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Large-Order Recurrence Asymptotics and Connection Amplitudes

Pincherle’s theorem identifies a line at infinity. Large-order asymptotics put a scale on that line, quantify its separation from the competing line, and provide useful terminal data for a backward sweep. Neither operation, by itself, fixes an absolute connection amplitude.

The central chain on this page is

ratio expansioncoefficient scaleminimal/dominant basisnormalized connection amplitudeODE endpoint coefficient.\begin{gathered} \text{ratio expansion}\\ \Downarrow\\ \text{coefficient scale}\\ \Downarrow\\ \text{minimal/dominant basis}\\ \Downarrow\\ \text{normalized connection amplitude}\\ \Downarrow\\ \text{ODE endpoint coefficient}. \end{gathered}

Every arrow has hypotheses. In particular, substituting a formal series into a recurrence is not an existence proof, and a coefficient amplitude is not automatically a physical wave amplitude.

Several mathematically different statements are often compressed into the phrase “the large-nn solution.” Keep them separate:

ClaimStatus and required evidence
A balance predicts a ratio scaleFormal Newton or dominant-balance calculation
Coefficient comparison produces a seriesFormal identity to the computed order
Exact solutions possess those expansionsAsymptotic-existence theorem with its hypotheses checked
A remainder is smaller than the last termRemainder theorem, not formal substitution alone
A finite-depth answer is stableNumerical observation over depth and precision
A coefficient is a physical amplitudeBasis normalization and a valid series-to-endpoint transfer

The Wong–Li theorems invoked below construct exact solutions for fixed recurrence parameters in the regular distinct-root and generic double-root cases. They do not automatically provide parameter-uniform analyticity near a root collision, a transition ray, or a finite singularity of the recurrence.

Ratios integrate into factorial and exponential scales

Section titled “Ratios integrate into factorial and exponential scales”

For the house recurrence

αnun+1+βnun+γnun1=0,\alpha_nu_{n+1} +\beta_nu_n +\gamma_nu_{n-1} =0,

write

Rn=unun1.R_n=\frac{u_n}{u_{n-1}}.

Then

un=u0k=1nRk.u_n=u_0\prod_{k=1}^{n}R_k.

This elementary product is the bridge from ratio asymptotics to sequence asymptotics. If, formally,

Rnλnη(1+j1djnj/p),R_n \sim \lambda n^\eta \left( 1+\sum_{j\geq1}d_jn^{-j/p_*} \right),

where pNp_*\in\mathbb N is the Puiseux denominator. Expand the logarithm as

log(1+j1djxj)=j1jxj.\log\left( 1+\sum_{j\geq1}d_jx^j \right) = \sum_{j\geq1}\ell_jx^j.

Euler–Maclaurin summation then gives the scale

unCλnΓ(n+1)η×exp[j=1p1j1j/pn1j/p]np(1+).\begin{aligned} u_n\sim{}& C\lambda^n\Gamma(n+1)^\eta\\ &\times \exp\left[ \sum_{j=1}^{p_*-1} \frac{\ell_j}{ 1-j/p_* } n^{1-j/p_*} \right] n^{\ell_{p_*}} \left(1+\cdots\right). \end{aligned}

This formula is best read as a dictionary:

  • λ\lambda produces an ordinary geometric factor λn\lambda^n;
  • nηn^\eta in the ratio produces Γ(n+1)η\Gamma(n+1)^\eta;
  • a ratio correction nδn^{-\delta} with 0<δ<10<\delta<1 produces a stretched exponential exp(cn1δ)\exp(cn^{1-\delta});
  • the n1n^{-1} term in the logarithm of the ratio produces an algebraic power of nn.

The last point prevents a common error. If

Rn±=r[1±κn1/2+c2n1+O(n3/2)],R_n^\pm = r\left[ 1\pm\kappa n^{-1/2} +c_2n^{-1} +O(n^{-3/2}) \right],

then

logRn±r=±κn1/2+(c2κ22)n1+O(n3/2),\log\frac{R_n^\pm}{r} = \pm\kappa n^{-1/2} +\left( c_2-\frac{\kappa^2}{2} \right)n^{-1} +O(n^{-3/2}),

and hence

un±C±rnexp(±2κn)nc2κ2/2[1+O(n1/2)].u_n^\pm \sim C_\pm r^n \exp\left(\pm2\kappa\sqrt n\right) n^{\,c_2-\kappa^2/2} \left[ 1+O(n^{-1/2}) \right].

The power is c2κ2/2c_2-\kappa^2/2, not c2c_2.

Exact asymptotic solutions for regular tails

Section titled “Exact asymptotic solutions for regular tails”

Put a regular tail into the standard form

w(n+2)+f(n)w(n+1)+g(n)w(n)=0,w(n+2)+f(n)w(n+1)+g(n)w(n)=0,

where

f(n)s0fsns,g(n)s0gsns,g00.\begin{aligned} f(n)&\sim\sum_{s\geq0}f_sn^{-s},\\ g(n)&\sim\sum_{s\geq0}g_sn^{-s}, & g_0&\neq0. \end{aligned}

The expansions here are Poincaré asymptotic expansions with the remainder conditions required by the theorem being invoked.

For the two cases used below, the operational checklist is:

  • hold the recurrence parameters fixed;
  • require ff and gg to possess the stated coefficient expansions with remainders through every order used;
  • require g00g_0\neq0 and an eventually nonsingular recurrence tail;
  • impose either two distinct characteristic roots, as in DLMF §2.9(i), or a double root with nonzero square-root splitting, as in DLMF §2.9(ii).

Wong and Li prove the existence statements behind those two DLMF cases. Checking this list at one parameter does not establish locally uniform control as the parameter varies.

Let r1,r2r_1,r_2 be the distinct roots of

P(r)=r2+f0r+g0.P(r)=r^2+f_0r+g_0.

