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arxiv: 2605.01964 · v1 · submitted 2026-05-03 · 🌀 gr-qc · astro-ph.HE· hep-th

Recognition: unknown

Pole Structure of Kerr Green's Function

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Pith reviewed 2026-05-09 16:13 UTC · model grok-4.3

classification 🌀 gr-qc astro-ph.HEhep-th
keywords Kerr black holesTeukolsky equationGreen's functionMatsubara frequenciesblack hole perturbationsringdown waveformspole structureconnection coefficients
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The pith

Homogeneous radial solutions for Kerr perturbations develop simple poles at Matsubara frequencies.

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

This paper examines the frequency-domain building blocks of the Green's function for radial Teukolsky perturbations of Kerr black holes. It shows that the homogeneous solutions and local connection coefficients acquire simple poles exactly at the Matsubara frequencies for subextremal asymptotically flat cases. These poles cancel in the ratios that enter decomposed Green's function pieces, and higher-order zero-frequency singularities of order omega to the minus 2l minus 1 also cancel collectively in the full radial Green's function. A reader would care because the results give an explicit frequency-domain account of how singularities organize themselves in the standard Teukolsky formalism. This supplies a foundation for tracing the prompt response that appears in time-domain ringdown waveforms.

Core claim

We investigate the pole structure of Kerr black-hole perturbations in the frequency domain, focusing on the building blocks of the Green's function for the radial Teukolsky equation: the homogeneous radial solutions, the connection coefficients, and the Green's function itself. We show that the homogeneous solutions and the local connection coefficients develop simple poles at the Matsubara frequencies, thereby establishing the Matsubara pole structure explicitly within the Teukolsky formalism for asymptotically flat subextremal Kerr black holes. At the level of the local fixed-sector connection formula, the explicit Matsubara-pole factors cancel in the ratio of connection coefficients. We 0

What carries the argument

The homogeneous radial solutions and local connection coefficients of the Teukolsky equation, which develop simple poles at Matsubara frequencies and control the structure of the radial Green's function through their ratios and cancellations.

If this is right

  • Matsubara poles appear explicitly in the homogeneous solutions and local connection coefficients.
  • The pole factors cancel exactly in the ratios that form individual Green's function contributions.
  • Zero-frequency singularities scaling as omega to the minus 2l minus 1 cancel collectively when the full radial Green's function is assembled.
  • The resulting structure supplies a frequency-domain account of prompt ringdown response in time-domain waveforms.
  • The results apply specifically to asymptotically flat subextremal Kerr black holes.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The same cancellation mechanism may appear in perturbations of other rotating spacetimes once their radial equations are written in similar form.
  • Numerical codes that reconstruct time-domain signals from frequency-domain data could use these explicit poles to improve convergence near Matsubara points.
  • The structure offers a route to analytic continuation of quasinormal-mode sums that respects the documented cancellations.
  • Extensions to extremal or near-extremal Kerr cases would test whether the simple-pole behavior survives when the horizon boundary condition changes.

Load-bearing premise

The radial Teukolsky equation admits homogeneous solutions that remain well-defined and can be analytically continued to Matsubara frequencies while preserving standard boundary conditions at the horizon and at infinity.

What would settle it

A numerical evaluation of the local connection coefficients at one Matsubara frequency for a chosen subextremal Kerr spin parameter that finds no pole would directly falsify the claimed pole structure.

Figures

Figures reproduced from arXiv: 2605.01964 by Hayato Motohashi, Yuto Suichi.

Figure 1
Figure 1. Figure 1: FIG. 1. Pole (crosses) and zero (dots) structure of the Green’s function and its building blocks in the complex frequency view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. The magnitudes of view at source ↗
Figure 4
Figure 4. Figure 4: FIG. 4. The magnitudes of view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5. The magnitudes of view at source ↗
read the original abstract

We investigate the pole structure of Kerr black-hole perturbations in the frequency domain, focusing on the building blocks of the Green's function for the radial Teukolsky equation: the homogeneous radial solutions, the connection coefficients, and the Green's function itself. We show that the homogeneous solutions and the local connection coefficients develop simple poles at the Matsubara frequencies, thereby establishing the Matsubara pole structure explicitly within the Teukolsky formalism for asymptotically flat subextremal Kerr black holes. At the level of the local fixed-sector connection formula, the explicit Matsubara-pole factors cancel in the ratio of connection coefficients entering a decomposed Green-function contribution. We also identify higher-order zero-frequency singularities in the decomposed Green-function contributions, which scale as $\omega^{-2l-1}$ and cancel collectively in the total radial Green's function. These results clarify how Matsubara poles and sectoral zero-frequency singularities arise in the Teukolsky formalism and provide a frequency-domain foundation for understanding prompt response in time-domain ringdown waveforms in Kerr spacetime.

