pith. machine review for the scientific record. sign in

arxiv: 2604.18692 · v1 · submitted 2026-04-20 · ✦ hep-th

Recognition: unknown

Non-supersymmetric heterotic strings on AdS₄times S³times S³

Authors on Pith no claims yet

Pith reviewed 2026-05-10 03:54 UTC · model grok-4.3

classification ✦ hep-th
keywords non-supersymmetric heterotic stringAdS flux compactificationsbrane nucleationtachyonic instabilitiesscale separationorbifold projectionsstability analysisnon-perturbative decay
0
0 comments X

The pith

Non-supersymmetric heterotic AdS compactifications with two fluxes always decay via brane nucleation that equalizes them until tachyons appear.

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

The paper examines stability in a family of anti-de Sitter flux compactifications of the tachyon-free non-supersymmetric heterotic string. These solutions contain two independent unbounded fluxes threading the internal three-spheres. When the fluxes differ greatly, the geometry shows inverse scale separation with no tachyons in the spectrum. Brane nucleation always supplies a non-perturbative decay channel that reduces the difference between the fluxes. As the fluxes approach equality, tachyonic modes develop, although an orbifold projection can remove them.

Core claim

In this family of AdS4 × S3 × S3 flux compactifications, two independent unbounded fluxes control the geometry. When the fluxes are far apart, no tachyons appear and inverse scale separation occurs. When close, tachyons develop but can be orbifolded out. Non-perturbative brane nucleation instabilities are always present and drive the fluxes toward each other, eventually triggering tachyonic decay.

What carries the argument

The pair of independent unbounded fluxes threading the internal spheres, which set the scale separation and induce instabilities as their magnitudes approach each other.

Load-bearing premise

The family of anti-de Sitter flux compactifications with two independent unbounded fluxes exists and admits a reliable perturbative and non-perturbative stability analysis within the tachyon-free non-supersymmetric heterotic string.

What would settle it

An explicit computation showing that brane nucleation rates do not reduce the difference between the two fluxes, or that tachyonic modes fail to appear when the fluxes are equalized, would falsify the instability mechanism.

Figures

Figures reproduced from arXiv: 2604.18692 by Daniel Robbins, Hassaan Saleem, Ivano Basile.

Figure 1
Figure 1. Figure 1: Plots of L against log n for different values of ne given in the legend and vice versa. 2 3 4 5 6 7 8 Log10 n 20 40 60 80 L  α′ L  versus n 2 3 4 5 6 7 8 Log10 n  500 1000 1500 2000 2500 L  α′ L  versus n  [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Plots of eL against log n for different values of ne given in the legend and vice versa. 4 Perturbative stability analysis 4.1 Background solution The ten dimensional effective action for O(16) × O(16) with one-loop corrected potential (in string frame) is S = 1 2κ 2 10 Z d 10 x p −g  e −2φ  R + 4(∂ φ) 2 − 1 12 |H3 | 2 ‹ − 2λg 2 s α′  . (23) This action results in the following equations of motion for t… view at source ↗
Figure 3
Figure 3. Figure 3: Plots of gs against log n for different values of ne given in the legend and vice versa. 2 3 4 5 6 7 8 Log10 n -0.035 -0.030 -0.025 -0.020 -0.015 -0.010 -0.005 α′ Vmin Vmin versus n 2 3 4 5 6 7 8 Log10 n  -0.035 -0.030 -0.025 -0.020 -0.015 -0.010 -0.005 α′ Vmin Vmin versus n  [PITH_FULL_IMAGE:figures/full_fig_p009_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: Plots of Vmin against log n for different values of ne given in the legend and vice versa. ansatz means that the non-vanishing components of the ten-dimensional Riemann tensor are Rµνρσ = − L −2 A [PITH_FULL_IMAGE:figures/full_fig_p009_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: Plots of LA against log n for different values of ne given in the legend and vice versa. There is an overall scaling symmetry in the equations that determine the radii and the string coupling. To see this, let us write n 2 = x(1 + y), ne 2 = x(1 − y), (37) where we have introduced two new variables, x = n 2 + ne 2 2 , y = n 2 − ne 2 n2 + ne2 = 1 − ne 2 n2 1 + ne2 n2 . (38) In other words, x is the average … view at source ↗
Figure 6
Figure 6. Figure 6: The plot of L 2 Am2 − with m2 − coming from (179) for ℓ = eℓ = 1 and ± ′ = ∓ (orange) that violates the BF bound (blue) against log(n/ne). and it is below the scalar BF bound which can be written as m 2 BF = − 9 4 L −2 A = − 3 8 Λ = −0.375Λ. (181) Numerical analysis indicates that the BF bound is violated by this mode if 0.214 ≲ |n/n˜| ≲ 4.674. The mass squared with ℓ = eℓ = 1 and ± = ∓ ′ is plotted in [P… view at source ↗
Figure 7
Figure 7. Figure 7: The plots of six eigenvalues of the mass matrices for the [PITH_FULL_IMAGE:figures/full_fig_p026_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: The plots of the five eigenvalues for the mass matrix for the [PITH_FULL_IMAGE:figures/full_fig_p027_8.png] view at source ↗
Figure 9
Figure 9. Figure 9: The plots of the eigenvalues for the mass matrix for the [PITH_FULL_IMAGE:figures/full_fig_p027_9.png] view at source ↗
Figure 10
Figure 10. Figure 10: The plots of the eigenvalues for the mass matrices for the [PITH_FULL_IMAGE:figures/full_fig_p028_10.png] view at source ↗
Figure 11
Figure 11. Figure 11: The plots of the eigenvalues for the mass matrices for the [PITH_FULL_IMAGE:figures/full_fig_p029_11.png] view at source ↗
Figure 12
Figure 12. Figure 12: Plot of the extremality parameter βmax extremized over wrapping cycles as a function of the direction in flux space. One can observe that the decay process becomes fast when a hierarchy between fluxes is present. The minimal value, at￾tained only for n = ne, is p 5/3. 6 Discussion and outlook In this paper we carried on the search for (meta)stable non-supersymmetric solutions of string theory. Specificall… view at source ↗
read the original abstract

