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Quartic versus Hyperbolic Double Wells

The quartic well and the Razavy well look alike on the real axis: below the barrier, each has two allowed islands separated by an open forbidden path. That resemblance is useful only after the coordinate, barrier height, kinetic scale, and energy have been matched.

Once both minima are placed at X=±1X=\pm1 and both barriers have height one, the comparison becomes exact:

vR(X;a)vQ(X),vR(X;a)vQ(X)(a0).\begin{aligned} v_{\mathrm R}(X;a) &\ge v_{\mathrm Q}(X), \\ v_{\mathrm R}(X;a) &\longrightarrow v_{\mathrm Q}(X) \quad (a\to0). \end{aligned}

At a common normalized kinetic scale η\eta, the first statement orders the indexed eigenvalues. The second gives a controlled local quartic limit of the hyperbolic well, not uniform convergence on R\mathbb R. Neither statement makes the global ODEs identical: polynomial infinity and the two irregular ends of a DCHE problem retain different Stokes and connection data.

One barrier-normalized passport makes comparison meaningful

Section titled “One barrier-normalized passport makes comparison meaningful”

Use the common spectral problem

L[v,η]ψ=(η2 ⁣d2 ⁣dX2+v(X))ψ=εψ.\mathscr L[v,\eta]\psi = \left( -\eta^2\frac{\dd^2}{\dd X^2} +v(X) \right)\psi = \varepsilon\psi.

Here the minima are at X=±1X=\pm1, the central barrier is v(0)=1v(0)=1, and η\eta measures kinetic energy relative to the chosen separation and barrier.

For the quartic convention of Page 3, set

X=2q1.X=2q-1.

Multiplying its eigenvalue equation by 32g32g gives

[(8g)2 ⁣d2 ⁣dX2+(1X2)2]ψ=32gEQψ.\left[ -(8g)^2\frac{\dd^2}{\dd X^2} +(1-X^2)^2 \right]\psi = 32gE_{\mathrm Q}\psi.

For Razavy, write

a=12arcosh ⁣(Mζ),C=cosh2a=Mζ,X=xa,a = \frac12\operatorname{arcosh}\!\left(\frac M\zeta\right), \qquad C=\cosh2a=\frac M\zeta, \qquad X=\frac xa,

in the double-well chamber M>ζM>\zeta. Division by the barrier (Mζ)2(M-\zeta)^2 gives

[1a2(Mζ)2 ⁣d2 ⁣dX2+vR(X;a)]ψ=ER(Mζ)2ψ,\left[ -\frac{1}{a^2(M-\zeta)^2} \frac{\dd^2}{\dd X^2} +v_{\mathrm R}(X;a) \right]\psi = \frac{E_{\mathrm R}}{(M-\zeta)^2}\psi,

where

vR(X;a)=[cosh2acosh(2aX)cosh2a1]2.v_{\mathrm R}(X;a) = \left[ \frac{\cosh2a-\cosh(2aX)} {\cosh2a-1} \right]^2.

The dictionary is therefore

DatumQuarticRazavy
ShapevQ=(1X2)2v_{\mathrm Q}=(1-X^2)^2vR(X;a)v_{\mathrm R}(X;a)
Kinetic scaleηQ=8g\eta_{\mathrm Q}=8gηR=[a(Mζ)]1\eta_{\mathrm R}=[a(M-\zeta)]^{-1}
EnergyεQ=32gEQ\varepsilon_{\mathrm Q}=32gE_{\mathrm Q}εR=ER/(Mζ)2\varepsilon_{\mathrm R}=E_{\mathrm R}/(M-\zeta)^2
Shape parameternonea=12arcosh(M/ζ)a=\tfrac12\operatorname{arcosh}(M/\zeta)

Raw energies or raw barrier actions from the two pages should not be placed in one ratio. A matched comparison means the same η\eta in the normalized operators. Choosing ηQ=ηR\eta_{\mathrm Q}=\eta_{\mathrm R} is a comparison protocol, not a universal identity between gg and (ζ,M)(\zeta,M).