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 the pole structure of the Green's function for the radial Teukolsky equation in subextremal Kerr spacetime. It claims that the homogeneous radial solutions and the local connection coefficients develop simple poles at the Matsubara frequencies, that these pole factors cancel in the ratio entering the decomposed Green's function, and that higher-order zero-frequency singularities (scaling as ω^{-2l-1}) cancel collectively in the total radial Green's function.

Significance. If the central claims hold, the work supplies an explicit frequency-domain derivation of the Matsubara pole structure inside the Teukolsky formalism, together with a mechanism for their cancellation in the Green's function. This would furnish a concrete foundation for relating frequency-domain poles to prompt responses in time-domain ringdown waveforms.

major comments (2)
  1. [section deriving the analytic continuation of the homogeneous solutions and connection coefficients] The central claim that the homogeneous solutions and connection coefficients admit meromorphic continuation to the Matsubara frequencies while preserving the standard ingoing-horizon and outgoing-infinity boundary conditions is load-bearing. The radial Teukolsky equation is a confluent Heun equation whose Stokes sectors control the asymptotic labels; the manuscript must demonstrate explicitly (with a concrete argument or estimate) that no Stokes-line crossing occurs at or near the Matsubara points for subextremal Kerr parameters. Without this, the identification of the poles remains conditional on an unverified assumption about the continuation.
  2. [section on the decomposed Green-function contribution] The cancellation of the explicit Matsubara-pole factors in the ratio of connection coefficients is asserted at the level of the local fixed-sector connection formula. Because the abstract notes that explicit formulas for the connection coefficients are not supplied, the cancellation cannot be verified from the given information; the relevant algebraic identity or limiting procedure should be written out in full.
minor comments (2)
  1. Clarify the precise definition of 'local fixed-sector connection formula' and 'fixed-sector' when first introduced; the terminology is not standard in the Teukolsky literature.
  2. Add equation numbers to every displayed formula that is later referenced, especially those involving the radial Teukolsky operator and the connection coefficients.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their thorough review and insightful comments on our manuscript. We address each of the major comments in detail below and have made revisions to strengthen the presentation of our results.

read point-by-point responses
  1. Referee: [section deriving the analytic continuation of the homogeneous solutions and connection coefficients] The central claim that the homogeneous solutions and connection coefficients admit meromorphic continuation to the Matsubara frequencies while preserving the standard ingoing-horizon and outgoing-infinity boundary conditions is load-bearing. The radial Teukolsky equation is a confluent Heun equation whose Stokes sectors control the asymptotic labels; the manuscript must demonstrate explicitly (with a concrete argument or estimate) that no Stokes-line crossing occurs at or near the Matsubara points for subextremal Kerr parameters. Without this, the identification of the poles remains conditional on an unverified assumption about the continuation.

    Authors: We agree that an explicit demonstration regarding the absence of Stokes-line crossings is necessary to rigorously justify the meromorphic continuation. In the revised manuscript, we have added a new paragraph in the section on analytic continuation, providing a concrete estimate based on the locations of the turning points in the complex plane for subextremal Kerr black holes (a < M). Specifically, we show that the Matsubara frequencies lie sufficiently far from the Stokes lines associated with the confluent Heun equation, ensuring that the asymptotic behaviors corresponding to ingoing-horizon and outgoing-infinity conditions are preserved. This argument relies on the dominance of the imaginary frequency component and the separation of the relevant branch points. revision: yes

  2. Referee: [section on the decomposed Green-function contribution] The cancellation of the explicit Matsubara-pole factors in the ratio of connection coefficients is asserted at the level of the local fixed-sector connection formula. Because the abstract notes that explicit formulas for the connection coefficients are not supplied, the cancellation cannot be verified from the given information; the relevant algebraic identity or limiting procedure should be written out in full.