Under the Wong–Li hypotheses, there are independent exact solutions

wj(n)rjnnαjs=0as,jns,a0,j=1,w_j(n) \sim r_j^n n^{\alpha_j} \sum_{s=0}^{\infty} \frac{a_{s,j}}{n^s}, \qquad a_{0,j}=1,

where

αj=f1rj+g1f0rj+2g0=f1rj+g1rjP(rj).\alpha_j = \frac{f_1r_j+g_1}{ f_0r_j+2g_0 } = -\frac{f_1r_j+g_1}{ r_jP'(r_j) }.

The preceding page used unequal root moduli to select a minimal branch. The refined form reveals another possibility. If r1=r2|r_1|=|r_2| but

Reα1<Reα2,\operatorname{Re}\alpha_1 < \operatorname{Re}\alpha_2,

then w1/w20w_1/w_2\to0 algebraically, so w1w_1 is still minimal. If both the root moduli and the real algebraic exponents agree, this level of asymptotics is inconclusive.

Now suppose

P(r)=(rr0)2,r00.P(r)=(r-r_0)^2, \qquad r_0\neq0.

Thus f0=2r0f_0=-2r_0 and g0=r02g_0=r_0^2. Define

κ2=f1r0+g1r02.\kappa^2 = -\frac{f_1r_0+g_1}{r_0^2}.

If κ0\kappa\neq0, the generic coincident-root theorem supplies exact solutions of the form

w±(n)r0nexp(±2κn)nαs=0cs(±)ns/2,w_\pm(n) \sim r_0^n \exp\left(\pm2\kappa\sqrt n\right) n^\alpha \sum_{s=0}^{\infty} c_s^{(\pm)}n^{-s/2},

with

c0(+)=c0()=1c_0^{(+)}=c_0^{(-)}=1

and

α=g0+2g14g0.\alpha = \frac{g_0+2g_1}{4g_0}.

Equivalently, the stretched-exponential coefficient used in DLMF §2.9 is 2κ2\kappa, and

(2κ)2=2f0f14g1g0.(2\kappa)^2 = \frac{2f_0f_1-4g_1}{g_0}.

Choose a square-root branch continuously on the parameter domain. If Reκ>0\operatorname{Re}\kappa>0, the minus solution is minimal and

w(n)w+(n)exp(4κn).\frac{w_-(n)}{w_+(n)} \sim \exp\left(-4\kappa\sqrt n\right).

If Reκ=0\operatorname{Re}\kappa=0, the two displayed envelopes have equal modulus on the positive-index ray; this leading expansion does not order them. If κ=0\kappa=0, the half-integer ansatz itself degenerates.

The repeated-root calculation in ratio form

Section titled “The repeated-root calculation in ratio form”

The practical calculation can be done without first guessing the full sequence. After multiplication of a recurrence row by a harmless common factor, suppose

αn=n2(1+A1n+A2n2+),βn=n2(2+B1n+B2n2+),γn=n2(1+C1n+C2n2+).\begin{aligned} \alpha_n &= n^2\left( 1+\frac{A_1}{n} +\frac{A_2}{n^2} +\cdots \right),\\ \beta_n &= n^2\left( -2+\frac{B_1}{n} +\frac{B_2}{n^2} +\cdots \right),\\ \gamma_n &= n^2\left( 1+\frac{C_1}{n} +\frac{C_2}{n^2} +\cdots \right). \end{aligned}

The limiting polynomial is (r1)2(r-1)^2. Dividing the nnth row by unu_n gives the exact Riccati equation

αnRn+1+βn+γnRn=0.\alpha_nR_{n+1} +\beta_n +\frac{\gamma_n}{R_n} =0.

Insert

Rn(ε)=1+εκn1/2+r1n1+O(n3/2),ε{+1,1}.R_n^{(\varepsilon)} = 1+\varepsilon\kappa n^{-1/2} +r_1n^{-1} +O(n^{-3/2}), \qquad \varepsilon\in\{+1,-1\}.

The first two nontrivial coefficient equations are

κ2+A1+B1+C1=0\kappa^2+A_1+B_1+C_1=0

and

2r1=κ2A1+C1+12.2r_1 = \kappa^2-A_1+C_1+\frac12.

Therefore

κ2=(A1+B1+C1),r1=12(κ2A1+C1+12),p=r1κ22=C1A12+14.\begin{aligned} \kappa^2 &= -\left(A_1+B_1+C_1\right),\\ r_1 &= \frac12\left( \kappa^2-A_1+C_1+\frac12 \right),\\ p &= r_1-\frac{\kappa^2}{2} = \frac{C_1-A_1}{2}+\frac14. \end{aligned}

The corresponding formal sequence scales are

un(ε)Cεexp(2εκn)np[1+O(n1/2)].u_n^{(\varepsilon)} \sim C_\varepsilon \exp\left( 2\varepsilon\kappa\sqrt n \right) n^p \left[ 1+O(n^{-1/2}) \right].

The nonzero constants CεC_\varepsilon are arbitrary normalizations; the ratio calculation cannot determine them.

This coefficient comparison is a convenient derivation engine. The existence theorem in the preceding section is what promotes the formal scales to asymptotic expansions of exact solutions.

Schwarzschild coefficients split on the square-root scale

Section titled “Schwarzschild coefficients split on the square-root scale”

Return to the Jaffé–Leaver recurrence derived earlier:

Anan+1+Bnan+Cnan1=0,\mathsf A_na_{n+1} +\mathsf B_na_n +\mathsf C_na_{n-1} =0,

where

An=(n+1)(n+2ϱ+1),\mathsf A_n=(n+1)(n+2\varrho+1), Bn=[2n2+(8ϱ+2)n+8ϱ2+4ϱ+(+1)σ],\begin{aligned} \mathsf B_n =-\bigl[ &2n^2+(8\varrho+2)n\\ &+8\varrho^2+4\varrho +\ell(\ell+1)-\sigma \bigr], \end{aligned}

and

Cn=(n+2ϱ)2s2.\mathsf C_n=(n+2\varrho)^2-s^2.