The normalized hyperbolic shape lies above the quartic

Section titled “The normalized hyperbolic shape lies above the quartic”

The ordering follows from the power series of cosh\cosh. Put u=X2u=X^2. For 0u10\le u\le1,

cosh(2aX)1=k1(2a)2kuk(2k)!u(cosh2a1),\cosh(2aX)-1 = \sum_{k\ge1} \frac{(2a)^{2k}u^k}{(2k)!} \le u\bigl(\cosh2a-1\bigr),

whereas the inequality reverses for u1u\ge1. In both ranges,

cosh(2aX)cosh2acosh2a1X21.\frac{ \left|\cosh(2aX)-\cosh2a\right| }{ \cosh2a-1 } \ge \left|X^2-1\right|.

Squaring proves

vR(X;a)vQ(X)(XR, a>0).v_{\mathrm R}(X;a)\ge v_{\mathrm Q}(X) \qquad (X\in\mathbb R,\ a>0).

Equality holds at the barrier and minima, X=0,±1X=0,\pm1, but is strict elsewhere. Thus barrier- and separation-matched hyperbolic wells are everywhere no lower than the quartic well.

Their local curvatures sharpen the picture:

X=0X=±1vQ48vR4a2sinh2a8a2coth2a\begin{array}{c|cc} &X=0&X=\pm1\\ \hline v_{\mathrm Q}'' &-4&8\\ v_{\mathrm R}'' &-\dfrac{4a^2}{\sinh^2a} &8a^2\coth^2a \end{array}

For a>0a>0, the normalized hyperbolic barrier is flatter at its top and its minima are steeper. Between the three matching points its barrier sits higher.

On every fixed compact set,

vR(X;a)=(1X2)2[1+2a2X23+O(a4)].v_{\mathrm R}(X;a) = (1-X^2)^2 \left[ 1+\frac{2a^2X^2}{3}+O(a^4) \right].

The bracketed form means

vR=vQ+2a23X2(1X2)2+O(a4).v_{\mathrm R} = v_{\mathrm Q} +\frac{2a^2}{3}X^2(1-X^2)^2 +O(a^4).

Barrier-normalized quartic and Razavy wells beside their bottom forbidden actions.

Left: after matching minima and barrier height, the Razavy shapes lie at or above the quartic shape and approach it as a0a\to0. Right: the dimensionless bottom action starts at AQ=4/3\mathcal A_{\mathrm Q}=4/3 and approaches 22 as the hyperbolic well becomes increasingly steep away from its minima.

Expert checkpoint: spectral ordering and convergence

At fixed η\eta, form ordering and the min–max principle give

εnR(a,η)>εnQ(η),n=0,1,.\varepsilon_n^{\mathrm R}(a,\eta) > \varepsilon_n^{\mathrm Q}(\eta), \qquad n=0,1,\ldots.

For strictness, put W=vRvQW=v_{\mathrm R}-v_{\mathrm Q} and WK=min(W,K)W_K=\min(W,K) with any K>0K>0. The bounded function WKW_K is positive almost everywhere. Along

Ht=HQ+tWK,0t1,H_t=H_{\mathrm Q}+tW_K, \qquad 0\le t\le1,

one-dimensional bound-state eigenvalues are simple, so the Hellmann–Feynman identity gives

 ⁣dEn(t) ⁣dt=RWK(X)ψn,t(X)2 ⁣dX>0.\frac{\dd E_n(t)}{\dd t} = \int_{\mathbb R} W_K(X)\lvert\psi_{n,t}(X)\rvert^2\,\dd X >0.

Since HRHQ+WKH_{\mathrm R}\ge H_{\mathrm Q}+W_K, a second use of min–max proves the displayed strict inequality for every nn.