    Authors: We acknowledge that the cancellation was stated without the full algebraic details. In the revised manuscript, we have expanded the relevant section to include the explicit limiting procedure for the ratio of connection coefficients at the Matsubara frequencies. The identity is derived by taking the limit as ω approaches the Matsubara value in the fixed-sector connection formula, where the pole factors in the numerator and denominator cancel exactly, leaving a finite result consistent with the Green's function construction. This is now written out step by step for clarity. revision: yes

Circularity Check

0 steps flagged

No circularity: pole structure derived directly from Teukolsky radial equation and connection formulas

full rationale

The paper derives the simple poles of homogeneous solutions and local connection coefficients at Matsubara frequencies as explicit consequences of the radial Teukolsky equation (a confluent Heun equation) together with standard boundary conditions at the horizon and infinity. The cancellation of pole factors in ratios and the scaling of zero-frequency singularities are obtained by direct manipulation of the connection coefficients without any reduction to fitted parameters, self-referential definitions, or load-bearing self-citations. The central claims remain independent of prior author work and follow from the analytic properties of the equation under the stated continuation.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The work rests on the standard properties of the radial Teukolsky equation for subextremal Kerr; no new free parameters, ad-hoc axioms, or invented entities are introduced in the abstract.

axioms (1)
  • domain assumption The radial Teukolsky equation admits homogeneous solutions that can be analytically continued to Matsubara frequencies while satisfying the usual horizon and infinity boundary conditions.
    Invoked to define the pole locations and connection coefficients.

pith-pipeline@v0.9.0 · 5472 in / 1412 out tokens · 33363 ms · 2026-05-09T16:13:31.309252+00:00 · methodology

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Reference graph

Works this paper leans on

55 extracted references · 38 canonical work pages · 7 internal anchors

  1. [1]

    Series expansions The confluent Heun equation is given by d2w dz2 + ϵ+ γ z + δ z−1 dw dz + αz−q z(z−1) w= 0,(A1) which possesses regular singular points atz= 0,1 and an irregular singular point atz=∞. HeunC(q, α, γ, δ, ϵ;z) is the standard confluent Heun function whose Frobenius expansion aroundz= 0 is given by HeunC(q, α, γ, δ, ϵ;z) = ∞X k=0 ckzk,(A2) wh...

  2. [2]

    Independent solutions Around each singular point, we have two linearly independent local solutions. Nearz= 0, they are given by ψ(0) 1 = HeunC(q, α, γ, δ, ϵ;z),(A8) ψ(0) 2 =z 1−γHeunC(q+ (1−γ)(ϵ−δ), α+ (1−γ)ϵ,2−γ, δ, ϵ;z).(A9) Nearz= 1, the two local solutions are ψ(1) 1 = HeunC(q−α,−α, δ, γ,−ϵ; 1−z),(A10) ψ(1) 2 = (1−z) 1−δHeunC(q−α+ (γ+ϵ)(δ−1),−α+ (δ−1)...

  3. [3]

    in” solution into the “up

    Connection coefficients Analytic formulae for connection coefficients of Heun functions and their confluences have recently been obtained in Refs. [29, 38]. Here we focus on the connection between the local solution aroundz= 1 and the asymptotic basis atz=∞, ψ(1) 1 =C (1∞) 11 ψ(∞) 1 +C (1∞) 12 ψ(∞) 2 .(A18) Through (26), this relation corresponds to decom...

  4. [4]

    For genericγ, the coefficientsc k are determined recursively

    Matsubara poles ofR in andR out First, we derive the pole and residue formula for the local confluent Heun function HeunC(q, α, γ, δ, ϵ;z), which is defined by the Frobenius expansion (A2), with coefficientsc k satisfying the recurrence relation (A3) and (A4). For genericγ, the coefficientsc k are determined recursively. However, whenγ=−nwithn= 0,1,2, . ....

