Pith. sign in

REVIEW 6 minor 91 references

The leading Kaluza–Klein tower correction that sets higher-derivative gravity scales is regulator-dependent matching data, so the two usual species-scale definitions agree only parametrically, not coefficient by coefficient.

Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →

T0 review · grok-4.5

2026-07-11 16:34 UTC pith:FPYEHMJF

load-bearing objection Clean technical clarification: KK-tower one-loop data split into scheme-dependent N-enhanced local thresholds and regulator-stable log N coefficients, so coefficient-level species-scale identification is not regulator-independent.

arxiv 2607.04602 v1 pith:FPYEHMJF submitted 2026-07-06 hep-th

Kaluza-Klein tower thresholds and scheme dependence of the species scale

classification hep-th
keywords species scaleKaluza-Klein towersEFT matchingscheme dependencehigher-derivative gravityproper-time cutoffone-loop effective action
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

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

Two common ways of defining the species scale in quantum gravity—one from the breakdown of the one-loop graviton propagator, the other from the suppression scale of higher-derivative operators—are routinely treated as interchangeable. This paper shows that, once an infinite Kaluza–Klein tower is integrated out with a controlled cutoff, they are not. The tower-enhanced local four-derivative terms depend on the choice of proper-time cutoff profile and must be absorbed into EFT matching coefficients; only a subleading logarithmic piece is universal inside the class of cutoffs studied. Explicit scalar and fermion calculations separate these pieces and recover the usual parametric species scaling only under the assumption that the regulator factor is order one and that ultraviolet counterterms do not cancel the tower enhancement. A sympathetic reader cares because many swampland and moduli-space arguments treat the two definitions as identical at the coefficient level; the calculation shows that only the parametric relation and the stable logarithm are robust.

Core claim

For a large number of species the leading tower-enhanced local correction is regulator dependent and should be interpreted as EFT matching data, while the subleading logarithmic contribution is universal within the class of proper-time cutoff profiles considered. Consequently the coefficient-level identification of the perturbative-breakdown and higher-derivative definitions of the species scale is not regulator independent.

What carries the argument

The regulated infinite-tower sum Na+b[fc] expressed via the Mellin transform of the proper-time cutoff profile: its leading N term carries the scheme-dependent factor efc(−1/2), while the log N coefficient is fixed by the residue Res s=0 efc = −1.

Load-bearing premise

The parametric consistency check assumes the cutoff Mellin factor is order one and that renormalized ultraviolet matching terms neither dominate nor cancel the tower contribution.

What would settle it

Compute the same four-derivative tower coefficients with two distinct proper-time cutoffs that change efc(−1/2) by an O(1) amount and check whether the difference is absorbed entirely into local counterterms while the curvature-squared log N coefficient remains identical.

Watch this falsifier — get emailed when new claim-graph text bears on it.

Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

0 major / 6 minor

Summary. The paper revisits the species scale in quantum gravity from an EFT matching perspective, comparing the perturbative-breakdown definition (from the one-loop graviton propagator) with the higher-derivative suppression-scale definition. For an S1-compactified KK tower of free scalars and Dirac fermions, it regulates the infinite tower sum with a class of proper-time cutoff profiles and shows that the large-N tower contribution separates into a leading local term proportional to N whose coefficient depends on the Mellin transform of the cutoff at s=-1/2, and a subleading log N term in the curvature-squared sector whose coefficient is fixed by Res_s=0 e_fc=-1. Explicit four-derivative one-loop matching data are computed for both spins (Eqs. (54), (62)), with a heat-kernel cross-check for scalars; after field redefinition the radion-graviton sector can be reduced to (nabla phi)^4 terms that remain matching data. The standard parametric species relation is recovered only as a self-consistency check under the stated O(1) and no-tuned-cancellation assumptions.