The pointwise limit is not uniform on the whole line: polynomial and exponential tails never become the same at fixed aa. Nevertheless, for each fixed nn and η>0\eta>0,

lima0+εnR(a,η)=εnQ(η).\lim_{a\to0^+} \varepsilon_n^{\mathrm R}(a,\eta) = \varepsilon_n^{\mathrm Q}(\eta).

The lower bound is the form ordering. For the upper bound, smoothly cut off the first n+1n+1 quartic eigenfunctions outside a large compact interval and use uniform convergence of vRv_{\mathrm R} on that interval in the min–max trial space. The cutoff error is made small before a0a\to0 is taken.

Four real turning points share one separatrix skeleton

Section titled “Four real turning points share one separatrix skeleton”

Let 0<ε<10<\varepsilon<1. For the quartic shape,

XinQ=1ε,XoutQ=1+ε.X_{\mathrm{in}}^{\mathrm Q} = \sqrt{1-\sqrt\varepsilon}, \qquad X_{\mathrm{out}}^{\mathrm Q} = \sqrt{1+\sqrt\varepsilon}.

For the hyperbolic shape,

XinR=12aarcosh ⁣[C(C1)ε],XoutR=12aarcosh ⁣[C+(C1)ε].\begin{aligned} X_{\mathrm{in}}^{\mathrm R} &= \frac{1}{2a} \operatorname{arcosh}\!\left[ C-(C-1)\sqrt\varepsilon \right], \\ X_{\mathrm{out}}^{\mathrm R} &= \frac{1}{2a} \operatorname{arcosh}\!\left[ C+(C-1)\sqrt\varepsilon \right]. \end{aligned}

In either model the ordered real roots are

Xout,Xin,Xin,Xout.-X_{\mathrm{out}}, \quad -X_{\mathrm{in}}, \quad X_{\mathrm{in}}, \quad X_{\mathrm{out}}.

The outer pairs bound two equal allowed intervals; the inner pair bounds the forbidden barrier. At ε=1\varepsilon=1, the inner roots collide at X=0X=0. Above the barrier, only the outer pair remains real. Expanding the hyperbolic formulas at small aa recovers the quartic formulas.

Four roots alone do not guarantee a narrow doublet. Near a minimum, the local harmonic energies measured in units of the barrier are

dQ,N=2(2N+1)η,dR,N=2acotha(2N+1)η.\begin{aligned} d_{\mathrm Q,N} &= 2(2N+1)\eta, \\ d_{\mathrm R,N} &= 2a\coth a\,(2N+1)\eta. \end{aligned}

The diagnostic dN1d_N\ll1 places a fixed local level well below the separatrix. It is not an error bound. When dNd_N approaches one, the inner turning points coalesce and a uniform Weber (parabolic-cylinder) barrier-top analysis replaces a dilute-instanton expansion.

Equal barriers do not mean equal tunnelling actions

Section titled “Equal barriers do not mean equal tunnelling actions”

For a barrier-normalized shape define the open bottom action

A[v]=11v(X) ⁣dX.\mathcal A[v] = \int_{-1}^{1}\sqrt{v(X)}\,\dd X.

The quartic value is

AQ=11(1X2) ⁣dX=43.\mathcal A_{\mathrm Q} = \int_{-1}^{1}(1-X^2)\,\dd X = \frac43.

For Razavy,

AR(a)=1C111[Ccosh(2aX)] ⁣dX=2cosh2asinh(2a)/acosh2a1.\begin{aligned} \mathcal A_{\mathrm R}(a) &= \frac{1}{C-1} \int_{-1}^{1} \left[C-\cosh(2aX)\right]\dd X \\ &= \frac{ 2\cosh2a-\sinh(2a)/a }{ \cosh2a-1 }. \end{aligned}