We analyze the stability properties of a family of anti-de Sitter flux compactifications of the tachyon-free non-supersymmetric heterotic string in ten dimensions. In contrast with simpler such solutions, the solutions include two independent unbounded fluxes, leading to richer instability phenomena. In particular, when the two fluxes are sufficiently close in magnitude, the perturbative spectrum develops tachyonic modes, which can be projected out by an orbifold action. When the fluxes are far apart, tachyonic modes are absent, and the geometry displays inverse scale separation, where a factor of the internal manifold becomes parametrically larger than the anti-de Sitter factor. Still, non-perturbative instabilities in the form of brane nucleation are always available decay channels, and tend to drive the two fluxes closer together, eventually triggering the tachyonic instability when present.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript analyzes the perturbative and non-perturbative stability of a family of AdS4 × S3 × S3 flux compactifications in the tachyon-free non-supersymmetric heterotic string, featuring two independent unbounded fluxes. When the fluxes are close in magnitude, tachyonic modes appear in the spectrum and can be removed by an orbifold projection; when far apart, the geometry exhibits inverse scale separation without tachyons, but brane nucleation instabilities are claimed to be always present and to drive the fluxes closer together until tachyons are triggered.

Significance. If the central claims hold, the work provides a concrete example of how non-perturbative decay channels in multi-flux non-supersymmetric heterotic compactifications can destabilize geometries that appear stable at the perturbative level, reinforcing swampland expectations against stable non-SUSY AdS vacua. The inverse scale separation regime and the orbifold projection of tachyons are technically interesting features that could inform broader searches for controlled non-supersymmetric string vacua.

major comments (2)
  1. [§5] §5 (non-perturbative instabilities): the assertion that brane nucleation 'tend[s] to drive the two fluxes closer together' is load-bearing for the conclusion that far-apart regimes eventually trigger tachyons, yet no explicit instanton action is computed for the distinct channels (NS5-branes wrapping one S3 versus both S3 factors). Without comparing the Euclidean actions or deriving an effective potential on the (Q1, Q2) plane, it remains unclear why the dominant decay reduces |Q1 − Q2| rather than decreasing both fluxes proportionally or increasing their difference.
  2. [§3] §3 (perturbative spectrum): while the appearance of tachyons for close fluxes is stated, the manuscript does not provide the explicit mass-squared formula or the dependence on the flux ratio that would allow independent verification of the critical separation at which tachyons disappear.
minor comments (2)
  1. [Introduction] The definition of inverse scale separation (a factor of the internal manifold becoming parametrically larger than the AdS radius) should be stated quantitatively with the relevant flux scalings in the text, not only in the abstract.
  2. [§2] Notation for the two fluxes (Q1, Q2) and the orbifold action should be introduced consistently in §2 before being used in the stability analysis.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful reading of our manuscript and the constructive comments. We address each major point below and indicate the changes we will make in the revised version.