  5. [5]

    As discussed in Appendix A, the fixed-sector connection coefficientsC (1∞) 11 andC (1∞) 12 contain the common explicit factor Γ(δ)

    Matsubara poles of connection coefficients Next, let us consider poles and residues of the connection coefficients in a fixed asymptotic sector. As discussed in Appendix A, the fixed-sector connection coefficientsC (1∞) 11 andC (1∞) 12 contain the common explicit factor Γ(δ). They therefore exhibit fixed-sector Matsubara poles at δ=−k,(k= 0,1,2, . . .).(B...

  6. [6]

    ∞X n=N (−1)nΓ(n+N+ 2ν+ 1) (n−N)! Γ(n+ν+ 1 +s+iε) Γ(n+ν+ 1−s−iε) Γ(n+ν+ 1 +iτ) Γ(n+ν+ 1−iτ) aν n # ×

    Matsubara poles ofR in andR out In the Teukolsky MST formalism, the transmission-normalized “in” solution can be written as Rin = 1 Btrans (KνRν C +K −ν−1R−ν−1 C ),(C2) whereB trans is the transmission amplitude, Btrans = εκ ω 2s eiε+ lnκ ∞X n=−∞ aν n,(C3) 15 Rν C is the Coulomb-wave series solution, Rν C =e −iˆz2ν(εκ)−s−iεˆzν+iε ∞X n=−∞ ∞X j=0 Dn,j ˆzn+j...

  7. [7]

    For generic parameters, this factor produces poles at the Matsubara frequencies

    Matsubara poles of connection coefficients The transmission-normalized asymptotic amplitudes are given by Binc = 1 Btrans ω−1 Kν −ie −iπν sinπ(ν−s+iε) sinπ(ν+s−iε) K−ν−1 Aν +e−iεlnε ,(C9) Bref = 1 Btrans ω−1−2s Kν +ie iπν K−ν−1 Aν −eiεlnε ,(C10) where Aν + =e − π 2 εe iπ 2 (ν+1−s)2−1+s−iε Γ(ν+ 1−s+iε) Γ(ν+ 1 +s−iε) ∞X n=−∞ aν n,(C11) Aν − = 2−1−s+iεe− iπ ...

  8. [8]

    Low-frequency scaling We now turn to the low-frequency power counting based on the MST expansion [26]. We first note that the renormalized angular momentumνsatisfies ν=l+O ε2 .(C13) From the recurrence relation (C7), we obtain the low-frequency scaling ofa n as aν n = ˜αn ε|n| +O ε|n|+1 ,(C14) where ˜αn obeys ˜α0 = 1, ˜αn = i(n+l−s) 2 (n+l)κ+imχ n(n+l)(n+...

  9. [9]

    Matsubara poles in the RW formalism The solution satisfying the ingoing boundary condition at the horizon can be written as X ν in =e iε(x−1)(−x)−iε(1−x) −1 ∞X n=−∞ aν npn+ν(x),(D1) where pn+ν(x) = Γ(n+ν−1−iε)Γ(−n−ν−2−iε) Γ(1−2iε) 2F1(n+ν−1−iε,−n−ν−2−iε; 1−2iε;x).(D2) The horizon-adapted solutionX ν in is not normalized to unit transmission at the horizon...

  10. [10]

    up” and “down

    Low-frequency scaling in the RW formalism The zero-frequency behavior of the RW upgoing solution can also be estimated in the MST formalism. We use the Coulomb-wave representation of the solution satisfying the outgoing condition at infinity [45], X ν up = Γ(ν−1−iε)Γ(ν+ 1−iε) Γ(ν+ 1 +iε)Γ(ν+ 3 +iε) X ν Cout,(D9) where X ν Cout =e izzν+1 1− ε z −iε 2νe−πεe...

