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arxiv: 2512.07904 · v2 · submitted 2025-12-07 · ⚛️ physics.gen-ph

Schr\"odinger and Klein-Gordon oscillators in Eddington-inspired Born-Infeld gravity: Degree-one Confluent Heun polynomial correspondence

Pith reviewed 2026-05-17 01:35 UTC · model grok-4.3

classification ⚛️ physics.gen-ph
keywords Eddington-inspired Born-Infeld gravityglobal monopoleconfluent Heun equationoscillatorKlein-Gordon equationSchrödinger equationWu-Yang monopoleangular deficit
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The pith

Degree-one confluent Heun polynomials supply closed frequencies and an upper bound on angular momentum for Schrödinger and Klein-Gordon oscillators in Eddington-inspired Born-Infeld gravity with a global monopole.

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

The paper reduces the radial equations for these oscillators in the EiBI global-monopole spacetime to the confluent Heun equation. Termination of the Heun series at the lowest nontrivial degree yields algebraic constraints that fix the oscillator frequency analytically and restrict orbital angular momentum ℓ to a finite range set by the EiBI deformation parameter and the monopole angular deficit. The same truncation produces exact particle and antiparticle energies for the Klein-Gordon case coupled to a Wu-Yang magnetic monopole, preserving charge symmetry. A sympathetic reader would care because the geometric parameters of the modified gravity theory and the monopole directly select which bound states exist through the polynomial termination condition.

Core claim

In the lowest nontrivial case n=0, the degree-one Heun polynomial yields a closed analytic expression for the frequency and determines a finite upper bound on ℓ, dictated jointly by the EiBI deformation and the GM deficit. The resulting parametric correlations reveal a sharp geometric control of the spectrum. Applying the same method to the KG oscillator with a WYMM produces conditionally exact particle and antiparticle energies in closed form that exhibit perfect charge symmetry and dependence on the WYMM strength together with the EiBI parameter and the angular momentum constraint.

What carries the argument

The degree-one confluent Heun polynomial obtained by enforcing termination of the series solution to the radial equation after the first term.

Load-bearing premise

The radial equations reduce exactly to the confluent Heun equation and termination of the series at degree one produces normalizable bound states without instabilities or violation of the field equations.

What would settle it

Direct substitution of the derived closed-form frequency back into the original radial differential equation to check whether the Heun series indeed terminates and satisfies the equation for the claimed range of ℓ.

Figures

Figures reproduced from arXiv: 2512.07904 by Abdullah Guvendi, Omar Mustafa.

Figure 1
Figure 1. Figure 1: FIG. 1 [PITH_FULL_IMAGE:figures/full_fig_p004_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2 [PITH_FULL_IMAGE:figures/full_fig_p005_2.png] view at source ↗
read the original abstract

We investigate Schr\"odinger and Klein-Gordon (KG) oscillators in the spacetime of a global monopole (GM) within Eddington inspired Born-Infeld (EiBI) gravity, including, in the relativistic sector, the coupling to a Wu-Yang magnetic monopole (WYMM). By reducing the radial equations to the confluent Heun form and enforcing termination of the Heun series, we obtain conditionally exact solutions in which the radial eigenfunctions truncate to polynomials of degree $(n+1)\geq 1$. This truncation imposes algebraic constraints that quantize the oscillator frequency and restrict the values allowed for the orbital angular momenta $\ell$. In the lowest nontrivial case $n=0$, the degree-one Heun polynomial yields a closed analytic expression for the frequency and determines a finite upper bound on $\ell$, dictated jointly by the EiBI deformation and the GM deficit. The resulting parametric correlations reveal a sharp geometric control of the spectrum: EiBI nonlinearities and the angular deficit fix the admissible bound states through polynomial truncation conditions. The confluent Heun correspondence is made explicit, providing a rigorous and reproducible framework for extracting analytical solutions from otherwise non-polynomial Heun structures. Applying the same method to the KG oscillator with a WYMM, we derive conditionally exact particle and antiparticle energies in a closed form. The relativistic spectrum exhibits perfect charge symmetry and a precise dependence on the WYMM strength, the EiBI parameter and the angular momentum constraint. To the best of our knowledge, this constitutes the first unified and fully consistent treatment of conditionally exact Schr\"odinger and Klein-Gordon oscillators in EiBI gravity based on a degree-one confluent Heun polynomial.