The shape inequality gives

AR(a)>43(a>0),\mathcal A_{\mathrm R}(a)>\frac43 \qquad (a>0),

and direct expansion yields

AR(a)=43+4a245+O(a4),a0,AR(a)=21a+O(e2a),a.\begin{aligned} \mathcal A_{\mathrm R}(a) &= \frac43+\frac{4a^2}{45}+O(a^4), \qquad a\to0, \\ \mathcal A_{\mathrm R}(a) &= 2-\frac1a+O(\ee^{-2a}), \qquad a\to\infty. \end{aligned}

The normalized exponents reproduce the raw actions on the two earlier pages:

AQηQ=16g,ARηR=Marcosh ⁣(Mζ)M2ζ2.\frac{\mathcal A_{\mathrm Q}}{\eta_{\mathrm Q}} = \frac{1}{6g}, \qquad \frac{\mathcal A_{\mathrm R}}{\eta_{\mathrm R}} = M\operatorname{arcosh}\!\left(\frac M\zeta\right) -\sqrt{M^2-\zeta^2}.

The Razavy expression has two useful physical limits. With Δ=Mζ\Delta=M-\zeta,

SR223Δ3/2ζ,Δ0,S_{\mathrm R} \sim \frac{2\sqrt2}{3} \frac{\Delta^{3/2}}{\sqrt\zeta}, \qquad \Delta\downarrow0,

whereas

SR=M[log ⁣(2Mζ)1]+ζ24M+O ⁣(ζ4M3),Mζ.\begin{aligned} S_{\mathrm R} ={}& M\left[ \log\!\left(\frac{2M}{\zeta}\right)-1 \right] \\ &+ \frac{\zeta^2}{4M} +O\!\left(\frac{\zeta^4}{M^3}\right), \qquad \frac M\zeta\to\infty. \end{aligned}

For model j{Q,R}\mathrm j\in\{\mathrm Q,\mathrm R\}, define the positive odd–even gap of the NNth doublet by

ΔεNj=εodd,Njεeven,Nj>0.\Delta\varepsilon_N^{\mathrm j} = \varepsilon_{\mathrm{odd},N}^{\mathrm j} - \varepsilon_{\mathrm{even},N}^{\mathrm j} >0.

At matched η\eta, fixed NN, and fixed a>0a>0, the leading comparison is

logΔεNRΔεNQ=AR(a)AQη+o ⁣(η1),η0+.\log \frac{\Delta\varepsilon_N^{\mathrm R}} {\Delta\varepsilon_N^{\mathrm Q}} = -\frac{ \mathcal A_{\mathrm R}(a)-\mathcal A_{\mathrm Q} }{\eta} +o\!\left(\eta^{-1}\right), \qquad \eta\to0^+.

This orders the leading exponential scales, not the exact finite-η\eta splittings. Form ordering of individual eigenvalues does not order a difference of two eigenvalues. The quartic determinant prefactor and loop coefficients from Page 3 cannot be transplanted to Razavy.

A coalescing-well limit produces the quartic operator

Section titled “A coalescing-well limit produces the quartic operator”

The local limit becomes transparent if

λ=a(Mζ)=ηR1\lambda = a(M-\zeta) = \eta_{\mathrm R}^{-1}

is held fixed. Since M=ζcosh2aM=\zeta\cosh2a, this means

ζ=λa(cosh2a1),M=λcosh2aa(cosh2a1).\zeta = \frac{\lambda}{a(\cosh2a-1)}, \qquad M = \frac{\lambda\cosh2a} {a(\cosh2a-1)}.

Then

a2HR= ⁣d2 ⁣dX2+λ2vR(X;a),a^2H_{\mathrm R} = -\frac{\dd^2}{\dd X^2} +\lambda^2v_{\mathrm R}(X;a),

so that

a2HR ⁣d2 ⁣dX2+λ2(1X2)2(a0+)a^2H_{\mathrm R} \longrightarrow -\frac{\dd^2}{\dd X^2} +\lambda^2(1-X^2)^2 \qquad (a\to0^+)

on every fixed XX-window. The Page 3 quartic has

λ=18g.\lambda=\frac{1}{8g}.