The physical specialization used here is

σ=s21.\sigma=s^2-1.

Dividing the three coefficients by n2n^2 gives

A1=2ϱ+2,B1=8ϱ2,C1=4ϱ.\begin{aligned} A_1&=2\varrho+2,\\ B_1&=-8\varrho-2,\\ C_1&=4\varrho. \end{aligned}

Consequently,

κ2=2ϱ,p=ϱ34.\kappa^2=2\varrho, \qquad p=\varrho-\frac34.

On a domain where ϱ0\varrho\neq0, choose

κ=2ϱ\kappa=\sqrt{2\varrho}

continuously. If Reκ>0\operatorname{Re}\kappa>0, the exact minimal and dominant tails may be normalized so that

mnnϱ3/4exp(2κn)[1+O(n1/2)],dnnϱ3/4exp(+2κn)[1+O(n1/2)].\begin{aligned} m_n &\sim n^{\varrho-3/4} \exp\left(-2\kappa\sqrt n\right) \left[ 1+O(n^{-1/2}) \right],\\ d_n &\sim n^{\varrho-3/4} \exp\left(+2\kappa\sqrt n\right) \left[ 1+O(n^{-1/2}) \right]. \end{aligned}

Thus

mndn=O(exp[4Re(κ)n]).\frac{m_n}{d_n} = O\left( \exp\left[-4\operatorname{Re}(\kappa)\sqrt n\right] \right).

This is the missing tail theorem behind the continued-fraction candidate on the preceding page.

Let

Rn=anan1,L=(+1).R_n=\frac{a_n}{a_{n-1}}, \qquad L=\ell(\ell+1).

Substitution into

AnRn+1Rn+BnRn+Cn=0\mathsf A_nR_{n+1}R_n +\mathsf B_nR_n +\mathsf C_n=0

gives

Rn(ε)=1+εκn1/2+(2ϱ34)n1+εc3n3/2+c4n2+O(n5/2),\begin{aligned} R_n^{(\varepsilon)} ={}& 1+\varepsilon\kappa n^{-1/2} +\left(2\varrho-\frac34\right)n^{-1}\\ &+\varepsilon c_3n^{-3/2} +c_4n^{-2} +O(n^{-5/2}), \end{aligned}

where

c3=64ϱ248ϱ+16L+332κc_3 = \frac{ 64\varrho^2-48\varrho+16L+3 }{ 32\kappa }

and

c4=64ϱ(Ls2)+48ϱ+16L+3128ϱ.c_4 = \frac{ 64\varrho(L-s^2)+48\varrho+16L+3 }{ 128\varrho }.

The spin cancels through c3c_3 and first appears in c4c_4. This cancellation uses σ=s21\sigma=s^2-1; it should not be imposed while deriving a recurrence for a different equation.

Taking logarithms and choosing unit leading normalization reproduces

an(ε)nϱ3/4exp(2εκn)[1+O(n1/2)].a_n^{(\varepsilon)} \sim n^{\varrho-3/4} \exp\left( 2\varepsilon\kappa\sqrt n \right) \left[ 1+O(n^{-1/2}) \right].

At ϱ=0\varrho=0, the displayed coefficients are nonuniform. The ratio then has an algebraic form Rn=1+χ/n+R_n=1+\chi/n+\cdots, with

χ2+χ+1L+σs2=0.\chi^2+\chi+1-L+\sigma-s^2=0.

For σ=s21\sigma=s^2-1, the indices are χ=\chi=\ell and χ=1\chi=-\ell-1. The square-root seed must not be used near this transition unless the depth is large compared with the nonuniform scale κ2|\kappa|^{-2}.

Minimal and dominant large-order recurrence branches, with a mixed solution crossing to the dominant envelope

Repeated-root splitting on the n\sqrt n scale. After removal of the common power npn^p, the minimal and dominant envelopes have slopes 2Reκ-2\operatorname{Re}\kappa and +2Reκ+2\operatorname{Re}\kappa. A mixture Cmm+CddC_mm+C_dd eventually follows the dominant line whenever Cd0C_d\neq0.

Ignoring lower-order corrections, the crossover occurs near

ncrosslogCm/Cd4Reκ,\sqrt{n_{\mathrm{cross}}} \approx \frac{ \log\lvert C_m/C_d\rvert }{ 4\operatorname{Re}\kappa },

when the right-hand side is positive. A tiny unwanted amplitude can therefore remain hidden for a long finite range.

For Reκ>0\operatorname{Re}\kappa>0, the minimal coefficients obey

n0njmn<\sum_{n\geq0}n^j\lvert m_n\rvert<\infty

for every fixed nonnegative integer jj. Hence the minimal Jaffé power series factor and every fixed termwise xx-derivative of that factor converge absolutely at x=1x=1. This does not imply analytic continuation through x=1x=1, nor does it bypass differentiation of the prefactor and x(r)x(r) when derivatives of the full ODE solution are needed.

Asymptotic tail seeds and cutoff separation

Section titled “Asymptotic tail seeds and cutoff separation”

A backward ratio sweep ending at row NN requires a terminal value for RN+1R_{N+1}. The zero tail

RN+1=0R_{N+1}=0

is valid as a projective cutoff but discards known large-order information. For the Schwarzschild minimal branch, a four-term asymptotic seed is

RN+1seed=1κN+1+2ϱ34N+1c3(N+1)3/2+c4(N+1)2.\begin{aligned} R_{N+1}^{\mathrm{seed}} ={}& 1-\frac{\kappa}{\sqrt{N+1}} +\frac{2\varrho-\frac34}{N+1}\\ &-\frac{c_3}{(N+1)^{3/2}} +\frac{c_4}{(N+1)^2}. \end{aligned}

The index N+1N+1 matters: Rn=an/an1R_n=a_n/a_{n-1}. A formula for an+1/ana_{n+1}/a_n is shifted by one row.