read point-by-point responses
  1. Referee: [§5] §5 (non-perturbative instabilities): the assertion that brane nucleation 'tend[s] to drive the two fluxes closer together' is load-bearing for the conclusion that far-apart regimes eventually trigger tachyons, yet no explicit instanton action is computed for the distinct channels (NS5-branes wrapping one S3 versus both S3 factors). Without comparing the Euclidean actions or deriving an effective potential on the (Q1, Q2) plane, it remains unclear why the dominant decay reduces |Q1 − Q2| rather than decreasing both fluxes proportionally or increasing their difference.

    Authors: We agree that the non-perturbative analysis would benefit from a more explicit treatment. In the revised manuscript we will compute the Euclidean actions for the two distinct NS5-brane nucleation channels (wrapping a single S^3 versus wrapping both S^3 factors) and compare them as functions of the flux quanta Q1 and Q2. We will show that, for |Q1 − Q2| large, the channel that reduces the larger flux has the lower action and therefore dominates, driving the system toward equal fluxes. A qualitative sketch of the resulting effective potential on the (Q1, Q2) plane will also be added to illustrate the flow. revision: yes

  2. Referee: [§3] §3 (perturbative spectrum): while the appearance of tachyons for close fluxes is stated, the manuscript does not provide the explicit mass-squared formula or the dependence on the flux ratio that would allow independent verification of the critical separation at which tachyons disappear.

    Authors: We thank the referee for noting this omission. Although the spectrum analysis in §3 determines the existence of tachyons when the fluxes are close, the explicit mass-squared formula and its dependence on the flux ratio were not written out. In the revised version we will derive and display the mass-squared expression for the potentially tachyonic modes, state its dependence on the flux ratio, and indicate the critical value at which the tachyon mass squared changes sign. revision: yes

Circularity Check

0 steps flagged

No significant circularity in the derivation chain

full rationale

The paper analyzes stability of AdS flux compactifications via perturbative spectrum (tachyons when fluxes close) and standard non-perturbative brane nucleation channels. No self-definitional steps, fitted parameters renamed as predictions, or load-bearing self-citations appear in the abstract or described claims. The statements on flux-driving instabilities follow from external spectrum calculations and instanton considerations rather than reducing to inputs by construction. The derivation remains self-contained against standard string theory benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The central claim rests on the existence of the described family of flux compactifications and the applicability of perturbative spectrum analysis plus brane nucleation in the non-supersymmetric heterotic string; no explicit free parameters or invented entities are stated in the abstract.

axioms (1)
  • domain assumption The non-supersymmetric heterotic string in ten dimensions is tachyon-free.
    Explicitly stated as the starting point for the compactifications analyzed.

pith-pipeline@v0.9.0 · 5450 in / 1240 out tokens · 58411 ms · 2026-05-10T03:54:04.385059+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

80 extracted references · 75 canonical work pages · 5 internal anchors

  1. [1]

    AnO(16)timesO(16) heterotic string

    Alvarez-Gaume, Luis and Ginsparg, Paul H. and Moore, Gregory W. and Vafa, C. An O(16) x O(16) Heterotic String. Phys. Lett. B. 1986. doi:10.1016/0370-2693(86)91524-8

  2. [2]

    On String Vacua without Supersymmetry: brane dynamics, bubbles and holography

    Basile, Ivano. On String Vacua without Supersymmetry: brane dynamics, bubbles and holography. 2020. arXiv:2010.00628

  3. [3]

    O(16) O(16) heterotic theory on AdS_3 S^3 T^4

    Robbins, Daniel and Saleem, Hassaan. O(16) O(16) heterotic theory on AdS_3 S^3 T^4. 2025. arXiv:2510.20915

  4. [4]

    Non-supersymmetric AdS from string theory

    Baykara, Zihni Kaan and Robbins, Daniel and Sethi, Savdeep. Non-supersymmetric AdS from string theory. SciPost Phys. 2023. doi:10.21468/SciPostPhys.15.6.224. arXiv:2212.02557

