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.
Kaluza-Klein tower thresholds and scheme dependence of the species scale
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
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.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
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)
- 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.
- 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).
- 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.
- 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.
- 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.
- 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
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
free parameters (1)
- cutoff-profile parameter alpha (illustrative)
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).
- 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.
- 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.
- 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.
- domain assumption The renormalized UV matching contribution is neither parametrically larger than the tower term nor tuned to cancel it.
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.
Reference graph
Works this paper leans on
-
[1]
G. Dvali, Fortsch. Phys.,58, 528–536 (2010), arXiv:0706.2050,https://doi.org/10.1002/prop.201000009
-
[2]
G. Dvali and M. Redi, Phys. Rev. D, 77, 045027 (2008), arXiv:0710.4344, https://doi.org/10.1103/ PhysRevD.77.045027
Pith/arXiv arXiv 2008
-
[3]
G. Dvali and D. Lüst, Fortsch. Phys.,58, 505–527 (2010), arXiv:0912.3167,https://doi.org/10.1002/prop. 201000008
- [4]
-
[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]
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
Pith/arXiv arXiv 2005
-
[7]
G. Dvali, C. Gomez, and D. Lust, Fortsch. Phys.,61, 768–778 (2013), arXiv:1206.2365,https://doi.org/10. 1002/prop.201300002
Pith/arXiv arXiv 2013
-
[8]
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]
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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.physletb.2017.09.080 2017
-
[10]
A. Castellano, A. Herráez, and L. E. Ibáñez, JHEP,06, 047 (2023), arXiv:2212.03908,https://doi.org/10. 1007/JHEP06(2023)047
Pith/arXiv arXiv 2023
-
[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]
A. Castellano, I. Ruiz, and I. Valenzuela, JHEP,06, 037 (2024), arXiv:2311.01536,https://doi.org/10.1007/ JHEP06(2024)037
Pith/arXiv arXiv 2024
-
[13]
N. Cribiori, D. Lust, and C. Montella, JHEP,10, 059 (2023), arXiv:2305.10489, https://doi.org/10.1007/ JHEP10(2023)059
Pith/arXiv arXiv 2023
-
[14]
C. Aoufia, I. Basile, and G. Leone, JHEP, 12, 111 (2024), arXiv:2405.03683, https://doi.org/10.1007/ JHEP12(2024)111
Pith/arXiv arXiv 2024
-
[15]
B. Valeixo Bento and J. F. Melo, JHEP, 05, 212 (2025), arXiv:2501.08230, https://doi.org/10.1007/ JHEP05(2025)212
Pith/arXiv arXiv 2025
-
[16]
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]
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]
A. Castellano, A. Herráez, and L. E. Ibáñez, JHEP,12, 019 (2024), arXiv:2310.07708,https://doi.org/10. 1007/JHEP12(2024)019
Pith/arXiv arXiv 2024
-
[19]
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]
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]
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]
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]
N. Cribiori and D. Lüst, Fortsch. Phys.,71(10-11), 2300150 (2023), arXiv:2306.08673,https://doi.org/10. 22 1002/prop.202300150
Pith/arXiv arXiv 2023
-
[24]
A. Bedroya, R. K. Mishra, and M. Wiesner, JHEP,01, 144 (2025), arXiv:2405.00083, https://doi.org/10. 1007/JHEP01(2025)144
Pith/arXiv arXiv 2025
-
[25]
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]
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
Pith/arXiv arXiv 2024
-
[27]
A.CastellanoandM.Zatti,JHEP, 08,112(2025),arXiv:2502.02655, https://doi.org/10.1007/JHEP08(2025) 112
- [28]
-
[29]
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]
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]
S. Caron-Huot and Y.-Z. Li, JHEP, 02, 115 (2025), arXiv:2408.06440, https://doi.org/10.1007/ JHEP02(2025)115
Pith/arXiv arXiv 2025
-
[32]
A. V. Manohar (April 2018), arXiv:1804.05863,https://doi.org/10.1093/oso/9780198855743.003.0002
Pith/arXiv arXiv doi:10.1093/oso/9780198855743.003.0002 2018
-
[33]
C. P. Burgess, Introduction to Effective Field Theory, (Cambridge University Press, 12 2020),https://doi. org/10.1017/9781139048040