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 investigates Schrödinger and Klein-Gordon oscillators in the spacetime of a global monopole within Eddington-inspired Born-Infeld gravity, including Wu-Yang magnetic monopole coupling in the relativistic sector. The radial equations are reduced to the confluent Heun equation; termination of the series at degree one for the lowest nontrivial case n=0 yields algebraic constraints that quantize the oscillator frequency, impose a finite upper bound on orbital angular momentum ℓ, and reveal parametric correlations controlled by the EiBI deformation parameter and the monopole deficit angle. The authors present closed-form expressions for frequencies and energies, claiming this provides the first unified treatment of such conditionally exact solutions via explicit Heun polynomial correspondence.

Significance. If the reductions are exact and the resulting polynomials are verified to solve the original radial operators while remaining normalizable under the modified measure, the work would supply analytic control over spectra in nonlinear gravitational backgrounds, illustrating how geometric parameters (EiBI nonlinearity and angular deficit) enforce quantization through truncation conditions. This could serve as a template for extracting exact solutions from otherwise intractable Heun structures in modified gravity.

major comments (2)
  1. [Section on n=0 termination and frequency expression] The central derivation asserts that the radial equations in the EiBI global-monopole metric reduce exactly to the confluent Heun equation, yet the manuscript provides no explicit back-substitution of the degree-one polynomial (after standard prefactors from the radial coordinate change) into the unreduced second-order radial ODE to confirm it satisfies the original operator identically. This verification is load-bearing for the claim of physically acceptable normalizable bound states.
  2. [Discussion of normalizability and boundary conditions] No computation of the norm integral is reported for the degree-one solution with respect to the proper radial measure induced by the metric (including the angular-deficit factor and any EiBI modifications to the volume element). Without this, it remains unclear whether the algebraic constraint produces square-integrable states or introduces divergences at large r, undermining the bound-state interpretation.
minor comments (2)
  1. [Introduction] The abstract refers to 'conditionally exact solutions' without a concise definition in the introduction; adding one sentence clarifying that these are solutions valid only when the truncation conditions on parameters are met would improve clarity.
  2. [Metric and field equations] Notation for the EiBI deformation parameter and deficit angle should be introduced once with explicit symbols in the metric ansatz section and used consistently thereafter to avoid ambiguity in the parametric correlations.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the thorough review and valuable comments, which help improve the clarity and rigor of our work. We address the major comments point by point below, and indicate the revisions we will make to the manuscript.

read point-by-point responses
  1. Referee: The central derivation asserts that the radial equations in the EiBI global-monopole metric reduce exactly to the confluent Heun equation, yet the manuscript provides no explicit back-substitution of the degree-one polynomial (after standard prefactors from the radial coordinate change) into the unreduced second-order radial ODE to confirm it satisfies the original operator identically. This verification is load-bearing for the claim of physically acceptable normalizable bound states.

    Authors: We agree that an explicit verification by back-substituting the degree-one Heun polynomial into the original radial ODE would strengthen the manuscript. Although the reduction steps are detailed in the paper, the direct confirmation that the truncated solution satisfies the unreduced equation under the frequency constraint was not explicitly shown. In the revised version, we will include this calculation for the n=0 case, demonstrating that the proposed analytic solution fulfills the original differential equation identically. This addition will support the claim of conditionally exact solutions. revision: yes

  2. Referee: No computation of the norm integral is reported for the degree-one solution with respect to the proper radial measure induced by the metric (including the angular-deficit factor and any EiBI modifications to the volume element). Without this, it remains unclear whether the algebraic constraint produces square-integrable states or introduces divergences at large r, undermining the bound-state interpretation.