There is an exact way to see what a terminal seed controls. Let m,dm,d be an exact minimal–dominant basis and let a trial solution be

x=m+λd.x=m+\lambda d.

If its terminal ratio is

TN=xN+1xN,T_N=\frac{x_{N+1}}{x_N},

then

λ=mNdNRN+1mTNTNRN+1d.\lambda = \frac{m_N}{d_N} \frac{ R_{N+1}^{m}-T_N }{ T_N-R_{N+1}^{d} }.

For a zero tail this becomes

λ=mN+1dN+1=O(exp[4Re(κ)N]).\lambda = -\frac{m_{N+1}}{d_{N+1}} = O\left( \exp\left[-4\operatorname{Re}(\kappa)\sqrt N\right] \right).

An asymptotic seed makes the numerator RN+1mTNR_{N+1}^{m}-T_N smaller. Turning its formal omitted term into a rigorous head-error bound additionally requires a remainder estimate and control of the denominator. A small substituted Riccati defect alone is not such a bound.

At the algebraic test point

ϱ=14,=2,s=2,σ=3,\varrho=\frac14, \qquad \ell=2, \qquad s=2, \qquad \sigma=3,

the minimal ratio is

Rnmin=112n14n91232n3/2+14332n2+O(n5/2).\begin{aligned} R_n^{\min} ={}& 1-\frac{1}{\sqrt{2n}} -\frac{1}{4n} -\frac{91\sqrt2}{32n^{3/2}}\\ &+\frac{143}{32n^2} +O(n^{-5/2}). \end{aligned}

The reference uses 100-decimal-digit arithmetic, cutoff Nref=10000N_{\mathrm{ref}}=10\,000, and the displayed n2n^{-2} seed evaluated at R10001R_{10\,001}. The backward map is applied down to R1R_1. Doubling the cutoff to 2000020\,000 and raising the working precision to 150 digits leaves all digits quoted below unchanged:

R1min=0.1776779698080973454908003349989862.\begin{aligned} R_1^{\min} = -0.1776779698080973454908003349989862\ldots. \end{aligned}

Every finite-depth sweep in the following table was also performed at 100-digit working precision and compared with that same reference. The absolute errors in R1R_1 are:

NNZero tailSeed through n3/2n^{-3/2}Seed through n2n^{-2}
10101.4392×1061.4392\times10^{-6}1.9993×1071.9993\times10^{-7}4.9958×1084.9958\times10^{-8}
20201.3612×1081.3612\times10^{-8}6.7614×10106.7614\times10^{-10}1.6424×10101.6424\times10^{-10}
40403.2221×10113.2221\times10^{-11}5.5849×10135.5849\times10^{-13}1.2359×10131.2359\times10^{-13}
80801.0388×10141.0388\times10^{-14}6.1343×10176.1343\times10^{-17}1.1711×10171.1711\times10^{-17}

These are numerical observations, not certified bounds. They do, however, audit the indexing and signs: successive half-orders improve the same backward limit, while the zero tail converges on the predicted stretched-exponential scale. The reporting rule is conservative: retain only digits unchanged when both the cutoff is doubled and the working precision is increased.

The idea is often called a Nollert improvement in quasinormal-mode calculations. It is more general: any recurrence with a controlled large-order ratio expansion can use the expansion as terminal projective data.

Recurrence connection amplitudes from Casoratians

Section titled “Recurrence connection amplitudes from Casoratians”

Ratios are invariant under ucuu\mapsto cu, so they cannot determine an absolute amplitude. First normalize exact tail solutions by specified unit-leading asymptotic models:

mnmn1,dndn1.\frac{m_n}{\mathfrak m_n}\longrightarrow1, \qquad \frac{d_n}{\mathfrak d_n}\longrightarrow1.

To avoid collision with the angular index \ell, denote a left-normalized solution by uLu^{\mathrm L} and write

uL=Cmm+Cdd.u^{\mathrm L}=C_mm+C_dd.

With the chapter convention

Kn[u,v]=unvn+1un+1vn,\mathcal K_n[u,v] = u_nv_{n+1}-u_{n+1}v_n,

the exact coordinates are

Cm=Kn[uL,d]Kn[m,d],Cd=Kn[m,uL]Kn[m,d].\begin{aligned} C_m &= \frac{ \mathcal K_n[u^{\mathrm L},d] }{ \mathcal K_n[m,d] },\\ C_d &= \frac{ \mathcal K_n[m,u^{\mathrm L}] }{ \mathcal K_n[m,d] }. \end{aligned}

Both quotients are independent of nn: numerator and denominator obey the same discrete Abel scaling. Since mn/dn0m_n/d_n\to0,

Cd=limnunLdn=limnunLdn.C_d = \lim_{n\to\infty} \frac{u_n^{\mathrm L}}{d_n} = \lim_{n\to\infty} \frac{u_n^{\mathrm L}}{\mathfrak d_n}.

This limit is useful for measuring a dominant amplitude. It is a poor way to recover CmC_m from a generic mixture, because forward arithmetic erases the subdominant part.

The amplitude changes with the normalization of the objects it compares:

uLquL,dtdCmqCm,CdqtCd.u^{\mathrm L}\mapsto q\,u^{\mathrm L}, \qquad d\mapsto td \quad\Longrightarrow\quad \begin{aligned} C_m&\mapsto qC_m,\\ C_d&\mapsto\frac{q}{t}C_d. \end{aligned}

There is a subtler ambiguity. The replacement

dd+cmd\mapsto d+c\,m

does not change the complete dominant Poincaré expansion, because mm is beyond all algebraic orders relative to dd. It leaves CdC_d invariant but changes

CmCmcCd.C_m\mapsto C_m-cC_d.

