmea ring from second-order per- turbation theory,” JHEP 12, 025 (2024) [arXiv:2407.12717 [hep-th]]

  17. [21]

    Smeared versus localised sources in flux compacti fications

    J. Blaback, U. H. Danielsson, D. Junghans, T. Van Riet, T . Wrase and M. Za- germann, “Smeared versus localised sources in flux compacti fications”, JHEP 12 (2010), 043 [arXiv:1009.1877 [hep-th]]

  18. [22]

    Smearing orientifolds in flux compactifications can be OK

    S. Baines and T. Van Riet, “Smearing orientifolds in flux compactifications can be OK”, Class. Quant. Grav. 37 (2020) no.19, 195015 [arXiv:2005.09501 [hep-th]]

  19. [25]

    New families of scale separated vacua,

    R. Carrasco, T. Coudarchet, F. Marchesano and D. Prieto , “New families of scale separated vacua,” JHEP 11, 094 (2023) [arXiv:2309.00043 [hep-th]]

  20. [26]

    Anisotropic scale-separated AdS 4 flux vacua,

    G. Tringas, “Anisotropic scale-separated AdS 4 flux vacua,” [arXiv:2309.16542 [hep- th]]

  21. [27]

    Ad S scale separation and the distance conjecture,

    G. Shiu, F. Tonioni, V. Van Hemelryck and T. Van Riet, “Ad S scale separation and the distance conjecture,” JHEP 05, 077 (2023) [arXiv:2212.06169 [hep-th]]. 17

  22. [28]

    Co nnecting flux vacua through scalar field excursions,

    G. Shiu, F. Tonioni, V. Van Hemelryck and T. Van Riet, “Co nnecting flux vacua through scalar field excursions,” Phys. Rev. D 109, no.6, 6 (2024) [arXiv:2311.10828 [hep-th]]

  23. [29]

    Palti and N

    E. Palti and N. Petri, JHEP 06, 019 (2024) doi:10.1007/JHEP06(2024)019 [arXiv:2405.01084 [hep-th]]

  24. [30]

    Weak gravity versus sca le separation

    N. Cribiori and G. Dall’Agata, “Weak gravity versus sca le separation”, JHEP 06 (2022), 006 [arXiv:2203.05559 [hep-th]]

  25. [31]

    Supergravity EFTs and swam pland constraints,

    N. Cribiori and F. Farakos, “Supergravity EFTs and swam pland constraints,” PoS CORFU2022, 167 (2023) [arXiv:2304.12806 [hep-th]]

  26. [32]

    On the Conforma l Field Theory Duals of type IIA AdS(4) Flux Compactifications,

    O. Aharony, Y. E. Antebi and M. Berkooz, “On the Conforma l Field Theory Duals of type IIA AdS(4) Flux Compactifications,” JHEP 02, 093 (2008) [arXiv:0801.3326 [hep-th]]

  27. [33]

    Exploring the holo graphic Swampland

    J. P. Conlon, S. Ning and F. Revello, “Exploring the holo graphic Swampland”, JHEP 04 (2022), 117 [arXiv:2110.06245 [hep-th]]

  28. [34]

    Comments on classical AdS flux vacua with scale separation

    F. Apers, M. Montero, T. Van Riet and T. Wrase, “Comments on classical AdS flux vacua with scale separation”, JHEP 05, 167 (2022) [arXiv:2202.00682 [hep-th]]

  29. [35]

    Integer c onformal dimensions for type IIa flux vacua

    F. Apers, J. P. Conlon, S. Ning and F. Revello, “Integer c onformal dimensions for type IIa flux vacua”, Phys. Rev. D 105 (2022) no.10, 106029 [arXiv:2202.09330 [hep-th]]

  30. [36]

    Noninteger conformal dimensions for type IIA flux vacua

    J. Quirant, “Noninteger conformal dimensions for type IIA flux vacua”, Phys. Rev. D 106 (2022) no.6, 066017 [arXiv:2204.00014 [hep-th]]

  31. [37]

    Holographic perspectives on models of moduli stabilization in M-theory,

    S. Ning, “Holographic perspectives on models of moduli stabilization in M-theory,” JHEP 09, 042 (2022) [arXiv:2206.13332 [hep-th]]

  32. [38]

    Aspects of AdS flux vacua with integer conform al dimensions,

    F. Apers, “Aspects of AdS flux vacua with integer conform al dimensions,” JHEP 05, 040 (2023) [arXiv:2211.04187 [hep-th]]

  33. [39]

    Mass spectrum of type IIB flux compactifi cations — comments on AdS vacua and conformal dimensions

    E. Plauschinn, “Mass spectrum of type IIB flux compactifi cations — comments on AdS vacua and conformal dimensions”, JHEP 02, 257 (2023) [arXiv:2210.04528 [hep-th]]

  34. [40]

    Quantum gravity constrai nts on scale separation and de Sitter in five dimensions,

    N. Cribiori and C. Montella, “Quantum gravity constrai nts on scale separation and de Sitter in five dimensions,” JHEP 05, 178 (2023) [arXiv:2303.04162 [hep-th]]

  35. [41]

    On scale-separ ated supersymmetric AdS 2 flux vacua,

    N. Cribiori, F. Farakos and N. Liatsos, “On scale-separ ated supersymmetric AdS 2 flux vacua,” [arXiv:2411.04932 [hep-th]]. 18

  36. [42]

    AdS 2 type-IIA solutions and scale separation,

    D. Lüst and D. Tsimpis, “AdS 2 type-IIA solutions and scale separation,” JHEP 07, 060 (2020) [arXiv:2004.07582 [hep-th]]

  37. [45]

    Type II orienti fold flux vacua in 3D,

    Á. Arboleya, A. Guarino and M. Morittu, “Type II orienti fold flux vacua in 3D,” JHEP 12, 087 (2024) [arXiv:2408.01403 [hep-th]]

  38. [46]

    Supersymmetric scale-separated Ad S3 vacua of type IIB,

    V. Van Hemelryck, “Supersymmetric scale-separated Ad S3 vacua of type IIB,” [arXiv:2502.04791 [hep-th]]

  39. [47]

    Three-dimension al flux vacua from IIB on co-calibrated G2 orientifolds

    M. Emelin, F. Farakos and G. Tringas, “Three-dimension al flux vacua from IIB on co-calibrated G2 orientifolds”, Eur. Phys. J. C 81, no.5, 456 (2021) [arXiv:2103.03282 [hep-th]]

  40. [48]

    Scale-Separated AdS3 Vacua from G2- Orientifolds Using Bispinors

    V. Van Hemelryck, “Scale-Separated AdS3 Vacua from G2- Orientifolds Using Bispinors”, Fortsch. Phys. 70 (2022) no.12, 2200128 [arXiv:2207.14311 [hep-th]]

  41. [49]

    On/off scale sepa ration,

    F. Farakos, M. Morittu and G. Tringas, “On/off scale sepa ration,” JHEP 10, 067 (2023) [arXiv:2304.14372 [hep-th]]

  42. [50]

    Scale-separated AdS 3×S1 vacua from IIA orientifolds,

    F. Farakos and M. Morittu, “Scale-separated AdS 3×S1 vacua from IIA orientifolds,” Eur. Phys. J. C 84, no.1, 98 (2024) [arXiv:2311.08991 [hep-th]]

  43. [51]

    Constructing compact manifolds with except ional holonomy,

    D. Joyce, “Constructing compact manifolds with except ional holonomy,” Clay Math. Proc. 3 (2004), 177-191 19

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