    Authors: The referee correctly notes the absence of an explicit norm computation. In our analysis, the polynomial truncation ensures the appropriate asymptotic decay at large r, and the metric-induced measure (incorporating the deficit angle) is accounted for in the radial equation setup. However, to address this directly, we will add in the revision an evaluation of the normalization integral for the degree-one solutions, confirming square-integrability within the allowed ranges of the EiBI parameter and angular momentum bound. This will clarify that no divergences arise at infinity for the physically relevant parameter values. revision: yes

Circularity Check

1 steps flagged

Heun truncation conditions algebraically constrain frequency and ℓ from metric parameters

specific steps
  1. fitted input called prediction [Abstract]
    "In the lowest nontrivial case n=0, the degree-one Heun polynomial yields a closed analytic expression for the frequency and determines a finite upper bound on ℓ, dictated jointly by the EiBI deformation and the GM deficit."

    The frequency is obtained by solving the algebraic termination condition that forces the Heun series to stop at degree one. Because this condition is written directly in terms of the oscillator frequency, ℓ, the EiBI parameter and the deficit angle (all of which already appear in the radial equation), the 'closed analytic expression' is simply the root of that constraint equation and does not constitute an independent derivation.

full rationale

The paper reduces the radial ODE to confluent Heun form and then imposes series termination at degree one to obtain a closed-form frequency and an upper bound on ℓ. This termination condition is an algebraic relation among the very parameters that enter the original radial equation (oscillator frequency, angular momentum, EiBI deformation parameter, and global-monopole deficit). The resulting expression is therefore the direct solution of that imposed constraint rather than an independent prediction extracted from the field equations or from an external benchmark. No explicit back-substitution into the unreduced radial operator or verification of square-integrability with the metric measure is described, leaving the claimed eigenfunction status dependent on the truncation ansatz itself. This constitutes a moderate circularity: the quantization is real but is generated by construction from the chosen termination requirement applied to input parameters.

Axiom & Free-Parameter Ledger

2 free parameters · 1 axioms · 0 invented entities

Central results rest on the assumption that the chosen spacetime metric permits exact reduction to confluent Heun form and that truncation conditions are sufficient for physical solutions. No new entities are postulated; the EiBI parameter and monopole deficit function as external inputs whose values are constrained rather than derived.

free parameters (2)
  • EiBI deformation parameter
    Nonlinear gravity parameter whose value is restricted by the polynomial termination condition rather than predicted from first principles.
  • Global monopole deficit angle
    Geometric parameter fixed by the monopole topology and jointly constrained with the EiBI parameter by the truncation algebra.
axioms (1)
  • domain assumption The line element for a global monopole in Eddington-inspired Born-Infeld gravity permits separation of variables that reduces the radial oscillator equation to confluent Heun form.
    Invoked at the start of the analytic procedure described in the abstract.

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Works this paper leans on

57 extracted references · 57 canonical work pages

  1. [1]

    KG-oscillators in EiBI gravity spacetime 4 V

    Degree-one Confluent Heun polynomial correspondence 4 IV. KG-oscillators in EiBI gravity spacetime 4 V. Concluding remarks 5 References 6 I. INTRODUCTION Gravity is inherently portrayed as a geometric manifestati on of space- time by Einstein’s pioneering groundbreaking theory of gen eral relativ- ity (GR) [1]. GR has sparked significant interest in profoun...

  2. [2]

    Strictly speaking, for 0 < ˜α < √ 66/ 11 the only allowed value is ℓ = 0 and for √ 66/ 11 ≤ ˜α < 1 the allowed values are ℓ = 0, 1

    Hence, the maximum value for the angular momentum quantum number is an integer and reads ℓmax = 1. Strictly speaking, for 0 < ˜α < √ 66/ 11 the only allowed value is ℓ = 0 and for √ 66/ 11 ≤ ˜α < 1 the allowed values are ℓ = 0, 1. In Figure 1, we meticulously follow the parametric restrictions men- tioned above and show the Schr¨ odinger oscillator energi...

  3. [3]

    Degree-one Confluent Heun polynomial correspondence Next, for the case n = 0 we have our confluent Heun polynomial of degree one in the form of H0(s) = HC, 0 (α, β, γ, δ, η, s ) = A0 + A1s. A straightforward textbook substitution of H0(s) in ( 24) would yield for s2 coefficient ⇒ µ 0 + ν = − α ⇒ µ 0 + ν = ˜κω 2 for s1 coefficient ⇒ (P − µ 0)A1 = − (µ 0 + ν)A0 ⇒...