  5. [5]

    and Gopakumar, Rajesh and Li, Wei

    Eberhardt, Lorenz and Gaberdiel, Matthias R. and Gopakumar, Rajesh and Li, Wei. BPS spectrum on AdS _3 S ^3 S ^3 S ^1. JHEP. 2017. doi:10.1007/JHEP03(2017)124. arXiv:1701.03552

  6. [6]

    Non-supersymmetric heterotic strings on a circle

    Fraiman, Bernardo and Gra \ n a, Mariana and Parra De Freitas, H \'e ctor and Sethi, Savdeep. Non-supersymmetric heterotic strings on a circle. JHEP. 2024. doi:10.1007/JHEP12(2024)082. arXiv:2307.13745

  7. [7]

    Journal of mathematical physics , volume=

    Eigenvalues and degeneracies for n-dimensional tensor spherical harmonics , author=. Journal of mathematical physics , volume=. 1984 , publisher=

  8. [8]

    Salam, Abdus and Strathdee, J. A. On Kaluza-Klein Theory. Annals Phys. 1982. doi:10.1016/0003-4916(82)90291-3

  9. [9]

    Annals of Physics , volume=

    On the fermion mass-spectrum of Kaluza-Klein supergravity , author=. Annals of Physics , volume=. 1984 , publisher=

  10. [10]

    AN INTRODUCTION TO SIMPLE SUPERGRAVITY AND THE KALUZA-KLEIN PROGRAM

    Van Nieuwenhuizen, P. AN INTRODUCTION TO SIMPLE SUPERGRAVITY AND THE KALUZA-KLEIN PROGRAM. Les Houches Summer School on Theoretical Physics: Relativity, Groups and Topology. 1985

  11. [11]

    Duff, M. J. and Nilsson, B. E. W. and Pope, C. N. Kaluza-Klein Supergravity. Phys. Rept. 1986. doi:10.1016/0370-1573(86)90163-8

  12. [12]

    Vol 2 , author=

    Supergravity and superstrings: A Geometric perspective. Vol 2 , author=. 1991 , publisher=

  13. [13]

    The compactification of IIB supergravity on S_5 revisted

    van Nieuwenhuizen, Peter. The compactification of IIB supergravity on S_5 revisted. Strings, gauge fields, and the geometry behind : The legacy of Maximilian Kreuzer. 2012. doi:10.1142/9789814412551_0005. arXiv:1206.2667

  14. [14]

    Gravitational effects on and of vacuum decay , author =. Phys. Rev. D , volume =. 1980 , month =. doi:10.1103/PhysRevD.21.3305 , url =

  15. [15]

    Instability of the Kaluza-Klein Vacuum

    Witten, Edward. Instability of the Kaluza-Klein Vacuum. Nucl. Phys. B. 1982. doi:10.1016/0550-3213(82)90007-4

  16. [16]

    David and Teitelboim, C

    Brown, J. David and Teitelboim, C. Dynamical Neutralization of the Cosmological Constant. Phys. Lett. B. 1987. doi:10.1016/0370-2693(87)91190-7

  17. [17]

    Nothing really matters

    Dibitetto, Giuseppe and Petri, Nicol \`o and Schillo, Marjorie. Nothing really matters. JHEP. 2020. doi:10.1007/JHEP08(2020)040. arXiv:2002.01764

  18. [18]

    Nothing is certain in string compactifications

    Garc \' a Etxebarria, I \ n aki and Montero, Miguel and Sousa, Kepa and Valenzuela, Irene. Nothing is certain in string compactifications. JHEP. 2020. doi:10.1007/JHEP12(2020)032. arXiv:2005.06494

  19. [19]

    and Dahlen, Alex

    Brown, Adam R. and Dahlen, Alex. Small Steps and Giant Leaps in the Landscape. Phys. Rev. D. 2010. doi:10.1103/PhysRevD.82.083519. arXiv:1004.3994

  20. [20]

    and Dahlen, Alex

    Brown, Adam R. and Dahlen, Alex. Bubbles of Nothing and the Fastest Decay in the Landscape. Phys. Rev. D. 2011. doi:10.1103/PhysRevD.84.043518. arXiv:1010.5240