Significance. The work supplies a controlled, regulator-aware EFT interpretation of a relation that is often treated as coefficient-level equality in the species-scale literature. The Mellin/residue argument (Eq. (14), App. B) cleanly separates scheme-dependent local thresholds from a universal log N coefficient within a well-defined cutoff class, and the explicit scalar/fermion four-derivative results give concrete matching data for graviton, radion, and KK-photon operators. The heat-kernel versus hybrid diagrammatic cross-check for scalars, the careful treatment of the fermion multiplicative-anomaly issue, and the explicit scoping of the parametric self-consistency condition are genuine strengths. If the separation holds under broader regulator classes, it clarifies which higher-derivative data can robustly probe moduli dependence of the species scale (e.g., Distance-Conjecture rates) and why coefficient-level identification of the two characterizations is not regulator-independent.

minor comments (6)
  1. In Sec. 5 and App. D the hybrid Pauli-Villars + proper-time factorization is presented as a calculational scheme that reproduces the heat-kernel result for scalars; a short explicit statement that the same factorization for fermions is an assumption (not a theorem) about the absence of multiplicative-anomaly contamination in the local four-derivative sector would make the scoping of Eqs. (62)-(63) even clearer for readers who skip App. C.
  2. Sec. 6, after the field redefinitions (56)-(60): both scalar and fermion towers yield the same leading coefficient -1/24 for (nabla phi)^4 in the chosen basis. A one-sentence remark that this coincidence is basis- and scheme-dependent matching data (and not a spin-independent physical Wilson coefficient) would prevent over-reading of Eqs. (61) and (63).
  3. App. F (string tower): the assumptions (all excitations treated as scalars; only asymptotic degeneracy retained) are stated, but the comparison with naive cumulative counting (Eq. (F17) vs (F14)) would be easier to assess if the text briefly noted which of spin, ghosts, or modular completion is expected to affect the leading exponential versus the (log N)^{1/2} prefactor.
  4. Notation: N(phi_0) is introduced as the regulated number of KK levels and is carefully distinguished from spin/polarization degeneracy, but in a few places (e.g. around Eqs. (11) and (41)) the shorthand N appears without the argument; consistent use of N(phi_0) would reduce ambiguity.
  5. The Supplemental Material cited as [87] is essential for reproducing the photon-radion diagrams of App. E.3; for journal publication it should be deposited with a stable identifier or folded into an expanded appendix.
  6. Typos/clarity: 'in linewiththeSwampland' (p. 3) and similar run-together phrases in the introduction; 'thesameis true for k <= d/2' (end of Sec. 4.2) could be expanded by one clause for parallel structure with the k >= d/2+1 case.

Circularity Check

0 steps flagged

No significant circularity: Mellin/residue separation of scheme-dependent N terms from universal log N is derived from cutoff asymptotics; species scaling is a parametric self-consistency check under stated O(1)/no-cancellation assumptions, not a forced coefficient equality.

full rationale

The load-bearing technical chain is self-contained. Appendix B and Eq. (14)/(B15) obtain the tower sum Na+b[fc] = (1/2) ga+b efc(-1/2) N + δa+b,0 Res_s=0 efc · log N + O(N0) from the Mellin transform of admissible proper-time cutoffs with the stated boundary conditions fc(u) o1 (u o∞), fc(u) o0 (u o0); Res_s=0 efc = -1 follows directly from those asymptotics (structure theorem / singular expansion of the Mellin transform), not from fitting or from defining the species scale. Explicit four-derivative scalar (heat-kernel and diagrammatic) and fermion (diagrammatic) results, Eqs. (54) and (62), instantiate the same separation. The species-scale relation (Eqs. (42)–(43)) is introduced only as a provisional cutoff and recovered as a parametric self-consistency condition under the explicit assumptions that efc(-1/2) is O(1) and that renormalized matching neither dominates nor cancels the tower term; the paper does not claim a regulator-independent coefficient-level identification of the two characterizations—it explains why that identification fails. Citations to the broader species-scale literature supply context, not a load-bearing uniqueness theorem or ansatz that forces the result. No self-definitional loop, fitted-input-as-prediction, or self-citation chain reduces the central claim to its inputs by construction.