  4. [4]

    Einstein, ”The basis of general relativity ” Ann

    A. Einstein, ”The basis of general relativity ” Ann. Phys. (Berlin) 354 (1916) 769

  5. [5]

    T W B Kibble, ”Some implications of a cosmological phase tran - sition” Phys. Rep. 67 (1980) 183

  6. [6]

    M Barriola, A Vilenkin, ”Gravitational field of a global mono pole” Phys. Rev. Lett. 63 (1989) 341

  7. [7]

    A Vilenkin, ”Cosmic strings and domain walls” Phys. Rep. 121 (1985) 263

  8. [8]

    A Vilenkin, ”Gravitational field of vacuum domain walls and strings” Phys. Rev. D 23 (1981) 852

  9. [9]

    A Vilenkin, ”Cosmological Density Fluctuations Produced b y Vac- uum Strings” Phys. Rev. Lett. 46 (1988) 1169

  10. [10]

    A Vilenkin, ”Gravitational field of vacuum domain walls” Phys. Lett. B 133 (1983) 177

  11. [11]

    W A Hiscock, ”Exact gravitational field of a string” Phys. Rev. D 31 (1985) 3288

  12. [12]

    B Linet, ”The static metrics with cylindrical symmetry desc ribing a model of cosmic strings” Gen. Rel. Gravit. 17 (1985) 1109

  13. [13]

    Deser, G.W

    S. Deser, G.W. Gibbons, ”Born-Infeld-Einstein actions?” Class. Quant. Grav. 15 (1998) L35

  14. [14]

    Ba˜ nados, P.G

    M. Ba˜ nados, P.G. Ferreira, ”Eddington’s theory of gravity and its progeny” Phys. Rev. Lett. 105 011101 (2010) . [Erratum: Phys. Rev. Lett. 113 (2014) 119901. ]

  15. [15]

    M. Born, L. Infeld, ”Foundations of the new field theory” Proc. Roy. Soc. A 144 (1934) 425

  16. [16]

    Vollick, ”Palatini approach to Born-Infeld-Einstein theory and a geometric description of electrodynamics” Phys

    D.N. Vollick, ”Palatini approach to Born-Infeld-Einstein theory and a geometric description of electrodynamics” Phys. Rev. D 69 (2004) 064030

  17. [17]

    Delsate, J

    T. Delsate, J. Steinhoff, ”New insights on the matter–gravit y cou- pling paradigm” Phys. Rev. Lett. 109 (2012) 021101

  18. [18]

    Avelino, ”Eddington-inspired Born-Infeld gravity: A strophys- ical and cosmological constraints” Phys

    P.P. Avelino, ”Eddington-inspired Born-Infeld gravity: A strophys- ical and cosmological constraints” Phys. Rev. D 85 104053 (2012)

  19. [19]

    P. Pani, V. Cardoso, T. Delsate, ”Compact stars in Eddington inspired gravity” Phys. Rev. Lett. 107 (2011) 031101

  20. [20]

    P. Pani, T. Delsate, V. Cardoso, ”Eddington-inspired Born- Infeld gravity: Phenomenology of nonlinear gravity–matter coupl ing” Phys. Rev. D 85 (2012) 084020

  21. [21]

    Fiorini, R

    F. Fiorini, R. Ferraro, ”A type of Born-Infeld reg- ular gravity and its cosmological consequences” Int. J. Mod. Phys. A 24 (2009)1686

  22. [22]

    Sham, P.T

    Y.-H. Sham, P.T. Leung, L.-M. Lin, ”Compact stars in Eddingt on- inspired Born-Infeld gravity: Anomalies associated with p hase transitions” Phys. Rev. D 87 (2013) 061503(R)

  23. [23]

    Harko, F.S.N

    T. Harko, F.S.N. Lobo, M.K. Mak, S.V. Sushkov, ”Modified-gravity wormholes without exotic matter” Phys. Rev.D 87 (2013) 067504

  24. [24]

    Lambaga, H.S

    R.D. Lambaga, H.S. Ramadhan, ”Gravitational field of global monopole within the Eddington-inspired Born-Infeld theor y of 7 gravity” Eur. Phys. J. C 78 (2018) 436

  25. [25]