The action limit is automatic:

SR=λAR(a)4λ3=16g.S_{\mathrm R} = \lambda\mathcal A_{\mathrm R}(a) \longrightarrow \frac{4\lambda}{3} = \frac{1}{6g}.

This is a singular double scaling. Indeed,

ζλ2a3,Mλ2a3.\zeta\sim\frac{\lambda}{2a^3}, \qquad M\sim\frac{\lambda}{2a^3}.

Taking MζM\downarrow\zeta at fixed ζ\zeta instead collapses the barrier and sends ηR\eta_{\mathrm R} to infinity; it does not retain a finite quartic quantum problem.

The Page 5 benchmark (ζ,M)=(1,4)(\zeta,M)=(1,4) has (Mζ)/ζ=3(M-\zeta)/\zeta=3, so it is deliberately far from this threshold scaling.

Fixed λ\lambda produces a finite quartic quantum operator. To make that operator semiclassical as well, one needs λ1\lambda\gg1. In terms of Δ=Mζ\Delta=M-\zeta, simultaneous shape convergence and a deep-well limit require

Δζ0,Δ3ζ.\frac{\Delta}{\zeta}\to0, \qquad \frac{\Delta^3}{\zeta}\to\infty.

These conditions use the Page 5 convention =1\hbar=1. If the scaling is tuned through integer values of MM, the invariant-space dimension grows with MM. Although any fixed low level can be followed inside these growing algebraic sectors, the representation does not stabilize to a fixed-dimensional invariant polynomial space for the limiting quartic operator.

The global analytic passports remain different

Section titled “The global analytic passports remain different”

The quartic limit is local in the scaled coordinate. It does not erase the following global distinctions.

DatumQuartic completionHyperbolic completion
Real tailvQX4v_{\mathrm Q}\sim X^4vRe4aX/[4(C1)2]v_{\mathrm R}\sim \ee^{4a\lvert X\rvert}/[4(C-1)^2]
WKB growthXv ⁣dXX3/3\int^X\sqrt v\,\dd X\sim X^3/3Xv ⁣dXe2aX/[4a(C1)]\int^X\sqrt v\,\dd X\sim \ee^{2a\lvert X\rvert}/[4a(C-1)]
Turning pointsfour finite points in the XX-planeinfinitely repeated in xx, four on the exponential cylinder
Irregular endssectors of one polynomial infinitytwo distinct ends r=0,r=0,\infty
Canonical scalar formquartic Schrödinger normal form with one polynomial irregular infinityDCHE after r=e2xr=\ee^{2x}
Finite algebra used herenonefirst MM states when MNM\in\mathbb N

For Razavy, define

Y2=[ζ(r2+1)2Mr]24Er2.Y^2 = \left[ \zeta(r^2+1)-2Mr \right]^2 -4Er^2.

This is quartic in rr, but the WKB differential is

λR=Y4r2 ⁣dr.\lambda_{\mathrm R} = \frac{Y}{4r^2}\,\dd r.

For the normalized quartic,

y2=(1X2)2ε,λQ=y ⁣dX.y^2=(1-X^2)^2-\varepsilon, \qquad \lambda_{\mathrm Q}=y\,\dd X.

Both compactified branch curves are generically genus one. Genus does not determine a connection problem. On the quartic curve, λQ\lambda_{\mathrm Q} has a fourth-order pole at each of the two points above X=X=\infty. On the Razavy curve, λR\lambda_{\mathrm R} has a second-order pole at each of the two points above r=0r=0 and each of the two points above r=r=\infty. Thus the pole divisors differ: two fourth-order poles over one base endpoint versus four second-order poles over two base endpoints.