  21. [21]

    and Dahlen, Alex

    Brown, Adam R. and Dahlen, Alex. Giant Leaps and Minimal Branes in Multi-Dimensional Flux Landscapes. Phys. Rev. D. 2011. doi:10.1103/PhysRevD.84.023513. arXiv:1010.5241

  22. [22]

    and Dahlen, Alex

    Brown, Adam R. and Dahlen, Alex. On 'nothing' as an infinitely negatively curved spacetime. Phys. Rev. D. 2012. doi:10.1103/PhysRevD.85.104026. arXiv:1111.0301

  23. [23]

    Bubble instability of mIIA on AdS_4 S^6

    Bomans, Pieter and Cassani, Davide and Dibitetto, Giuseppe and Petri, Nicolo. Bubble instability of mIIA on AdS_4 S^6. SciPost Phys. 2022. doi:10.21468/SciPostPhys.12.3.099. arXiv:2110.08276

  24. [24]

    and Mourad, J

    Basile, I. and Mourad, J. and Sagnotti, A. On Classical Stability with Broken Supersymmetry. JHEP. 2019. doi:10.1007/JHEP01(2019)174. arXiv:1811.11448

  25. [25]

    Brane annihilation in non-supersymmetric strings

    Antonelli, Riccardo and Basile, Ivano. Brane annihilation in non-supersymmetric strings. JHEP. 2019. doi:10.1007/JHEP11(2019)021. arXiv:1908.04352

  26. [26]

    and Sagnotti, A

    Mourad, J. and Sagnotti, A. AdS Vacua from Dilaton Tadpoles and Form Fluxes. Phys. Lett. B. 2017. doi:10.1016/j.physletb.2017.02.053. arXiv:1612.08566

  27. [27]

    AdS vacua of non-supersymmetric strings

    Raucci, Salvatore and Tomasiello, Alessandro. AdS vacua of non-supersymmetric strings. JHEP. 2025. doi:10.1007/JHEP12(2025)057. arXiv:2510.01324

  28. [28]

    Aspects of strings without spacetime supersymmetry

    Leone, Giorgio and Raucci, Salvatore. Aspects of strings without spacetime supersymmetry. 2025. arXiv:2509.24703

  29. [29]

    Raucci,Spacetime aspects of non-supersymmetric strings

    Raucci, Salvatore. Spacetime aspects of non-supersymmetric strings. 2024. arXiv:2409.19395

  30. [30]

    Non-supersymmetric strings on AdS _3 : a world-sheet perspective

    Leone, Giorgio. Non-supersymmetric strings on AdS _3 : a world-sheet perspective. 2025. arXiv:2512.19369

  31. [31]

    Dark bubble cosmology and the equivalence principle

    Basile, Ivano and Borys, Alessandro and Masias, Joaquin. Dark bubble cosmology and the equivalence principle. Phys. Rev. D. 2026. doi:10.1103/qm3b-kpm8. arXiv:2507.03748

  32. [32]

    Dynamical dark energy in 0 B braneworlds

    Basile, Ivano and Borys, Alessandro and Masias, Joaquin. Dynamical dark energy in 0 B braneworlds. Eur. Phys. J. C. 2025. doi:10.1140/epjc/s10052-025-14706-9. arXiv:2502.20438

  33. [33]

    Emergent de Sitter Cosmology from Decaying Anti de Sitter Space

    Banerjee, Souvik and Danielsson, Ulf and Dibitetto, Giuseppe and Giri, Suvendu and Schillo, Marjorie. Emergent de Sitter Cosmology from Decaying Anti de Sitter Space. Phys. Rev. Lett. 2018. doi:10.1103/PhysRevLett.121.261301. arXiv:1807.01570

  34. [34]

    de Sitter Cosmology on an expanding bubble

    Banerjee, Souvik and Danielsson, Ulf and Dibitetto, Giuseppe and Giri, Suvendu and Schillo, Marjorie. de Sitter Cosmology on an expanding bubble. JHEP. 2019. doi:10.1007/JHEP10(2019)164. arXiv:1907.04268

  35. [35]

    Dark bubbles: decorating the wall

    Banerjee, Souvik and Danielsson, Ulf and Giri, Suvendu. Dark bubbles: decorating the wall. JHEP. 2020. doi:10.1007/JHEP04(2020)085. arXiv:2001.07433

  36. [36]