Thus the unwanted dominant amplitude is canonical after the left and dominant leading normalizations are fixed. A full pair of exact connection coefficients needs an additional analytic prescription for the dominant complement.

The continued-fraction residual and the unwanted amplitude

Section titled “The continued-fraction residual and the unwanted amplitude”

Normalize the left solution by

u0L=1,u1L=β0α0,u_0^{\mathrm L}=1, \qquad u_1^{\mathrm L}=-\frac{\beta_0}{\alpha_0},

and let mm be the exact minimal solution. The Leaver residual is

F0=β0+α0m1m0.F_0 = \beta_0+\alpha_0\frac{m_1}{m_0}.

At the first row,

K0[m,uL]=m0u1Lm1u0L=m0α0F0.\mathcal K_0[m,u^{\mathrm L}] = m_0u_1^{\mathrm L}-m_1u_0^{\mathrm L} = -\frac{m_0}{\alpha_0}F_0.

Therefore the dominant recurrence amplitude is

Cd=m0α0K0[m,d]F0.C_d = -\frac{m_0}{ \alpha_0\mathcal K_0[m,d] } F_0.

The residual and CdC_d have the same zeros wherever the displayed prefactor is finite and nonzero, but they are not the same normalized function. At a ratio-chart pole, use homogeneous pairs and Casoratians rather than this affine formula.

If the series-to-ODE map is denoted by S\mathscr S and the endpoint ODE basis is unit-normalized as

S[m]=νmyadm,S[d]=νdybad,\mathscr S[m]=\nu_m y_{\mathrm{adm}}, \qquad \mathscr S[d]=\nu_d y_{\mathrm{bad}},

then

S[uL]=νmCmyadm+νdCdybad.\mathscr S[u^{\mathrm L}] = \nu_mC_m y_{\mathrm{adm}} +\nu_dC_d y_{\mathrm{bad}}.

The physical bad-endpoint coefficient is νdCd\nu_dC_d, not automatically CdC_d and not automatically F0F_0.

Darboux transfer for algebraic endpoint amplitudes

Section titled “Darboux transfer for algebraic endpoint amplitudes”

Coefficient tails can encode endpoint connection coefficients directly. Assume in this subsection that

μ{0,1,2,}.\mu\notin\{0,-1,-2,\ldots\}.

The excluded values are polynomial or limiting cases and do not obey the coefficient-limit formula below without separate treatment. The exact binomial identity

(1x)μ=n=0Γ(n+μ)Γ(μ)Γ(n+1)xn(1-x)^{-\mu} = \sum_{n=0}^{\infty} \frac{ \Gamma(n+\mu) }{ \Gamma(\mu)\Gamma(n+1) } x^n

implies

[xn](1x)μnμ1Γ(μ).[x^n](1-x)^{-\mu} \sim \frac{n^{\mu-1}}{\Gamma(\mu)}.

More generally, suppose FF has the required continuation to a Δ\Delta-domain at x=1x=1, no competing boundary singularity contributes at the same scale, and

F(x)A(1x)μ.F(x) \sim A(1-x)^{-\mu}.

Then the transfer theorem gives

[xn]F(x)AΓ(μ)nμ1,[x^n]F(x) \sim \frac{A}{\Gamma(\mu)}n^{\mu-1},

so

A=Γ(μ)limnn1μ[xn]F(x).A = \Gamma(\mu) \lim_{n\to\infty} n^{1-\mu}[x^n]F(x).

This direction is a theorem under the stated analyticity hypotheses. The converse is not automatic: the same coefficient asymptotics need not, by itself, prove a unique local singular expansion.

Let

F(x)=2F1(a,b;c;x)=n=0unxn,F(x)={}_2F_1(a,b;c;x) = \sum_{n=0}^{\infty}u_nx^n,

with

un=(a)n(b)n(c)nn!.u_n = \frac{(a)_n(b)_n}{(c)_n\,n!}.

Put μ=a+bc\mu=a+b-c and assume

cZ0,a,bZ0,μZ.\begin{gathered} c\notin\mathbb Z_{\leq0}, \qquad a,b\notin\mathbb Z_{\leq0},\\ \mu\notin\mathbb Z. \end{gathered}

These conditions exclude denominator poles, terminating numerator series, and the resonant connection cases. Gamma-ratio asymptotics give

unΓ(c)Γ(a)Γ(b)nμ1.u_n \sim \frac{\Gamma(c)}{ \Gamma(a)\Gamma(b) } n^{\mu-1}.

The unit-leading singular solution at x=1x=1 begins with (1x)μ(1-x)^{-\mu}, and its exact connection coefficient is

B=Γ(c)Γ(μ)Γ(a)Γ(b).B = \frac{ \Gamma(c)\Gamma(\mu) }{ \Gamma(a)\Gamma(b) }.

Darboux transfer recovers the same entry:

B=Γ(μ)limnn1μun.B = \Gamma(\mu) \lim_{n\to\infty} n^{1-\mu}u_n.

For

a=12,b=23,c=1,a=\frac12, \qquad b=\frac23, \qquad c=1,

one has μ=1/6\mu=1/6 and

B=Γ(1/6)πΓ(2/3)2.3191905339278567.B = \frac{ \Gamma(1/6) }{ \sqrt\pi\,\Gamma(2/3) } \approx 2.3191905339278567.

This independently checks the power, the gamma factor, and the unit-leading endpoint normalization against the connection matrix derived in Chapter 2.