There is also a complex Razavy collision at

E=(M+ζ)2,r=1(x=πi2modπi),E=(M+\zeta)^2, \qquad r=-1 \quad \left(x=\frac{\pi i}{2}\bmod \pi i\right),

in addition to the real barrier collision E=(Mζ)2E=(M-\zeta)^2 at r=1r=1. As a0a\to0, the imaginary period πi/a\pi i/a of the hyperbolic shape recedes from every compact XX-window, but the finite-aa DCHE problem is not globally conjugate to the quartic polynomial-infinity problem.

Geometry, QES, and exact WKB answer different questions

Section titled “Geometry, QES, and exact WKB answer different questions”

In the normalized variables, every a>0a>0 and η>0\eta>0 corresponds to

ζ=1aη(C1),M=Caη(C1).\zeta = \frac{1}{a\eta(C-1)}, \qquad M = \frac{C}{a\eta(C-1)}.

The Razavy operator is QES only on the curves

Caη(C1)N.\frac{C}{a\eta(C-1)} \in\mathbb N.

That arithmetic condition neither creates the double-well shape nor makes a sub-barrier pair narrow. It merely closes the finite polynomial block derived on Page 5.

Choose the method from the question:

  • Deep quartic, fixed local level. Use the instanton/transseries quantization of Page 3 and audit it with its independent Galerkin and coordinate-space spectra.
  • Generic Razavy below the barrier. Use a DCHE connection determinant or exact WKB, then check with a parity-resolved coordinate solver.
  • Integer Razavy, first MM states. Use the finite Jacobi block as an exact calibration and check it independently against the full operator.
  • Near either separatrix. Use a uniform Weber treatment for coalescing turning points; a fixed-level dilute-instanton expansion is not uniform.
  • Above the barrier. Use the two-real-turning-point problem and stop calling adjacent levels a tunnelling doublet.

Detuning integer MM does not remove parity, the boundary problem, or the exact-WKB construction; only the finite block disappears. Away from discriminants and Stokes walls, chosen turning points and cycles continue analytically, although the Stokes graph may still wall-cross. Page 7, Quasi-exact solvability versus generic exact-WKB behavior, isolates that separation. Page 8, Three controlled capstones, will use recurrence, direct numerics, and exact WKB as genuinely independent checks.

Comparing raw numbers before normalizing. The two earlier pages use different coordinates, barriers, kinetic terms, and energy units. Match the passport before comparing levels, actions, or splittings.

Treating four real roots as proof of a doublet. Four roots establish a sub-barrier topology. Exponentially narrow splitting additionally requires a small normalized kinetic scale at fixed local level.

Using a bottom action as a finite-energy answer. The displayed actions are exact at the well bottom. A finite-energy splitting requires the energy-dependent inner cycle and model-specific fluctuation data.

Turning a local limit into a global Heun identity. The normalized Razavy potential converges to the quartic on compact scaled regions. Its finite-aa endpoint singularities and Stokes data remain different.

Using QES as a synonym for semiclassical. Integer MM is an algebraic closure condition. It does not imply a high barrier, a narrow doublet, or a terminating WKB series.

Starting from the operators on Pages 3 and 5, derive ηQ\eta_{\mathrm Q}, εQ\varepsilon_{\mathrm Q}, ηR\eta_{\mathrm R}, and εR\varepsilon_{\mathrm R}.

Solution

For the quartic problem, X=2q1X=2q-1 gives q=2X\partial_q=2\partial_X and q2(1q)2=(1X2)2/16q^2(1-q)^2=(1-X^2)^2/16. Multiplication by 32g32g produces

[(8g)2X2+(1X2)2]ψ=32gEQψ.\left[ -(8g)^2\partial_X^2+(1-X^2)^2 \right]\psi = 32gE_{\mathrm Q}\psi.

Hence

ηQ=8g,εQ=32gEQ.\eta_{\mathrm Q}=8g, \qquad \varepsilon_{\mathrm Q}=32gE_{\mathrm Q}.