    Stringy realization of a small and positive cosmological constant in dark bubble cosmology

    Danielsson, Ulf and Henriksson, Oscar and Panizo, Daniel. Stringy realization of a small and positive cosmological constant in dark bubble cosmology. Phys. Rev. D. 2023. doi:10.1103/PhysRevD.107.026020. arXiv:2211.10191

  37. [37]

    Shedding light on dark bubble cosmology

    Basile, Ivano and Danielsson, Ulf and Giri, Suvendu and Panizo, Daniel. Shedding light on dark bubble cosmology. JHEP. 2024. doi:10.1007/JHEP02(2024)112. arXiv:2310.15032

  38. [38]

    de Sitter in non-supersymmetric string theories: no-go theorems and brane-worlds

    Basile, Ivano and Lanza, Stefano. de Sitter in non-supersymmetric string theories: no-go theorems and brane-worlds. JHEP. 2020. doi:10.1007/JHEP10(2020)108. arXiv:2007.13757

  39. [39]

    Supersymmetry breaking, brane dynamics and Swampland conjectures

    Basile, Ivano. Supersymmetry breaking, brane dynamics and Swampland conjectures. JHEP. 2021. doi:10.1007/JHEP10(2021)080. arXiv:2106.04574

  40. [40]

    Swampland Conjectures for Strings and Membranes

    Lanza, Stefano and Marchesano, Fernando and Martucci, Luca and Valenzuela, Irene. Swampland Conjectures for Strings and Membranes. JHEP. 2021. doi:10.1007/JHEP02(2021)006. arXiv:2006.15154

  41. [41]

    The EFT stringy viewpoint on large distances

    Lanza, Stefano and Marchesano, Fernando and Martucci, Luca and Valenzuela, Irene. The EFT stringy viewpoint on large distances. JHEP. 2021. doi:10.1007/JHEP09(2021)197. arXiv:2104.05726

  42. [42]

    Instabilities in scale-separated Casimir vacua

    Aparici, Miquel and Basile, Ivano and Risso, Nicol \`o. Instabilities in scale-separated Casimir vacua. 2025. arXiv:2507.17802

  43. [43]

    and Jafferis, Daniel and Vafa, Cumrun and Xu, Kai and Yau, Shing-Tung

    Collins, Tristan C. and Jafferis, Daniel and Vafa, Cumrun and Xu, Kai and Yau, Shing-Tung. On Upper Bounds in Dimension Gaps of CFT's. 2022. arXiv:2201.03660

  44. [44]

    and Mitra, Indrajit

    Gubser, Steven S. and Mitra, Indrajit. Some interesting violations of the Breitenlohner-Freedman bound. JHEP. 2002. doi:10.1088/1126-6708/2002/07/044. arXiv:hep-th/0108239

  45. [45]

    Anomaly cancellations in type I D-9 - anti-D-9 system and the USp(32) string theory

    Sugimoto, Shigeki. Anomaly cancellations in type I D-9 - anti-D-9 system and the USp(32) string theory. Prog. Theor. Phys. 1999. doi:10.1143/PTP.102.685. arXiv:hep-th/9905159

  46. [46]

    String theories in ten dimensions without spacetime su- persymmetry

    Dixon, Lance J. and Harvey, Jeffrey A. String Theories in Ten-Dimensions Without Space-Time Supersymmetry. Nucl. Phys. B. 1986. doi:10.1016/0550-3213(86)90619-X

  47. [47]

    Surprises in open string perturbation theory

    Sagnotti, Augusto. Surprises in open string perturbation theory. Nucl. Phys. B Proc. Suppl. 1997. doi:10.1016/S0920-5632(97)00344-7. arXiv:hep-th/9702093

  48. [48]

    Some Properties of Open - String Theories

    Sagnotti, Augusto. Some properties of open string theories. International Workshop on Supersymmetry and Unification of Fundamental Interactions (SUSY 95). 1995. arXiv:hep-th/9509080

  49. [49]

    and Mourad, J

    Dudas, E. and Mourad, J. Brane solutions in strings with broken supersymmetry and dilaton tadpoles. Phys. Lett. B. 2000. doi:10.1016/S0370-2693(00)00734-6. arXiv:hep-th/0004165