Axiom & Free-Parameter Ledger

1 free parameters · 5 axioms · 0 invented entities

The central claim rests on standard heat-kernel and zeta-function technology, the EFT matching philosophy that local loop pieces must be combined with counterterms, and a specific but well-documented class of proper-time cutoffs. No free parameters are fitted to data; the only free function is the cutoff profile itself, whose Mellin transform is left arbitrary within the stated boundary conditions. No new particles or forces are postulated.

free parameters (1)
  • cutoff-profile parameter alpha (illustrative)
    Appears only in the example fc(u)=1-e^{-u}+alpha u e^{-u^2} to show that e_fc(-1/2) can be varied; not fitted to any physical data and not used in the final claims.
axioms (5)
  • standard math Heat-kernel expansion of the one-loop effective action for Laplace-type operators (standard coefficients e_{2k} up to four derivatives).
    Invoked throughout Sec. 4 and Table 1; taken from Vassilevich and Avramidi.
  • domain assumption Local higher-derivative coefficients are EFT matching data that combine loop contributions with renormalized counterterms; physical amplitudes are scheme-independent only after consistent treatment.
    Stated in Sec. 1 and Sec. 3; standard EFT lore (Manohar, Burgess, Donoghue).
  • ad hoc to paper Admissible proper-time cutoffs satisfy fc(u)->1 as u->infty, fc(u)->0 as u->0, and possess a Mellin transform finite at s=-1/2 with Res_s=0 e_fc=-1.
    Defines the universality class in App. B; the residue condition follows from the boundary values but the precise function class is chosen by the author.
  • ad hoc to paper For fermions the factorized diagrammatic prescription (Pauli–Villars single-mode + proper-time tower sum) correctly captures the local matching data without multiplicative-anomaly contamination.
    Adopted in Sec. 5 and App. D because direct heat-kernel doubling is obstructed; verified only for scalars against heat kernel.
  • domain assumption The renormalized UV matching contribution is neither parametrically larger than the tower term nor tuned to cancel it.
    Required for the parametric self-consistency relation (Eq. 42) to reproduce the standard species scaling.

pith-pipeline@v1.1.0-grok45 · 42628 in / 2888 out tokens · 30948 ms · 2026-07-11T16:34:17.586024+00:00 · methodology

0 comments
read the original abstract

We revisit the species scale in quantum gravity from the viewpoint of effective field theory (EFT). Two characterizations are commonly used: one defines it as the energy at which the perturbative description of quantum gravity breaks down, as inferred from the one-loop correction to the graviton propagator; the other identifies it with the suppression scale of higher-derivative operators in the gravitational effective action. We clarify the relation between these characterizations by analyzing the cutoff-scheme dependence of the one-loop tower contribution. For a large number of species, the leading tower-enhanced local correction is regulator dependent and should be interpreted as EFT matching data, while the subleading logarithmic contribution is universal within the class of proper-time cutoff profiles considered here. As a concrete application, we compute the full four-derivative one-loop corrections from Kaluza-Klein towers. Our results separate regulator-stable logarithmic data from scheme-dependent local threshold contributions, providing a controlled EFT interpretation of the relation between perturbative-breakdown and higher-derivative definitions of the species scale and explaining why their coefficient-level identification is not regulator independent.

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

91 extracted references · 17 canonical work pages · 8 internal anchors

  1. [1]

    Dvali, Fortsch

    G. Dvali, Fortsch. Phys.,58, 528–536 (2010), arXiv:0706.2050,https://doi.org/10.1002/prop.201000009

  2. [2]

    Dvali and M

    G. Dvali and M. Redi, Phys. Rev. D, 77, 045027 (2008), arXiv:0710.4344, https://doi.org/10.1103/ PhysRevD.77.045027

  3. [3]

    Dvali and D

    G. Dvali and D. Lüst, Fortsch. Phys.,58, 505–527 (2010), arXiv:0912.3167,https://doi.org/10.1002/prop. 201000008

  4. [4]

    Dvali and C

    G. Dvali and C. Gomez (4 2010), arXiv:1004.3744

  5. [5]

    Veneziano, JHEP,06, 051 (2002), hep-th/0110129,https://doi.org/10.1088/1126-6708/2002/06/051

    G. Veneziano, JHEP,06, 051 (2002), hep-th/0110129,https://doi.org/10.1088/1126-6708/2002/06/051

  6. [6]

    Han and S

    T. Han and S. Willenbrock, Phys. Lett. B,616, 215–220 (2005), hep-ph/0404182,https://doi.org/10.1016/ j.physletb.2005.04.040

  7. [7]

    Dvali, C

    G. Dvali, C. Gomez, and D. Lust, Fortsch. Phys.,61, 768–778 (2013), arXiv:1206.2365,https://doi.org/10. 1002/prop.201300002

  8. [8]