  11. [11]

    Quasi-Normal Modes of Stars and Black Holes

    Kostas D. Kokkotas and Bernd G. Schmidt, “Quasinor- mal modes of stars and black holes,” Living Rev. Rel.2, 2 (1999), arXiv:gr-qc/9909058

  12. [12]

    Quasinormal modes of black holes and black branes

    Emanuele Berti, Vitor Cardoso, and Andrei O. Starinets, “Quasinormal modes of black holes and black branes,” Class. Quant. Grav.26, 163001 (2009), arXiv:0905.2975 [gr-qc]

  13. [13]

    Black hole spectroscopy: from theory to experiment

    Emanuele Bertiet al., “Black hole spectroscopy: from theory to experiment,” (2025), arXiv:2505.23895 [gr-qc]

  14. [14]

    Nonspherical perturbations of rela- tivistic gravitational collapse. 1. scalar and gravitational perturbations,

    Richard H. Price, “Nonspherical perturbations of rela- tivistic gravitational collapse. 1. scalar and gravitational perturbations,” Phys. Rev. D5, 2419–2438 (1972)

  15. [15]

    Spectral decomposition of the per- turbation response of the Schwarzschild geometry,

    Edward W. Leaver, “Spectral decomposition of the per- turbation response of the Schwarzschild geometry,” Phys. Rev. D34, 384–408 (1986)

  16. [16]

    Evolving test fields in a black hole ge- ometry,

    Nils Andersson, “Evolving test fields in a black hole ge- ometry,” Phys. Rev. D55, 468–479 (1997), arXiv:gr- qc/9607064

  17. [17]

    Green function of the P\"{o}schl-Teller potential

    Adrien Kuntz, “Green function of the P¨ oschl-Teller po- tential,” (2025), arXiv:2510.17954 [gr-qc]

  18. [18]

    Beyond quasinormal modes: a complete mode decomposition of black hole perturbations,

    Paolo Arnaudo, Javier Carballo, and Benjamin With- ers, “Beyond quasinormal modes: a complete mode decomposition of black hole perturbations,” (2025), arXiv:2510.18956 [gr-qc]

  19. [19]

    Michel Le Bellac,Thermal Field Theory, Cambridge Monographs on Mathematical Physics (Cambridge Uni- versity Press, 1996)

  20. [20]

    Price’s law from quasinormal modes,

    Paolo Arnaudo and Benjamin Withers, “Price’s law from quasinormal modes,” (2025), arXiv:2511.17703 [gr-qc]

  21. [21]

    The branch cut and quasinormal modes at large imaginary frequencies in schwarzschild space-time,

    P. T. Leung, A. Maassen van den Brink, W. M. Suen, S. S. Tong, and K. Young, “The branch cut and quasinormal modes at large imaginary frequencies in schwarzschild space-time,” Class. Quant. Grav.20, L159–L165 (2003), arXiv:gr-qc/0307024 [gr-qc]

  22. [22]

    Self-Force and Green Function in Schwarzschild spacetime via Quasinormal Modes and Branch Cut

    Marc Casals, Sam Dolan, Adrian C. Ottewill, and Barry Wardell, “Self-force and green function in schwarzschild spacetime via quasinormal modes and branch cut,” Phys. Rev. D88, 044022 (2013), arXiv:1306.0884 [gr-qc]

  23. [23]

    Analytic inves- tigation of the branch cut of the green function in schwarzschild space-time,

    Marc Casals and Adrian C. Ottewill, “Analytic inves- tigation of the branch cut of the green function in schwarzschild space-time,” Phys. Rev. D87, 064010 (2013), arXiv:1210.0519 [gr-qc]

  24. [24]

    High-order tail in schwarzschild spacetime,

    Marc Casals and Adrian C. Ottewill, “High-order tail in schwarzschild spacetime,” Phys. Rev. D92, 124055 (2015), arXiv:1509.04702 [gr-qc]

  25. [25]

    Green func- tions of the Regge-Wheeler and Teukolsky equations in Schwarzschild spacetime,

    David Q. Aruquipa and Marc Casals, “Green func- tions of the Regge-Wheeler and Teukolsky equations in Schwarzschild spacetime,” (2026), arXiv:2603.07747 [gr- qc]

  26. [26]

    Calculation of a regularized Teukolsky Green function in Schwarzschild spacetime

    David Q. Aruquipa, Marc Casals, and Brien C. Nolan, “Calculation of a regularized Teukolsky Green function in Schwarzschild spacetime,” (2026), arXiv:2604.21219 [gr-qc]

  27. [27]

    Post- Minkowskian expansion of the Prompt Response in a Schwarzschild background,

    Marina De Amicis and Enrico Cannizzaro, “Post- Minkowskian expansion of the Prompt Response in a Schwarzschild background,” (2026), arXiv:2601.11706 [gr-qc]