-
[34]
J. F. Donoghue, Phys. Rev. D,50, 3874–3888 (1994), gr-qc/9405057,https://doi.org/10.1103/PhysRevD. 50.3874
-
[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]
J. C. Criado and M. Pérez-Victoria, JHEP, 03, 038 (2019), arXiv:1811.09413, https://doi.org/10.1007/ JHEP03(2019)038
Pith/arXiv arXiv 2019
-
[37]
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
Pith/arXiv arXiv doi:10.1016/j 2007
-
[38]
T. W. Grimm, E. Palti, and I. Valenzuela, JHEP,08, 143 (2018), arXiv:1802.08264, https://doi.org/10. 1007/JHEP08(2018)143
Pith/arXiv arXiv 2018
-
[39]
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]
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]
M. Montero, C. Vafa, and I. Valenzuela, JHEP,02, 022 (2023), arXiv:2205.12293,https://doi.org/10.1007/ JHEP02(2023)022
Pith/arXiv arXiv 2023
-
[42]
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]
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]
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]
D. V. Vassilevich, Phys. Rept.,388, 279–360 (2003), hep-th/0306138,https://doi.org/10.1016/j.physrep. 2003.09.002
-
[46]
P. B. Gilkey,Invariance theory, the heat equation and the Atiyah-Singer index theorem, (CRC Press, 1995)
1995
-
[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]
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]
I. G. Avramidi, Phys. Lett. B,238, 92–97 (1990),https://doi.org/10.1016/0370-2693(90)92105-R
-
[50]
G. De Berredo-Peixoto, Mod. Phys. Lett. A,16, 2463–2468 (2001), hep-th/0108223,https://doi.org/10. 1142/S0217732301005965
Pith/arXiv arXiv 2001
- [51]
-
[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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.80.104013 2009
-
[53]
E. Elizalde, L. Vanzo, and S. Zerbini, Commun. Math. Phys.,194, 613–630 (1998), hep-th/9701060,https: //doi.org/10.1007/s002200050371
-
[54]
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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/s0550-3213(98)00442-8 1998
-
[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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1126-6708/1999/07/015 1999
-
[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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/s00220-003-0844-2 2003
-
[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
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.108.045007 2023
-
[58]
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
Pith/arXiv arXiv 2001
-
[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]
M. M. Anber and J. F. Donoghue, Phys. Rev. D,85, 104016 (2012), arXiv:1111.2875,https://doi.org/10. 1103/PhysRevD.85.104016
Pith/arXiv arXiv 2012
-
[61]
’t Hooft and M
G. ’t Hooft and M. J. G. Veltman, Ann. Inst. H. Poincare A Phys. Theor.,20, 69–94 (1974)
1974
-
[62]
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]
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]
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]
P. F. Mende and H. Ooguri, Nucl. Phys. B,339, 641–662 (1990),https://doi.org/10.1016/0550-3213(90) 90202-O
-
[66]
I. Basile, D. Lüst, and C. Montella, JHEP, 07, 208 (2024), arXiv:2311.12113, https://doi.org/10.1007/ JHEP07(2024)208
Pith/arXiv arXiv 2024
-
[67]
S.-J. Lee, W. Lerche, and T. Weigand, JHEP,02, 190 (2022), arXiv:1910.01135,https://doi.org/10.1007/ JHEP02(2022)190
Pith/arXiv arXiv 2022
-
[68]
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]
M. B. Green and P. Vanhove, Phys. Rev. D,61, 104011 (2000), hep-th/9910056,https://doi.org/10.1103/ PhysRevD.61.104011
Pith/arXiv arXiv 2000
-
[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]
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
2003
-
[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]
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)
1964
-
[74]
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]
Bochner, Annals of Mathematics,53(2), 332–363 (1951)
S. Bochner, Annals of Mathematics,53(2), 332–363 (1951)
1951
-
[76]
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]
A. F. Lavrik, Mathematics of the USSR-Izvestiya, 36(3), 519 (jun 1991), https://doi.org/10.1070/ IM1991v036n03ABEH002033
1991
-
[78]
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]
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]
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
1931
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