For the exact test function

F(x)=75(1x)3/2=n=0anxn,F(x) = \frac75(1-x)^{-3/2} = \sum_{n=0}^{\infty}a_nx^n,

define

A^n=Γ(3/2)ann1/2.\widehat A_n = \Gamma(3/2)a_n n^{-1/2}.

Then A^n7/5\widehat A_n\to7/5. Since

A^n=75(1+38n+O(n2)),\widehat A_n = \frac75 \left( 1+\frac{3}{8n} +O(n^{-2}) \right),

division by 1+3/(8n)1+3/(8n) removes the first correction:

nnRaw A^n\widehat A_nFirst-correction estimate
551.50203911881.50203911881.39724569191.3972456919
10101.45174690541.45174690541.39927412571.3992741257
50501.41046947381.41046947381.39996970111.3999697011
2002001.40262308751.40262308751.39999809111.3999980911

An extrapolated coefficient is still conditional on the assumed transfer model. Several singularities on the same convergence circle contribute a sum of asymptotic terms and must be separated before applying this one-singularity estimator.

For the Jaffé representation used earlier,

ψ(r)=(r1)ϱr2ϱexp[ϱ(r1)]×n=0an(r1r)n.\begin{aligned} \psi(r) ={}& (r-1)^\varrho r^{-2\varrho} \exp[-\varrho(r-1)]\\ &\times \sum_{n=0}^{\infty} a_n \left( \frac{r-1}{r} \right)^n. \end{aligned}

Put

x=r1r,S(x)=n=0anxn.x=\frac{r-1}{r}, \qquad S(x)=\sum_{n=0}^{\infty}a_nx^n.

At a spectral parameter satisfying F0=0F_0=0, the left-normalized coefficient sequence is minimal. If Reκ>0\operatorname{Re}\kappa>0, then

S(1)=n=0anS(1)=\sum_{n=0}^{\infty}a_n

converges absolutely. Relative to the unit remote behavior

rϱexp(ϱr),r^{-\varrho}\exp(-\varrho r),

the endpoint amplitude is

Aadm=exp(ϱ)S(1).A_{\mathrm{adm}} = \exp(\varrho)S(1).

The factor exp(ϱ)\exp(\varrho) comes from the prefactor; omitting it is a normalization error.

The minimal tail also estimates the endpoint-sum remainder. If

anCmnϱ3/4exp(2κn),a_n \sim C_mn^{\varrho-3/4} \exp(-2\kappa\sqrt n),

then, in a sector where the integral comparison is valid,

n>NanCmκNϱ1/4exp(2κN).\sum_{n>N}a_n \sim \frac{C_m}{\kappa} N^{\varrho-1/4} \exp(-2\kappa\sqrt N).

This provides a useful tail correction after CmC_m has been fitted or computed by a Casoratian.

The unwanted dominant tail has a different transfer mechanism. For a generic left sequence with

anCdnϱ3/4exp(+2κn),a_n \sim C_dn^{\varrho-3/4} \exp(+2\kappa\sqrt n),

put x=exp(τ)x=\exp(-\tau). Assume τ0\tau\to0 with Reτ>0\operatorname{Re}\tau>0, so x<1|x|<1, in a fixed sector for which

argκτ<π4ϵ\left| \arg\frac{\kappa}{\sqrt\tau} \right| < \frac{\pi}{4}-\epsilon

with some ϵ>0\epsilon>0. For positive real τ\tau, this is argκ<π/4ϵ|\arg\kappa|<\pi/4-\epsilon. In this sector the interior saddle is accessible and dominant. Replacing the tail sum by its continuum model and setting n=t2n=t^2 gives

S(exp[τ])2Cd0t2ϱ1/2×exp(2κtτt2) ⁣dt.\begin{aligned} S(\exp[-\tau]) \sim 2C_d\int_0^\infty &t^{2\varrho-1/2}\\ &\times \exp(2\kappa t-\tau t^2)\,\dd t. \end{aligned}

The phase has saddle t=κ/τt_*=\kappa/\tau. Completing the square supplies exp(κ2/τ)=exp(2ϱ/τ)\exp(\kappa^2/\tau)=\exp(2\varrho/\tau), while the Gaussian width contributes π/τ\sqrt{\pi/\tau}. Combining the remaining powers gives, in the corresponding validity sector,

S(x)2πCdκ2ϱ1/2×τ2ϱexp(2ϱτ).\begin{aligned} S(x) \sim{}& 2\sqrt\pi\,C_d \kappa^{\,2\varrho-1/2}\\ &\times \tau^{-2\varrho} \exp\left(\frac{2\varrho}{\tau}\right). \end{aligned}

Since τ1=r12+O(r1)\tau^{-1}=r-\tfrac12+O(r^{-1}), multiplication by the Jaffé prefactor produces the opposite remote wave rϱexp(ϱr)r^\varrho\exp(\varrho r) with coefficient

Bopp=2πCdκ2ϱ1/2.B_{\mathrm{opp}} = 2\sqrt\pi\,C_d \kappa^{\,2\varrho-1/2}.

Thus the dominant coefficient-tail amplitude is proportional to the unwanted physical connection amplitude, with a calculable normalization. The power of κ\kappa uses the branch induced by its declared continuous choice. Outside the stated saddle sector, analytic continuation and Stokes control are required; the coefficient tail alone does not justify retaining an exponentially subdominant saddle contribution. At a quasinormal-mode zero, Cd=0C_d=0; the minimal sum instead yields AadmA_{\mathrm{adm}}.