For Razavy, x=aXx=aX and M=ζcosh2aM=\zeta\cosh2a. The barrier is Mζ=ζ(cosh2a1)M-\zeta=\zeta(\cosh2a-1) in square-root units. Division by its square gives

ηR=1a(Mζ),εR=ER(Mζ)2.\eta_{\mathrm R}=\frac{1}{a(M-\zeta)}, \qquad \varepsilon_{\mathrm R} = \frac{E_{\mathrm R}}{(M-\zeta)^2}.

2. Prove the shape ordering and compare curvatures

Section titled “2. Prove the shape ordering and compare curvatures”

Use the power series of cosh(2aX)\cosh(2aX) to prove vRvQv_{\mathrm R}\ge v_{\mathrm Q}, then differentiate at X=0,±1X=0,\pm1.

Solution

With u=X2u=X^2, every coefficient in

cosh(2aX)1=k1(2a)2kuk(2k)!\cosh(2aX)-1 = \sum_{k\ge1}\frac{(2a)^{2k}u^k}{(2k)!}

is positive. For u1u\le1, ukuu^k\le u; for u1u\ge1, ukuu^k\ge u. Comparing with u(cosh2a1)u(\cosh2a-1) and taking the correct absolute value on each side of u=1u=1 gives

cosh(2aX)cosh2acosh2a1X21.\frac{|\cosh(2aX)-\cosh2a|} {\cosh2a-1} \ge|X^2-1|.

Squaring proves the claim. Direct differentiation gives

vR(0)=4a2sinh2a,vR(±1)=8a2coth2a.v_{\mathrm R}''(0) = -\frac{4a^2}{\sinh^2a}, \qquad v_{\mathrm R}''(\pm1) = 8a^2\coth^2a.

The quartic values are 4-4 and 88.

3. Recover the turning-point limit and depth tests

Section titled “3. Recover the turning-point limit and depth tests”

Derive both pairs of positive turning points at normalized energy 0<ε<10<\varepsilon<1, and show that the hyperbolic pair tends to the quartic pair as a0a\to0.

Solution

The quartic equation

(1X2)2=ε(1-X^2)^2=\varepsilon

gives X2=1εX^2=1\mp\sqrt\varepsilon. For Razavy,

cosh(2aX)=C(C1)ε.\cosh(2aX) = C\mp(C-1)\sqrt\varepsilon.

Taking the positive inverse hyperbolic cosine gives the displayed inner and outer roots. Since

C(C1)ε=1+2a2(1ε)+O(a4)C\mp(C-1)\sqrt\varepsilon = 1+2a^2(1\mp\sqrt\varepsilon)+O(a^4)

and arcosh(1+2a2A)=2aA+O(a3)\operatorname{arcosh}(1+2a^2A)=2a\sqrt A+O(a^3), the quartic roots follow.

Near a minimum, vκ2(X1)2v\sim\kappa^2(X-1)^2. Here

κQ=2,κR=2acotha.\kappa_{\mathrm Q}=2, \qquad \kappa_{\mathrm R}=2a\coth a.

The local level is (2N+1)ηκ(2N+1)\eta\kappa, which yields the two depth diagnostics in the text.

Evaluate AR(a)\mathcal A_{\mathrm R}(a) and derive its small-aa limit. Then recover the near-threshold form of the raw Razavy action.

Solution

Inside the barrier,

vR=Ccosh(2aX)C1.\sqrt{v_{\mathrm R}} = \frac{C-\cosh(2aX)}{C-1}.

Integration gives

AR=2Csinh(2a)/aC1=43+4a245+O(a4).\mathcal A_{\mathrm R} = \frac{2C-\sinh(2a)/a}{C-1} = \frac43+\frac{4a^2}{45}+O(a^4).