    Aydemir, M

    U. Aydemir, M. M. Anber, and J. F. Donoghue, Phys. Rev. D,86, 014025 (2012), arXiv:1203.5153, https: //doi.org/10.1103/PhysRevD.86.014025

  9. [9]

    Graviton propagator, renormalization scale and black-hole like states

    X. Calmet, R. Casadio, A. Yu. Kamenshchik, and O. V. Teryaev, Phys. Lett. B, 774, 332–337 (2017), arXiv:1708.01485, https://doi.org/10.1016/j.physletb.2017.09.080

  10. [10]

    Castellano, A

    A. Castellano, A. Herráez, and L. E. Ibáñez, JHEP,06, 047 (2023), arXiv:2212.03908,https://doi.org/10. 1007/JHEP06(2023)047

  11. [11]

    C. Long, M. Montero, C. Vafa, and I. Valenzuela, JHEP,03, 109 (2023), arXiv:2112.11467,https://doi.org/ 10.1007/JHEP03(2023)109

  12. [12]

    Castellano, I

    A. Castellano, I. Ruiz, and I. Valenzuela, JHEP,06, 037 (2024), arXiv:2311.01536,https://doi.org/10.1007/ JHEP06(2024)037

  13. [13]

    Cribiori, D

    N. Cribiori, D. Lust, and C. Montella, JHEP,10, 059 (2023), arXiv:2305.10489, https://doi.org/10.1007/ JHEP10(2023)059

  14. [14]

    Aoufia, I

    C. Aoufia, I. Basile, and G. Leone, JHEP, 12, 111 (2024), arXiv:2405.03683, https://doi.org/10.1007/ JHEP12(2024)111

  15. [15]

    Valeixo Bento and J

    B. Valeixo Bento and J. F. Melo, JHEP, 05, 212 (2025), arXiv:2501.08230, https://doi.org/10.1007/ JHEP05(2025)212

  16. [16]

    van de Heisteeg, C

    D. van de Heisteeg, C. Vafa, M. Wiesner, and D. H. Wu, Beijing J. Pure Appl. Math.,1(1), 1–41 (2024), arXiv:2212.06841, https://doi.org/10.4310/bpam.2024.v1.n1.a1

  17. [17]

    Cribiori, D

    N. Cribiori, D. Lüst, and G. Staudt, Phys. Lett. B,844, 138113 (2023), arXiv:2212.10286,https://doi.org/ 10.1016/j.physletb.2023.138113

  18. [18]

    Castellano, A

    A. Castellano, A. Herráez, and L. E. Ibáñez, JHEP,12, 019 (2024), arXiv:2310.07708,https://doi.org/10. 1007/JHEP12(2024)019

  19. [19]

    van de Heisteeg, C

    D. van de Heisteeg, C. Vafa, and M. Wiesner, Fortsch. Phys.,71(10-11), 2300143 (2023), arXiv:2303.13580, https://doi.org/10.1002/prop.202300143

  20. [20]

    van de Heisteeg, C

    D. van de Heisteeg, C. Vafa, M. Wiesner, and D. H. Wu, JHEP,05, 112 (2024), arXiv:2310.07213, https: //doi.org/10.1007/JHEP05(2024)112

  21. [21]

    Calderón-Infante, M

    J. Calderón-Infante, M. Delgado, and A. M. Uranga, JHEP,01, 003 (2024), arXiv:2310.04488,https://doi. org/10.1007/JHEP01(2024)003

  22. [22]

    Castellano, I

    A. Castellano, I. Ruiz, and I. Valenzuela, Phys. Rev. Lett.,132(18), 181601 (2024), arXiv:2311.01501,https: //doi.org/10.1103/PhysRevLett.132.181601

  23. [23]

    Cribiori and D

    N. Cribiori and D. Lüst, Fortsch. Phys.,71(10-11), 2300150 (2023), arXiv:2306.08673,https://doi.org/10. 22 1002/prop.202300150

  24. [24]

    Bedroya, R

    A. Bedroya, R. K. Mishra, and M. Wiesner, JHEP,01, 144 (2025), arXiv:2405.00083, https://doi.org/10. 1007/JHEP01(2025)144

  25. [25]

    Bedroya, C

    A. Bedroya, C. Vafa, and D. H. Wu, Phys. Rev. D,113(10), 106011 (2026), arXiv:2403.18005,https://doi. org/10.1103/4lsn-l2ln