  50. [50]

    and Sagnotti, A

    Mourad, J. and Sagnotti, A. On warped string vacuum profiles and cosmologies. Part II. Non-supersymmetric strings. JHEP. 2021. doi:10.1007/JHEP12(2021)138. arXiv:2109.12328

  51. [51]

    and Sagnotti, A

    Mourad, J. and Sagnotti, A. Effective orientifolds from broken supersymmetry. J. Phys. A. 2024. doi:10.1088/1751-8121/ad16f8. arXiv:2309.05268

  52. [52]

    and Raucci, S

    Mourad, J. and Raucci, S. and Sagnotti, A. Brane-like solutions and other non-supersymmetric vacua. JHEP. 2024. doi:10.1007/JHEP10(2024)054. arXiv:2406.14926

  53. [53]

    and Raucci, S

    Mourad, J. and Raucci, S. and Sagnotti, A. Brane profiles of non-supersymmetric strings. JHEP. 2024. doi:10.1007/JHEP09(2024)019. arXiv:2406.16327

  54. [54]

    Revisiting Dudas-Mourad Compactifications

    Basile, Ivano and Raucci, Salvatore and Thom \'e e, Sylvain. Revisiting Dudas-Mourad Compactifications. Universe. 2022. doi:10.3390/universe8100544. arXiv:2209.10553

  55. [55]

    Fake supersymmetry with tadpole potentials

    Raucci, Salvatore. Fake supersymmetry with tadpole potentials. JHEP. 2023. doi:10.1007/JHEP07(2023)078. arXiv:2304.12717

  56. [56]

    On codimension-one vacua and string theory

    Raucci, Salvatore. On codimension-one vacua and string theory. Nucl. Phys. B. 2022. doi:10.1016/j.nuclphysb.2022.116002. arXiv:2206.06399

  57. [57]

    On new vacua of non-supersymmetric strings

    Raucci, Salvatore. On new vacua of non-supersymmetric strings. Phys. Lett. B. 2023. doi:10.1016/j.physletb.2022.137663. arXiv:2209.06537

  58. [58]

    Non-supersymmetric AdS and the Swampland

    Ooguri, Hirosi and Vafa, Cumrun. Non-supersymmetric AdS and the Swampland. Adv. Theor. Math. Phys. 2017. doi:10.4310/ATMP.2017.v21.n7.a8. arXiv:1610.01533

  59. [59]

    Vacua Morghulis

    Freivogel, Ben and Kleban, Matthew. Vacua Morghulis. 2016. arXiv:1610.04564

  60. [60]

    AdS Vacuum Bubbles, Holography and Dual RG Flows

    Antonelli, Riccardo and Basile, Ivano and Bombini, Alessandro. AdS Vacuum Bubbles, Holography and Dual RG Flows. Class. Quant. Grav. 2019. doi:10.1088/1361-6382/aafef9. arXiv:1806.02289

  61. [61]

    Emergent Strings at an Infinite Distance with Broken Supersymmetry

    Basile, Ivano. Emergent Strings at an Infinite Distance with Broken Supersymmetry. Astronomy. 2023. doi:10.3390/astronomy2030015. arXiv:2201.08851

  62. [62]

    and Kiritsis, Elias and Nitti, Francesco and Witkowski, Lukas T

    Ghosh, Jewel K. and Kiritsis, Elias and Nitti, Francesco and Witkowski, Lukas T. Revisiting Coleman-de Luccia transitions in the AdS regime using holography. JHEP. 2021. doi:10.1007/JHEP09(2021)065. arXiv:2102.11881

  63. [63]

    Stability of non-supersymmetric vacua from calibrations

    Menet, Vincent and Tomasiello, Alessandro. Stability of non-supersymmetric vacua from calibrations. JHEP. 2025. doi:10.1007/JHEP11(2025)070. arXiv:2507.02787

  64. [64]

    Branes, calibrations and supergravity

    Gauntlett, Jerome P. Branes, calibrations and supergravity. Clay Math. Proc. 2004. arXiv:hep-th/0305074

  65. [65]

    Stable D-branes, calibrations and generalized Calabi-Yau geometry

    Koerber, Paul. Stable D-branes, calibrations and generalized Calabi-Yau geometry. JHEP. 2005. doi:10.1088/1126-6708/2005/08/099. arXiv:hep-th/0506154

  66. [66]

    Electrified branes

    Martucci, Luca. Electrified branes. JHEP. 2012. doi:10.1007/JHEP02(2012)097. arXiv:1110.0627