For the raw action, put M=ζ+ΔM=\zeta+\Delta. From

cosh2a=1+Δζ\cosh2a=1+\frac{\Delta}{\zeta}

one has aΔ/(2ζ)a\sim\sqrt{\Delta/(2\zeta)}. Also,

SR=ζ(2acosh2asinh2a)=8ζa33+O(ζa5).S_{\mathrm R} = \zeta\left(2a\cosh2a-\sinh2a\right) = \frac{8\zeta a^3}{3}+O(\zeta a^5).

Substitution yields

SR223Δ3/2ζ.S_{\mathrm R} \sim \frac{2\sqrt2}{3} \frac{\Delta^{3/2}}{\sqrt\zeta}.

Hold λ=a(Mζ)\lambda=a(M-\zeta) fixed as a0a\to0. Derive the limiting operator and match its action to the Page 3 exponent.

Solution

The rescaled Razavy operator is exactly

a2HR=X2+λ2vR(X;a).a^2H_{\mathrm R} = -\partial_X^2+\lambda^2v_{\mathrm R}(X;a).

Local uniform convergence of the shape gives

a2HRX2+λ2(1X2)2.a^2H_{\mathrm R} \longrightarrow -\partial_X^2+\lambda^2(1-X^2)^2.

Multiplying the normalized quartic problem by ηQ2\eta_{\mathrm Q}^{-2} shows that λ=ηQ1=1/(8g)\lambda=\eta_{\mathrm Q}^{-1}=1/(8g). Therefore

λAQ=18g43=16g,\lambda\mathcal A_{\mathrm Q} = \frac{1}{8g}\frac43 = \frac{1}{6g},

which is the one-instanton exponent on Page 3.

Derive the quartic equation for the Razavy turning points in r=e2xr=\ee^{2x} and its WKB differential. Compare it with the normalized quartic curve.

Solution

Since

cosh2x=12(r+1r), ⁣dx= ⁣dr2r,\cosh2x=\frac12\left(r+\frac1r\right), \qquad \dd x=\frac{\dd r}{2r},

one finds

VRE=[ζ(r2+1)2Mr]24Er24r2.V_{\mathrm R}-E = \frac{ \left[\zeta(r^2+1)-2Mr\right]^2-4Er^2 }{4r^2}.

Thus the numerator can be denoted by Y2Y^2, and

VRE ⁣dx=Y4r2 ⁣dr.\sqrt{V_{\mathrm R}-E}\,\dd x = \frac{Y}{4r^2}\,\dd r.

Both Y2Y^2 and y2=(1X2)2εy^2=(1-X^2)^2-\varepsilon are quartic branch curves and are generically genus one. On the compact quartic curve, y ⁣dXy\,\dd X has fourth-order poles at the two points above X=X=\infty. On the compact Razavy curve, Y ⁣dr/(4r2)Y\,\dd r/(4r^2) has second-order poles at the two points above r=0r=0 and the two points above r=r=\infty. Therefore the genera agree while the pole divisors, periods, and connection data need not.

7. Separate geometry, QES, and method choice

Section titled “7. Separate geometry, QES, and method choice”

Classify the four parameter pairs

(ζ,M)=(2,1),(1,5/2),(1,4),(2,3/2),(\zeta,M) = (2,1),\quad (1,5/2),\quad (1,4),\quad (2,3/2),

then name the primary method and one independent check for a deep quartic, a generic noninteger Razavy well, and the first MM states of an integer Razavy well.

Solution

The conditions are independent:

(ζ,M)(\zeta,M)GeometryAlgebra
(2,1)(2,1)single wellQES, M=1M=1
(1,5/2)(1,5/2)double wellnon-QES
(1,4)(1,4)double wellQES
(2,3/2)(2,3/2)single wellnon-QES

For a deep quartic at fixed local level, use its instanton/transseries condition and compare the Galerkin and coordinate-space spectra. For noninteger Razavy, use exact WKB or the DCHE connection problem and check a parity-resolved grid. For the first MM integer-Razavy states, use the finite Jacobi block and check the full coordinate operator. Near either barrier top, replace a fixed-level instanton formula by a uniform turning-point treatment.