  26. [26]

    Castellano, The Quantum Gravity Scale and the Swampland, PhD thesis, U

    A. Castellano, The Quantum Gravity Scale and the Swampland, PhD thesis, U. Autonoma, Madrid (main) (2024), arXiv:2409.10003

  27. [27]

    A.CastellanoandM.Zatti,JHEP, 08,112(2025),arXiv:2502.02655, https://doi.org/10.1007/JHEP08(2025) 112

  28. [28]

    Aoufia, A

    C. Aoufia, A. Castellano, and L. Ibáñez, JHEP,02, 203 (2026), arXiv:2506.03253,https://doi.org/10.1007/ JHEP02(2026)203

  29. [29]

    Basile, N

    I. Basile, N. Cribiori, D. Lust, and C. Montella, JHEP,06, 127 (2024), arXiv:2401.06851,https://doi.org/ 10.1007/JHEP06(2024)127

  30. [30]

    Herráez, D

    A. Herráez, D. Lüst, J. Masias, and M. Scalisi, SciPost Phys.,18(3), 083 (2025), arXiv:2406.17851, https: //doi.org/10.21468/SciPostPhys.18.3.083

  31. [31]

    Caron-Huot and Y.-Z

    S. Caron-Huot and Y.-Z. Li, JHEP, 02, 115 (2025), arXiv:2408.06440, https://doi.org/10.1007/ JHEP02(2025)115

  32. [32]

    A. V. Manohar (April 2018), arXiv:1804.05863,https://doi.org/10.1093/oso/9780198855743.003.0002

  33. [33]

    C. P. Burgess, Introduction to Effective Field Theory, (Cambridge University Press, 12 2020),https://doi. org/10.1017/9781139048040

  34. [34]

    J. F. Donoghue, Phys. Rev. D,50, 3874–3888 (1994), gr-qc/9405057,https://doi.org/10.1103/PhysRevD. 50.3874

  35. [35]

    J. F. Donoghue, Quantum General Relativity and Effective Field Theory(2023), arXiv:2211.09902, https: //doi.org/10.1007/978-981-19-3079-9_1-1

  36. [36]

    J. C. Criado and M. Pérez-Victoria, JHEP, 03, 038 (2019), arXiv:1811.09413, https://doi.org/10.1007/ JHEP03(2019)038

  37. [37]

    Ooguri and C

    H. Ooguri and C. Vafa, Nucl. Phys. B,766, 21–33 (2007), hep-th/0605264,https://doi.org/10.1016/j. nuclphysb.2006.10.033

  38. [38]

    T. W. Grimm, E. Palti, and I. Valenzuela, JHEP,08, 143 (2018), arXiv:1802.08264, https://doi.org/10. 1007/JHEP08(2018)143

  39. [39]

    Heidenreich, M

    B. Heidenreich, M. Reece, and T. Rudelius, Eur. Phys. J., C78(4), 337 (2018), arXiv:1712.01868, https: //doi.org/10.1140/epjc/s10052-018-5811-3

  40. [40]

    Heidenreich, M

    B. Heidenreich, M. Reece, and T. Rudelius, Phys. Rev. Lett.,121(5), 051601 (2018), arXiv:1802.08698,https: //doi.org/10.1103/PhysRevLett.121.051601

  41. [41]

    Montero, C

    M. Montero, C. Vafa, and I. Valenzuela, JHEP,02, 022 (2023), arXiv:2205.12293,https://doi.org/10.1007/ JHEP02(2023)022

  42. [42]

    Etheredge, B

    M. Etheredge, B. Heidenreich, J. McNamara, T. Rudelius, I. Ruiz, and I. Valenzuela, JHEP,12, 182 (2023), arXiv:2306.16440, https://doi.org/10.1007/JHEP12(2023)182

  43. [43]

    Etheredge, B

    M. Etheredge, B. Heidenreich, T. Rudelius, I. Ruiz, and I. Valenzuela, JHEP,03, 213 (2025), arXiv:2405.20332, https://doi.org/10.1007/JHEP03(2025)213

  44. [44]

