Polyhedra, Moduli,
and Quantum Geometry

Web working edition

On this page
  1. 16.1 Peripheral conventions and the two small parameters
  2. 16.2 What the linear term does to real volume optimization
  3. 16.3 The cusp shape in the inverse volume Hessian
  4. 16.4 An exact holomorphic critical-value identity
  5. 16.5 The Neumann–Zagier coefficients through sixth order
  6. 16.6 Computing the quartic coefficient from angle-volume derivatives
  7. 16.7 The closed quantum-volume statement and its local consequence
  8. 16.8 The Gaussian factor and the torsion surgery formula
  9. 16.9 A figure-eight benchmark and the scope of the conclusion
  10. 16.10 The symplectic pairing behind the calculation
  11. 16.10.1 From the tetrahedra to the boundary intersection form
  12. 16.10.2 The potential and the volume primitive
  13. 16.10.3 Filling as a canonical transformation
  14. 16.10.4 Covariance of the filling coefficients
  15. 16.10.5 An exact Hessian and Monge–Ampere identity
  16. 16.10.6 The quantum Gaussian as a half-density transformation

16 Dehn filling, variational response, and quantum surgery

There is a second route from volume optimization to a quantum-volume comparison: perturb a complete cusped structure by prescribing peripheral holonomy. This route has a particularly explicit answer. The critical-value response of the real concave optimization recovers the Euclidean cusp quadratic form. After passage to a holomorphic boundary potential, the local volume response is exactly the imaginary part of a Legendre critical value, and gives the filled volume when the geometric completion exists. Its Taylor coefficients reproduce the Neumann–Zagier expansion, and its Hessian is the derivative entering the torsion surgery formula. These are deductions from the established variational, deformation, and torsion identities cited below; no novelty claim is made.

16.1 Peripheral conventions and the two small parameters

Let MM be an oriented, finite-volume, one-cusped hyperbolic three-manifold. Fix an oriented meridian–longitude basis (μ,λ)(\mu,\lambda) and the geometric deformation branch through the complete structure. We use logarithms of the PSL2(ℂ)\mathrm{PSL}_2(\mathbb C) multipliers, equivalently of the eigenvalue ratios, so that u=H(μ),v=H(λ),v(u)=τu+c3u3+c5u5+O(u7),B=ℑτ>0.u=H(\mu),\qquad v=H(\lambda),\qquad v(u)=\tau u+c_3u^3+c_5u^5+O(u^7),\qquad B=\Im\tau>0.(16.1) Thus uu is twice a local logarithm of an SL2\mathrm{SL}_2 eigenvalue, after removing its constant sign at the complete representation. In particular, the smooth filling equation is pu+qv=2πipu+qv=2\pi i, with the branch chosen continuously from the cusp. Using eigenvalue logarithms û=u/2\widehat u=u/2, v̂=v/2\widehat v=v/2 instead gives pû+qv̂=πip\widehat u+q\widehat v=\pi i and v̂=τû+4c3û3+16c5û5+⋯\widehat v=\tau\widehat u+4c_3\widehat u^3+16c_5\widehat u^5+\cdots. The oddness and the holomorphic potential are those of Neumann–Zagier [36, Sections 4–6].

For a primitive slope (p,q)(p,q) put A=p+qτ,Q(p,q)=|A|2B,pu+qv(u)=iθ.A=p+q\tau,\qquad Q(p,q)=\frac{|A|^2}{B},\qquad pu+qv(u)=i\theta.(16.2) Here θ\theta is an angular holonomy parameter. It is the cone angle when the local structure has the corresponding geometric cone completion; θ=0\theta=0 is the complete cusp and θ=2π\theta=2\pi gives a smooth hyperbolic filling when that completion exists. The quantity QQ is the squared length of the slope on a Euclidean cusp cross section divided by its area. For sufficiently long slopes the small solution stays in one fixed holonomy neighborhood throughout 0≤θ≤2π0\leq\theta\leq2\pi. Indeed, put h(u)=v(u)−τu=O(u3)h(u)=v(u)-\tau u=O(u^3) and t=q/At=q/A. Since |t|≤B−1|t|\leq B^{-1}, a sufficiently small disk has |th′(u)|<1/2|t h'(u)|<1/2 uniformly in the slope. The equation u+th(u)=iθ/Au+t h(u)=i\theta/A then has a unique small analytic solution, uniformly for bounded θ\theta and sufficiently large |A||A|, with u=O(|A|−1)u=O(|A|^{-1}). This is an assertion about a holonomy germ; the hyperbolic Dehn surgery theorem supplies the smooth geometric completion for sufficiently long primitive slopes [36, Section 4]. Geometric completion is a separate statement from the analytic existence of this small solution.