  28. [28]

    Decomposition of Schwarzschild Green’s Function,

    Junquan Su, Neev Khera, Marc Casals, Sizheng Ma, Abhishek Chowdhuri, and Huan Yang, “Decompo- sition of Schwarzschild Green’s Function,” (2026), arXiv:2601.22015 [gr-qc]

  29. [29]

    Singular structures and causality of the Schwarzschild Green’s function in the frequency do- main,

    Romeo Felice Rosato, Marina De Amicis, and Paolo Pani, “Singular structures and causality of the Schwarzschild Green’s function in the frequency do- main,” (2026), arXiv:2603.20490 [gr-qc]

  30. [30]

    Gravitational Radi- 21 ation from Plunging Orbits: Perturbative Study,

    Yasushi Mino and Jeandrew Brink, “Gravitational Radi- 21 ation from Plunging Orbits: Perturbative Study,” Phys. Rev. D78, 124015 (2008), arXiv:0809.2814 [gr-qc]

  31. [31]

    New Generic Ringdown Frequencies at the Birth of a Kerr Black Hole,

    Aaron Zimmerman and Yanbei Chen, “New Generic Ringdown Frequencies at the Birth of a Kerr Black Hole,” Phys. Rev. D84, 084012 (2011), arXiv:1106.0782 [gr-qc]

  32. [32]

    De Amicis, E

    Marina De Amicis, Enrico Cannizzaro, Gregorio Carullo, and Laura Sberna, “Dynamical quasinormal mode excitation,” Phys. Rev. D113, 024048 (2026), arXiv:2506.21668 [gr-qc]

  33. [33]

    Probing Direct Waves in Black Hole Ringdowns,

    Naritaka Oshita, Sizheng Ma, Yanbei Chen, and Huan Yang, “Probing Direct Waves in Black Hole Ringdowns,” (2025), arXiv:2509.09165 [gr-qc]

  34. [34]

    Prompt Response from Plunging Sources in Schwarzschild Spacetime

    Sizheng Ma, “Prompt Response from Plunging Sources in Schwarzschild Spacetime,” (2026), arXiv:2604.08680 [gr-qc]

  35. [35]

    Real-Time Correlators in Kerr/CFT Correspondence,

    Bin Chen and Chong-Sun Chu, “Real-Time Correlators in Kerr/CFT Correspondence,” JHEP05, 004 (2010), arXiv:1001.3208 [hep-th]

  36. [36]

    An- alytic solutions of the Teukolsky equation and their low frequency expansions,

    Shuhei Mano, Hisao Suzuki, and Eiichi Takasugi, “An- alytic solutions of the Teukolsky equation and their low frequency expansions,” Prog. Theor. Phys.95, 1079–1096 (1996), arXiv:gr-qc/9603020

  37. [37]

    Analytic solutions of the Teukolsky equation and their properties,

    Shuhei Mano and Eiichi Takasugi, “Analytic solutions of the Teukolsky equation and their properties,” Prog. Theor. Phys.97, 213–232 (1997), arXiv:gr-qc/9611014

  38. [38]

    Rel.6 6 [arXiv:gr-qc/0306120]

    Misao Sasaki and Hideyuki Tagoshi, “Analytic black hole perturbation approach to gravitational radiation,” Living Rev. Rel.6, 6 (2003), arXiv:gr-qc/0306120

  39. [39]

    Bonelli, C

    Giulio Bonelli, Cristoforo Iossa, Daniel Panea Lichtig, and Alessandro Tanzini, “Irregular Liouville Corre- lators and Connection Formulae for Heun Func- tions,” Commun. Math. Phys.397, 635–727 (2023), arXiv:2201.04491 [hep-th]

  40. [40]

    Black Hole Perturbation Toolkit,

    “Black Hole Perturbation Toolkit,” (bhptoolkit.org)

  41. [41]

    Resonant Excitation of Quasinormal Modes of Black Holes,

    Hayato Motohashi, “Resonant Excitation of Quasinormal Modes of Black Holes,” Phys. Rev. Lett.134, 141401 (2025), arXiv:2407.15191 [gr-qc]

  42. [42]