    Blumenhagen, N

    R. Blumenhagen, N. Cribiori, A. Gligovic, and A. Paraskevopoulou, Phys. Rev. D,109(2), L021901 (2024), arXiv:2309.11554, https://doi.org/10.1103/PhysRevD.109.L021901

  45. [45]

    D. V. Vassilevich, Phys. Rept.,388, 279–360 (2003), hep-th/0306138,https://doi.org/10.1016/j.physrep. 2003.09.002

  46. [46]

    P. B. Gilkey,Invariance theory, the heat equation and the Atiyah-Singer index theorem, (CRC Press, 1995)

  47. [47]

    I. G. Avramidi,Heat kernel and quantum gravity, volume 64, (Springer, New York, 2000),https://doi.org/ 10.1007/3-540-46523-5

  48. [48]

    I. G. Avramidi, Nucl. Phys. B, 355, 712–754, [Erratum: Nucl.Phys.B 509, 557–558 (1998)] (1991),https: //doi.org/10.1016/0550-3213(91)90492-G

  49. [49]

    I. G. Avramidi, Phys. Lett. B,238, 92–97 (1990),https://doi.org/10.1016/0370-2693(90)92105-R

  50. [50]

    De Berredo-Peixoto, Mod

    G. De Berredo-Peixoto, Mod. Phys. Lett. A,16, 2463–2468 (2001), hep-th/0108223,https://doi.org/10. 1142/S0217732301005965

  51. [51]

    Kontsevich and S

    M. Kontsevich and S. Vishik (June 1994), hep-th/9406140

  52. [52]

    One-loop corrections to the photon propagator in the curved-space QED

    B. Goncalves, G. de Berredo-Peixoto, and I. L. Shapiro, Phys. Rev. D,80, 104013 (2009), arXiv:0906.3837, https://doi.org/10.1103/PhysRevD.80.104013

  53. [53]

    Elizalde, L

    E. Elizalde, L. Vanzo, and S. Zerbini, Commun. Math. Phys.,194, 613–630 (1998), hep-th/9701060,https: //doi.org/10.1007/s002200050371

  54. [54]

    Applications in physics of the multiplicative anomaly formula involving some basic differential operators

    E. Elizalde, G. Cognola, and S. Zerbini, Nucl. Phys. B,532, 407–428 (1998), hep-th/9804118,https://doi. 23 org/10.1016/S0550-3213(98)00442-8

  55. [55]

    On the concept of determinant for the differential operators of Quantum Physics

    E. Elizalde, JHEP, 07, 015 (1999), hep-th/9906229,https://doi.org/10.1088/1126-6708/1999/07/015

  56. [56]

    Dirac Functional Determinants in Terms of the Eta Invariant and the Noncommutative Residue

    G. Cognola, E. Elizalde, and S. Zerbini, Commun. Math. Phys.,237, 507–532 (2003), hep-th/9910038,https: //doi.org/10.1007/s00220-003-0844-2

  57. [57]

    Naturalness and UV sensitivity in Kaluza-Klein theories

    C. Branchina, V. Branchina, and F. Contino, Phys. Rev. D,108(4), 045007 (2023), arXiv:2304.08040,https: //doi.org/10.1103/PhysRevD.108.045007

  58. [58]

    Contino and L

    R. Contino and L. Pilo, Phys. Lett. B,523, 347–350 (2001), hep-ph/0104130,https://doi.org/10.1016/ S0370-2693(01)01352-1

  59. [59]

    M. M. Anber, J. F. Donoghue, and M. El-Houssieny, Phys. Rev. D,83, 124003 (2011), arXiv:1011.3229,https: //doi.org/10.1103/PhysRevD.83.124003

  60. [60]

    M. M. Anber and J. F. Donoghue, Phys. Rev. D,85, 104016 (2012), arXiv:1111.2875,https://doi.org/10. 1103/PhysRevD.85.104016

  61. [61]

    ’t Hooft and M

    G. ’t Hooft and M. J. G. Veltman, Ann. Inst. H. Poincare A Phys. Theor.,20, 69–94 (1974)

  62. [62]

    Calderón-Infante, A

    J. Calderón-Infante, A. Castellano, and A. Herráez, SciPost Phys.,19(4), 096 (2025), arXiv:2501.14880,https: //doi.org/10.21468/SciPostPhys.19.4.096