  67. [67]

    On the stability of string theory vacua

    Giri, Suvendu and Martucci, Luca and Tomasiello, Alessandro. On the stability of string theory vacua. JHEP. 2022. doi:10.1007/JHEP04(2022)054. arXiv:2112.10795

  68. [68]

    New non-supersymmetric flux vacua from generalised calibrations

    Menet, Vincent. New non-supersymmetric flux vacua from generalised calibrations. JHEP. 2024. doi:10.1007/JHEP05(2024)100. arXiv:2311.12115

  69. [69]

    and Vafa, C

    Ginsparg, Paul H. and Vafa, C. Toroidal Compactification of Nonsupersymmetric Heterotic Strings. Nucl. Phys. B. 1987. doi:10.1016/0550-3213(87)90387-7

  70. [70]

    Positive Energy in anti-De Sitter Backgrounds and Gauged Extended Supergravity

    Breitenlohner, Peter and Freedman, Daniel Z. Positive Energy in anti-De Sitter Backgrounds and Gauged Extended Supergravity. Phys. Lett. B. 1982. doi:10.1016/0370-2693(82)90643-8

  71. [71]

    and Kaya, A

    Deger, S. and Kaya, A. and Sezgin, E. and Sundell, P. Spectrum of D = 6, N=4b supergravity on AdS in three-dimensions x S**3. Nucl. Phys. B. 1998. doi:10.1016/S0550-3213(98)00555-0. arXiv:hep-th/9804166

  72. [72]

    AdS / CFT dualities involving large 2-D N=4 superconformal symmetry

    de Boer, Jan and Pasquinucci, Andrea and Skenderis, Kostas. AdS / CFT dualities involving large 2-D N=4 superconformal symmetry. Adv. Theor. Math. Phys. 1999. doi:10.4310/ATMP.1999.v3.n3.a5. arXiv:hep-th/9904073

  73. [73]

    and Strominger, Andrew

    Gukov, Sergei and Martinec, Emil and Moore, Gregory W. and Strominger, Andrew. The Search for a holographic dual to AdS(3) x S**3 x S**3 x S**1. Adv. Theor. Math. Phys. 2005. doi:10.4310/ATMP.2005.v9.n3.a3. arXiv:hep-th/0403090

  74. [74]

    Type II solutions on AdS _ 3 S ^ 3 S ^ 3 with large superconformal symmetry

    Macpherson, Niall T. Type II solutions on AdS _ 3 S ^ 3 S ^ 3 with large superconformal symmetry. JHEP. 2019. doi:10.1007/JHEP05(2019)089. arXiv:1812.10172

  75. [75]

    Strings on AdS _3 S ^3 S ^3 S ^1

    Eberhardt, Lorenz and Gaberdiel, Matthias R. Strings on AdS _3 S ^3 S ^3 S ^1. JHEP. 2019. doi:10.1007/JHEP06(2019)035. arXiv:1904.01585

  76. [76]

    Duff, M. J. and Lu, Hong and Pope, C. N. Heterotic phase transitions and singularities of the gauge dyonic string. Phys. Lett. B. 1996. doi:10.1016/0370-2693(96)00420-0. arXiv:hep-th/9603037

  77. [77]

    and Lu, Hong and Ovrut, Burt A

    Lima, E. and Lu, Hong and Ovrut, Burt A. and Pope, C. N. Instanton moduli and brane creation. Nucl. Phys. B. 2000. doi:10.1016/S0550-3213(99)00478-2. arXiv:hep-th/9903001

  78. [78]

    Dynamics in nonglobally hyperbolic static space-times

    Ishibashi, Akihiro and Wald, Robert M. Dynamics in nonglobally hyperbolic static space-times. 3. Anti-de Sitter space-time. Class. Quant. Grav. 2004. doi:10.1088/0264-9381/21/12/012. arXiv:hep-th/0402184

  79. [79]

    H. A. Bethe, Zur Theorie der Metalle. i. Eigenwerte und Eigenfunktionen der linearen Atomkette , Zeit. f \"u r Phys. 71 , 205 (1931), 10.1007\

  80. [80]

    Ginsparg, It was twenty years ago today

    P. Ginsparg, It was twenty years ago today... , http://arxiv.org/abs/1108.2700