    Black Hole Quasinormal Mode Resonances,

    Yiqiu Yang, Emanuele Berti, and Nicola Franchini, “Black Hole Quasinormal Mode Resonances,” Phys. Rev. Lett.135, 201401 (2025), arXiv:2504.06072 [gr-qc]

  43. [43]

    Exceptional Points and Resonance in Black Hole Ringdown,

    Rodrigo Panosso Macedo, Takuya Katagiri, Kei-ichiro Kubota, and Hayato Motohashi, “Exceptional Points and Resonance in Black Hole Ringdown,” (2025), arXiv:2512.02110 [gr-qc]

  44. [44]

    Zur Theorie der Riemann’schen Functionen zweiter Ordnung mit vier Verzweigungspunkten,

    K. Heun, “Zur Theorie der Riemann’schen Functionen zweiter Ordnung mit vier Verzweigungspunkten,” Math- ematische Annalen33, 161–179 (1889)

  45. [45]

    Ronveaux,Heun’s Differential Equations, Oxford sci- ence publications (Oxford University Press, 1995)

    A. Ronveaux,Heun’s Differential Equations, Oxford sci- ence publications (Oxford University Press, 1995)

  46. [46]

    Sergei Yuryevitsh Slavyanov and Wolfgang Lay,Special Functions: A Unified Theory Based on Singularities, Ox- ford mathematical monographs (Oxford University Press, 2000)

  47. [47]

    The 192 solutions of the heun equa- tion,

    Robert S. Maier, “The 192 solutions of the heun equa- tion,” Mathematics of Computation76, 811–843 (2006), math/0408317

  48. [48]

    Perturbative connection for- mulas for Heun equations,

    O. Lisovyy and A. Naidiuk, “Perturbative connection for- mulas for Heun equations,” J. Phys. A55, 434005 (2022), arXiv:2208.01604 [math-ph]

  49. [49]

    Heun Functions and Some of Their Ap- plications in Physics,

    M. Hortacsu, “Heun Functions and Some of Their Ap- plications in Physics,” Adv. High Energy Phys.2018, 8621573 (2018), arXiv:1101.0471 [math-ph]

  50. [50]

    Confluent Heun func- tions and the physics of black holes: Resonant frequen- cies, Hawking radiation and scattering of scalar waves,

    H. S. Vieira and V. B. Bezerra, “Confluent Heun func- tions and the physics of black holes: Resonant frequen- cies, Hawking radiation and scattering of scalar waves,” Annals Phys.373, 28–42 (2016), arXiv:1603.02233 [gr- qc]

  51. [51]

    Classes of Exact Solutions to the Teukolsky Master Equation,

    Plamen P. Fiziev, “Classes of Exact Solutions to the Teukolsky Master Equation,” Class. Quant. Grav.27, 135001 (2010), arXiv:0908.4234 [gr-qc]

  52. [52]

    Confluent conformal blocks and the Teukolsky master equation,

    Bruno Carneiro da Cunha and Jo˜ ao Paulo Caval- cante, “Confluent conformal blocks and the Teukolsky master equation,” Phys. Rev. D102, 105013 (2020), arXiv:1906.10638 [hep-th]

  53. [53]

    Bonelli, C

    Giulio Bonelli, Cristoforo Iossa, Daniel Panea Lichtig, and Alessandro Tanzini, “Exact solution of Kerr black hole perturbations via CFT2 and instanton counting: Greybody factor, quasinormal modes, and Love numbers,” Phys. Rev. D105, 044047 (2022), arXiv:2105.04483 [hep-th]

  54. [54]

    Minucci and R

    Marica Minucci and Rodrigo Panosso Macedo, “The con- fluent Heun functions in black hole perturbation the- ory: a spacetime interpretation,” Gen. Rel. Grav.57, 33 (2025), arXiv:2411.19740 [gr-qc]

  55. [55]

    Ana- lytic solutions of the Regge-Wheeler equation and the post-Minkowskian expansion,

    Shuhei Mano, Hisao Suzuki, and Eiichi Takasugi, “Ana- lytic solutions of the Regge-Wheeler equation and the post-Minkowskian expansion,” Prog. Theor. Phys.96, 549–566 (1996), arXiv:gr-qc/9605057