A numerical workflow that preserves the mathematics

Section titled “A numerical workflow that preserves the mathematics”
  1. Record the original recurrence, row scaling, exceptional indices, parameter point, and square-root branch.
  2. Derive the ratio expansion in the original indexing and substitute it back to record its formal defect order.
  3. Check the hypotheses of an asymptotic-existence theorem before calling the formal branches exact minimal and dominant solutions.
  4. Evaluate the minimal seed at the actual terminal ratio index N+1N+1.
  5. Sweep backward with homogeneous pairs and rescale them, switching ratio charts near poles.
  6. Compare zero-tail and successive asymptotic seeds over several depths and precisions. Treat agreement as evidence unless an error theorem supplies constants.
  7. Measure zeros with the homogeneous Casoratian or residual; measure an absolute amplitude only after fixing both basis normalizations.
  8. Translate the recurrence amplitude to an ODE amplitude with the representation factor, then audit it against direct ODE matching or an exact special-function benchmark.

Near Reκ=0\operatorname{Re}\kappa=0 or κ=0\kappa=0, fixed-parameter tail asymptotics are nonuniform. Increasing precision cannot compensate for a depth that is too short to resolve the branch separation.

Promoting a formal balance to a theorem. Coefficient comparison proves that a series formally cancels the recurrence. An asymptotic-existence theorem is what supplies exact solutions having that series.

Changing the square-root branch point by point. The labels “plus” and “minus” are meaningful only after 2ϱ\sqrt{2\varrho} is continued on a declared parameter domain. Crossing a branch cut can exchange the two labels.

Using a repeated-root seed at its transition. The half-power expansion is singular at ϱ=0\varrho=0 and loses separation when Re2ϱ=0\operatorname{Re}\sqrt{2\varrho}=0. Recompute the relevant algebraic or transition asymptotics.

Inferring an absolute amplitude from ratios. Ratios determine a projective line. A connection amplitude additionally requires normalizations for the left solution and the endpoint basis.

Calling the residual the physical coefficient. F0F_0, CdC_d, and the ODE bad-endpoint coefficient have the same generic zeros but differ by normalization factors.

Extracting a subdominant coefficient by forward subtraction. Once the dominant branch overwhelms a floating-point sequence, subtracting it leaves mostly roundoff. Use a Casoratian, backward propagation, or a matched basis.

Treating a tail seed as an error certificate. A higher-order seed often accelerates convergence dramatically. Certification still requires a remainder bound, denominator control, and a valid depth range.

Applying one-singularity Darboux transfer blindly. Competing singularities on the convergence circle, logarithmic resonance, or a missing continuation domain change the coefficient asymptotics.

Suppose

Rn=r(1+κn1/2+cn1+O(n3/2)).R_n = r\left( 1+\kappa n^{-1/2} +cn^{-1} +O(n^{-3/2}) \right).

Derive the leading asymptotic form of unu_n.

Solution

Take logarithms:

logRn=logr+κn1/2+(cκ22)n1+O(n3/2).\log R_n = \log r +\kappa n^{-1/2} +\left(c-\frac{\kappa^2}{2}\right)n^{-1} +O(n^{-3/2}).

Use

k=1nk1/2=2n+O(1),k=1nk1=logn+O(1).\sum_{k=1}^{n}k^{-1/2} = 2\sqrt n+O(1), \qquad \sum_{k=1}^{n}k^{-1} = \log n+O(1).

The summable remainder changes only the constant and lower corrections, so

unCrnexp(2κn)ncκ2/2.u_n \sim Cr^n \exp(2\kappa\sqrt n) n^{c-\kappa^2/2}.

For the normalized coefficients A1,B1,C1A_1,B_1,C_1 on this page, substitute the half-power ratio ansatz and recover κ2\kappa^2, r1r_1, and pp.

Solution

Expand

Rn+1=1+εκn1/2+r1n1+ε(r2κ2)n3/2+O(n2).\begin{aligned} R_{n+1} ={}& 1+\varepsilon\kappa n^{-1/2} +r_1n^{-1}\\ &+\varepsilon \left( r_2-\frac{\kappa}{2} \right)n^{-3/2} +O(n^{-2}). \end{aligned}

and

1Rn=1εκn1/2+(κ2r1)n1+ε(r2+2κr1κ3)n3/2+O(n2).\begin{aligned} \frac1{R_n} ={}& 1-\varepsilon\kappa n^{-1/2} +(\kappa^2-r_1)n^{-1}\\ &+\varepsilon \left( -r_2+2\kappa r_1-\kappa^3 \right)n^{-3/2} +O(n^{-2}). \end{aligned}

Here εr2\varepsilon r_2 denotes the unneeded next coefficient in the ratio ansatz. In

αnRn+1+βn+γnRn=0,\alpha_nR_{n+1} +\beta_n +\frac{\gamma_n}{R_n} =0,

the n1n^{-1} coefficient gives

κ2+A1+B1+C1=0.\kappa^2+A_1+B_1+C_1=0.

The r2r_2 terms cancel from the n3/2n^{-3/2} coefficient, which gives

2r1=κ2A1+C1+12.2r_1 = \kappa^2-A_1+C_1+\frac12.

Finally p=r1κ2/2p=r_1-\kappa^2/2, because the logarithm of the ratio contains r1κ2/2r_1-\kappa^2/2 at order n1n^{-1}.

Use the displayed Schwarzschild coefficients to prove

κ2=2ϱ,p=ϱ34.\kappa^2=2\varrho, \qquad p=\varrho-\frac34.

At ϱ=1/4\varrho=1/4, show that the minimal series and all of its fixed termwise xx-derivatives converge absolutely at x=1x=1.

Solution

The normalized first coefficients are

A1=2ϱ+2,B1=8ϱ2,C1=4ϱ.A_1=2\varrho+2, \quad B_1=-8\varrho-2, \quad C_1=4\varrho.

Therefore

κ2=(A1+B1+C1)=2ϱ\kappa^2 = -(A_1+B_1+C_1) = 2\varrho

and

p=C1A12+14=ϱ34.p = \frac{C_1-A_1}{2}+\frac14 = \varrho-\frac34.