    Beltr´ an Jim´ enez, L

    J. Beltr´ an Jim´ enez, L. Heisenberg, G.J. Olmo, D. Rubiera- Garcia, ”On gravitational waves in Born-Infeld inspired non-singular cosmologies” JCAP 10 (2017) 029. [Erratum: JCAP 2018 (2018) E01 ]

  26. [26]

    A L Cavalcanti de Oliveira, E R Bezerra de Mello, ”Exact solut ions of the Klein-Gordon equation in the presence of a dyon, magne tic flux and scalar potential in the specetime of gravitational d efects” Class. Quant. Grav. 23 (2006) 5249

  27. [27]

    Caramˆ es, J.C

    T.R.P. Caramˆ es, J.C. Fabris, E R Bezerra de Mello, H Belich, ”f(R) global monopole revisited” Eur. Phys. J. C 77 (2017) 496

  28. [28]

    R L L Vit´ oria, H Belich, ”Harmonic oscillator in an environm ent with a pointlike defect” Phys. Scr. 94 (2019) 125301

  29. [29]

    O. Mustafa, ”Schr¨ odinger oscillators in a deformed point- like global monopole spacetime and a W u–Yang magnetic monopole: Position-dependent mass correspondence and iso spec- trality” Ann. Phys. 459 (2023) 169550

  30. [30]

    C Furtado, F Moraes, ”Harmonic oscillator interacting with coni- cal singularities” J. Phys. A: Math. Gen. 33 (2000) 5513

  31. [31]

    Banados, F

    M. Banados, F. Ferreira, ”Eddington’s Theory of Gravity and Its Progeny” Phys. Rev. Lett. 105 (2010) 011101. Erratum: [ Phys. Rev. Lett. 113 (2014) 119901. ]

  32. [32]

    Deser and G

    S. Deser and G. W. Gibbons, ”Born - Infeld - Einstein actions? ” Class. Quant. Grav. 15 (1998) L35

  33. [33]

    D. N. Vollick, ”Palatini approach to Born-Infeld-Einstein theory and a geometric description of electrodynamics” Phys. Rev. D 69 (2004) 064030

  34. [34]

    Delsate, J, Steinhoff, ”New Insights on the Matter-Gravit y Cou- pling Paradigm” Phys

    T. Delsate, J, Steinhoff, ”New Insights on the Matter-Gravit y Cou- pling Paradigm” Phys. Rev. Lett. 109 (2012) 021101

  35. [35]

    R.D Lambaga, H S Ramadhan, ”Gravitational field of global monopole within the Eddington-inspired Born-Infeld theor y of gravity” Eur. Phys. J. C 78 (2018) 436

  36. [36]

    J. R. Nascimento, G. J. Olmo, P. J. Porf ´ ırio, A. Yu. Petrov, A . R. Soares, ”Nonlinear σ -models in the Eddington-inspired Born- Infeld gravity” Phys. Rev. D 101 (2020) 064043

  37. [37]

    C F S Rereira, A R Soares, R L L Vit´ oria, H Belich, ”Bosonic quan- tum dynamics in Eddington-inspired Born–Infeld gravity gl obal monopole spacetime” Eur. Phys. J. C 83 (2023) 270

  38. [38]

    A R Soares, R L L Vit´ oria, C F S Rereira, ”Gravitational lensi ng in a topologically charged Eddington-inspired Born–Infel d space- time” Eur. Phys. J. C 83 (2023) 903

  39. [39]

    C F S Rereira, R L L Vit´ oria, A R Soares, H Belich, ”Gravitational Effects on a Position-Dependent Mass Quan- tum Particle in Eddington-Inspired Born-Infeld Spacetime ” Int. J. Theor. Phys. 62 (2023) 225

  40. [40]

    Mustafa, ”KG-oscillators in Eddington-inspired Born-I nfeld gravity: W u-Yang magnetic monopole and Ricci scalar curvat ure effects” Nucl

    O. Mustafa, ”KG-oscillators in Eddington-inspired Born-I nfeld gravity: W u-Yang magnetic monopole and Ricci scalar curvat ure effects” Nucl. Phys. B 1012 (2025) 116827

  41. [41]

    Mustafa, ”Klein–Gordon particles in a quasi- pointlike global monopole spacetime and a W u-Yang magnetic monopole: invariance and isospectrality” J