  63. [63]

    van Beest, J

    M. van Beest, J. Calderón-Infante, D. Mirfendereski, and I. Valenzuela, Phys. Rept., 989, 1–50 (2022), arXiv:2102.01111, https://doi.org/10.1016/j.physrep.2022.09.002

  64. [64]

    Adams, N

    A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis, and R. Rattazzi, JHEP,10, 014 (2006), hep-th/0602178, https://doi.org/10.1088/1126-6708/2006/10/014

  65. [65]

    P. F. Mende and H. Ooguri, Nucl. Phys. B,339, 641–662 (1990),https://doi.org/10.1016/0550-3213(90) 90202-O

  66. [66]

    Basile, D

    I. Basile, D. Lüst, and C. Montella, JHEP, 07, 208 (2024), arXiv:2311.12113, https://doi.org/10.1007/ JHEP07(2024)208

  67. [67]

    S.-J. Lee, W. Lerche, and T. Weigand, JHEP,02, 190 (2022), arXiv:1910.01135,https://doi.org/10.1007/ JHEP02(2022)190

  68. [68]

    Antoniadis, E

    I. Antoniadis, E. Gava, and K. S. Narain, Phys. Lett. B,283, 209–212 (1992), hep-th/9203071,https://doi. org/10.1016/0370-2693(92)90009-S

  69. [69]

    M. B. Green and P. Vanhove, Phys. Rev. D,61, 104011 (2000), hep-th/9910056,https://doi.org/10.1103/ PhysRevD.61.104011

  70. [70]

    Ooguri, Soryushiron Kenkyu,70(3), 231–249, in Japanese (1984),https://doi.org/10.24532/soken.70

    H. Ooguri, Soryushiron Kenkyu,70(3), 231–249, in Japanese (1984),https://doi.org/10.24532/soken.70. 3_231

  71. [71]

    Hörmander, The Analysis of Linear Partial Differential Operators I: Distribution Theory and Fourier Analysis, Classics in Mathematics

    L. Hörmander, The Analysis of Linear Partial Differential Operators I: Distribution Theory and Fourier Analysis, Classics in Mathematics. (Springer, Berlin, Heidelberg, 2 edition, 2003),https://doi.org/10.1007/ 978-3-642-61497-2

  72. [72]

    R. P. Kanwal, Generalized Functions: Theory and Technique, (Birkhäuser, Boston, MA, 2 edition, 1998), https://doi.org/10.1007/978-1-4684-0035-9

  73. [73]

    I. M. Gel’fand and G. E. Shilov,Generalized Functions, Volume 1: Properties and Operations, volume 377 of AMS Chelsea Publishing, (American Mathematical Society, Providence, RI, 1964)

  74. [74]

    Flajolet, X

    P. Flajolet, X. Gourdon, and P. Dumas, Theoretical Computer Science,144(1), 3–58 (1995),https://doi. org/10.1016/0304-3975(95)00002-E

  75. [75]

    Bochner, Annals of Mathematics,53(2), 332–363 (1951)

    S. Bochner, Annals of Mathematics,53(2), 332–363 (1951)

  76. [76]

    Kanemitsu, Y

    S. Kanemitsu, Y. Tanigawa, and M. Yoshimoto, Developments in Mathematics,8 (01 2002), https://doi. org/10.1007/978-1-4757-3675-5_10

  77. [77]

    A. F. Lavrik, Mathematics of the USSR-Izvestiya, 36(3), 519 (jun 1991), https://doi.org/10.1070/ IM1991v036n03ABEH002033

  78. [78]

    Kanemitsu, Y

    S. Kanemitsu, Y. Tanigawa, and M. Yoshimoto, Abhandlungen aus dem Mathematischen Seminar der Universität Hamburg, 72(1), 187–206 (dec 2002),https://doi.org/10.1007/BF02941671

  79. [79]

    B. C. Berndt, Y. Lee, and J. Sohn,Koshliakovs Formula and Guinands Formula in Ramanujans Lost Notebook, pages 1–22, Springer New York, New York, NY (2008),https://doi.org/10.1007/978-0-387-78510-3_2

  80. [80]

    G. N. WATSON, The Quarterly Journal of Mathematics,os-2(1), 298–309 (01 1931),https://doi.org/10. 1093/qmath/os-2.1.298

Showing first 80 references.