At ϱ=1/4\varrho=1/4, choose κ=1/2\kappa=1/\sqrt2. Then

mnn1/2exp(2n).m_n \sim n^{-1/2}\exp(-\sqrt{2n}).

For every fixed jj, njmnn^j|m_n| is summable. This follows, for example, from the integral test after t=nt=\sqrt n, because a polynomial in tt is integrable against exp(2t)\exp(-\sqrt2\,t).

4. Prove the terminal-contamination identity

Section titled “4. Prove the terminal-contamination identity”

Let x=m+λdx=m+\lambda d and TN=xN+1/xNT_N=x_{N+1}/x_N. Derive the exact formula for λ\lambda and specialize it to the zero tail.

Solution

Cross-multiplication gives

TN(mN+λdN)=mN+1+λdN+1.T_N(m_N+\lambda d_N) = m_{N+1}+\lambda d_{N+1}.

Solving,

λ=mN+1TNmNTNdNdN+1=mNdNRN+1mTNTNRN+1d.\lambda = \frac{ m_{N+1}-T_Nm_N }{ T_Nd_N-d_{N+1} } = \frac{m_N}{d_N} \frac{ R_{N+1}^m-T_N }{ T_N-R_{N+1}^d }.

At TN=0T_N=0,

λ=mN+1dN+1.\lambda=-\frac{m_{N+1}}{d_{N+1}}.

For the stretched-exponential pair this has magnitude O(exp[4Re(κ)N])O(\exp[-4\operatorname{Re}(\kappa)\sqrt N]).

Starting from uL=Cmm+Cddu^{\mathrm L}=C_mm+C_dd, prove both Casoratian formulas. Determine how the coefficients change under uLquLu^{\mathrm L}\mapsto q\,u^{\mathrm L}, dtdd\mapsto td, and dd+cmd\mapsto d+c\,m.

Solution

Bilinearity and antisymmetry give

K[uL,d]=CmK[m,d],K[m,uL]=CdK[m,d].\mathcal K[u^{\mathrm L},d] = C_m\mathcal K[m,d], \qquad \mathcal K[m,u^{\mathrm L}] = C_d\mathcal K[m,d].

Division gives the two formulas. Scaling uLu^{\mathrm L} by qq scales both coefficients by qq; scaling dd by tt sends CdC_d to Cd/tC_d/t and leaves CmC_m unchanged. If d=d+cmd'=d+c\,m, then

uL=(CmcCd)m+Cdd,u^{\mathrm L} = (C_m-cC_d)m+C_dd',

so CdC_d is invariant and CmC_m becomes CmcCdC_m-cC_d.

6. Recover a hypergeometric connection coefficient

Section titled “6. Recover a hypergeometric connection coefficient”

Use gamma-ratio asymptotics on

un=(a)n(b)n(c)nn!u_n=\frac{(a)_n(b)_n}{(c)_n\,n!}

and Darboux transfer to recover the coefficient of the unit-leading (1x)cab(1-x)^{c-a-b} solution at x=1x=1.

Solution

Writing each Pochhammer symbol as a gamma quotient gives

un=Γ(c)Γ(a)Γ(b)Γ(n+a)Γ(n+b)Γ(n+c)Γ(n+1).u_n = \frac{\Gamma(c)}{\Gamma(a)\Gamma(b)} \frac{ \Gamma(n+a)\Gamma(n+b) }{ \Gamma(n+c)\Gamma(n+1) }.

Gamma-ratio asymptotics yield

unΓ(c)Γ(a)Γ(b)na+bc1.u_n \sim \frac{\Gamma(c)}{\Gamma(a)\Gamma(b)} n^{a+b-c-1}.

With μ=a+bc\mu=a+b-c, Darboux transfer multiplies the leading coefficient by Γ(μ)\Gamma(\mu). Therefore

B=Γ(c)Γ(a+bc)Γ(a)Γ(b),B = \frac{ \Gamma(c)\Gamma(a+b-c) }{ \Gamma(a)\Gamma(b) },

which is the standard hypergeometric connection coefficient.

Suppose

unL=Cmmn+Cddnu_n^{\mathrm L}=C_mm_n+C_dd_n

with the repeated-root scales on this page. Estimate when the two contributions have equal magnitude.

Solution

The common power of nn cancels. Equating the two leading envelopes gives

Cmexp(2Reκn)Cdexp(+2Reκn).|C_m|\exp(-2\operatorname{Re}\kappa\sqrt n) \approx |C_d|\exp(+2\operatorname{Re}\kappa\sqrt n).

Hence

4ReκnlogCm/Cd,4\operatorname{Re}\kappa\sqrt n \approx \log|C_m/C_d|,

which yields the displayed estimate for ncrossn_{\mathrm{cross}}. If Cd=0C_d=0, there is no crossover.

Let ENE_N be the zero-tail error in the finite-depth benchmark. Form the consecutive empirical slopes

s(N1,N2)=logEN2logEN1N2N1.s(N_1,N_2) = \frac{ \log E_{N_2}-\log E_{N_1} }{ \sqrt{N_2}-\sqrt{N_1} }.

Compare them with the predicted asymptotic slope at ϱ=1/4\varrho=1/4.

Solution

Here κ=1/2\kappa=1/\sqrt2, so

logEN=constant4κN+o(N)\log E_N = \text{constant} -4\kappa\sqrt N +o(\sqrt N)

predicts the limiting slope

4κ=222.82843.-4\kappa=-2\sqrt2\approx-2.82843.

The table gives

Pair (N1,N2)(N_1,N_2)Empirical slope
(10,20)(10,20)3.5583-3.5583
(20,40)(20,40)3.2639-3.2639
(40,80)(40,80)3.0689-3.0689

The sequence moves toward 22-2\sqrt2. The remaining drift is expected from algebraic prefactors and lower asymptotic terms. This fit supports the predicted scale; it is not a proof of a uniform error bound.

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