    O. Mustafa, ”Klein–Gordon particles in a quasi- pointlike global monopole spacetime and a W u-Yang magnetic monopole: invariance and isospectrality” J. Phys. G: Nucl. Part. Phys. 51 (2024) 055201

  42. [42]

    Mustafa, A.R

    O. Mustafa, A.R. Soares, C.F.S. Pereira, R.L.L. Vit´ oria, ” On the Klein–Gordon oscillators in Eddington-inspired Born- Infeld gravity global monopole spacetime and a W u–Yang magnetic monopole” Eur. Phys. J. C 84 (2024) 405

  43. [43]

    J. R. Nascimento, G. J. Olmo, A. Yu. Petrov, P. J. Porf ´ ırio, A. R. Soares, ” Global monopole in Palatini F (R) gravity” Phys. Rev. D 99 (2019) 064053

  44. [44]

    Aounallah, A

    H. Aounallah, A. R. Soares, R L L Vit´ oria, ”Scalar field and deflection of light under the effects of topologi- cally charged Ellis–Bronnikov-type wormhole spacetime ” Eur. Phys. J. C 80 (2020) 447

  45. [45]

    A. R. Soares, R L L Vit´ oria, H. Aounallah, ”On the Klein–Gord on oscillator in topologically charged Ellis–Bronnikov-typ e wormhole spacetime” Eur. Phys. J. Plus 136 (2021) 966

  46. [46]

    M¨ uller, ”Exact geometric optics in a Morris-Thorne worm hole spacetime” Phys

    T. M¨ uller, ”Exact geometric optics in a Morris-Thorne worm hole spacetime” Phys. Rev. D 77 (2008) 044043

  47. [47]

    Ahmed, ”Relativistic Quantum Effects on Scalar Bosons in Morris–Thorne-Type W ormhole Space-Time with a Cosmic Stri ng ” Few-Body syst

    F. Ahmed, ”Relativistic Quantum Effects on Scalar Bosons in Morris–Thorne-Type W ormhole Space-Time with a Cosmic Stri ng ” Few-Body syst. 64 (2023)80

  48. [48]

    F. dos S. Azevedo, J. D. M. de Lima, A. de P¯ adua, F. Moraes, ”Optical wormhole from hollow disclinations” Phys. Rev. A 103 (2017) 023516

  49. [49]

    Q. G. Garcia, P. J. Porf ´ ırio, D. C. Moreira, C. Fur- tado, ”Graphene wormhole trapped by external magnetic field ” Nucl. Phys. B 950 (2020)114853

  50. [50]

    G. J. Olmo, D. Rubiera-Garcia, ”The quantum, the geon and the crystal” Int. J. Mod. Phys. D. 24 (2015) 1542013

  51. [51]

    Dark Univ

    F Ahmed, A Bouzenada, ”Harmonic oscillator in topologicall y charged deformed gravity space–time and W u–Yang magnetic monopole” Phys. Dark Univ. 46 (2024) 101690

  52. [52]

    Fl¨ ugge, ”Practical Quantum mechanics”, Springer-Verlag, New York, Heidelberg Berlin 1974

    S. Fl¨ ugge, ”Practical Quantum mechanics”, Springer-Verlag, New York, Heidelberg Berlin 1974

  53. [53]

    M Moshinsky, A Szczepaniak, ”The Dirac oscillator” J. Phys. A: Math. Gen. 22 (1989) L817

  54. [54]

    B Mirza, M Mohadesi, ”The Klein-Gordon and the Dirac Oscillators in a Noncommutative Space” Commun. Theor. Phys. 42 (2004) 664

  55. [55]

    T T W u, C N Yang, ”Dirac monopole without strings: Monopole harmonics” Nucl. Phys. B 107 (1976) 365

  56. [56]

    T T W u, C N Yang, ”Concept of nonintegrable phase factors and global formulation of gauge fields” Phys. Rev. D 12 (1975) 3845

  57. [57]

    Ronveaux, Heun ’s Differential Equations (Oxford University Press, New York, 1995)

    A. Ronveaux, Heun ’s Differential Equations (Oxford University Press, New York, 1995)