Two expansions must be kept distinct: |A|−1→0|A|^{-1}\to0 is a classical long-slope expansion, whereas the quantum level r→∞r\to\infty is a semiclassical expansion. The coefficients c3,c5c_3,c_5 belong to the first. They are not by themselves quantum two-loop or higher-loop coefficients.

16.2 What the linear term does to real volume optimization

Suppose a chosen ideal triangulation of the compact core of MM has a positive complete geometric angle structure, with every ideal vertex link a torus. Use independent linear coordinates xx on its full angle space, with tetrahedral and edge-angle constraints already imposed, and center them at the complete maximum x=0x=0. Write 𝒱(x)=∑tetrahedraVol⁡(Δx),V0=𝒱(0),K=−D2𝒱(0)>0.\mathscr V(x)=\sum_{\text{tetrahedra}}\mathop{\mathrm{Vol}}(\Delta_x),\qquad V_0=\mathscr V(0),\qquad K=-D^2\mathscr V(0)>0. Peripheral angular holonomies are affine in the angles and vanish at 00 in the selected branches. Thus there is a real linear map PP such that Px=(ℑuℑv),L=(pq)P,Lx=θ.Px=\binom{\Im u}{\Im v},\qquad L=(p\ \ q)P,\qquad Lx=\theta. The boundary intersection pairing gives rank⁡P=2\operatorname{rank}P=2, so L≠0L\ne0. Together with K>0K>0, this makes the constrained stationarity system invertible at 00 and gives a unique nearby interior maximizer for sufficiently small θ\theta. These assertions use the full constrained angle space, not an arbitrarily restricted family of tetrahedral shapes.

At that maximizer, the leading–trailing edge variations impose the missing real edge equations; the peripheral variation imposes the missing real filling equation. This follows from the angle-holonomy pairing and volume derivative in [37, Lemma 4.4, Proposition 4.6 and Proposition 5.4]. It first identifies a local edge-glued holonomy solution. At θ=2π\theta=2\pi, an interior critical point on the corresponding slice gives a complete hyperbolic filling by their Theorem 6.1. For other angular slices we retain the local holonomy interpretation unless a cone completion is specified. For long slopes the small holonomy solution stays in this positive geometric neighborhood throughout a bounded angular interval, so the same constrained-stationarity identification applies there.

To see the peripheral part directly, on the edge-glued deformation space the volume differential is ⁡dV=12(ℜv⁡dℑu−ℜu⁡dℑv).\mathop{}\!\mathrm dV=\frac12\bigl(\Re v\,\mathop{}\!\mathrm d\Im u -\Re u\,\mathop{}\!\mathrm d\Im v\bigr).(16.3) Requiring this covector to be proportional to p⁡dℑu+q⁡dℑvp\,\mathop{}\!\mathrm d\Im u+q\,\mathop{}\!\mathrm d\Im v gives pℜu+qℜv=0p\Re u+q\Re v=0. Hence the single angular condition, together with constrained criticality, gives the full complex equation (16.2).

The proposed linear perturbation can therefore be written as ℬ(j)=maxx{𝒱(x)+jLx},θ=ℬ′(j),Vp,q(θ)=ℬ(j)−jθ.\mathscr B(j)=\max_x\{\mathscr V(x)+jLx\},\qquad \theta=\mathscr B'(j),\qquad V_{p,q}(\theta)=\mathscr B(j)-j\theta.(16.4) All statements here are local near the unique interior complete maximum. The envelope theorem gives Vp,q′(θ)=−j.V_{p,q}'(\theta)=-j. On a geometric cone branch, the Schläfli formula gives Vp,q′(θ)=−ℓcore/2V_{p,q}'(\theta)=-\ell_{\mathrm{core}}/2, so the coefficient of the added real linear term is j=ℓcore2.\boxed{j=\frac{\ell_{\mathrm{core}}}2.}(16.5) The cone angle is its conjugate variable. In particular, the critical value ℬ\mathscr B of the biased objective and the physical volume Vp,qV_{p,q} must be distinguished by the Legendre subtraction in (16.4).

16.3 The cusp shape in the inverse volume Hessian

Set χ=LK−1LT.\chi=L K^{-1}L^T. Differentiating the stationary equation for the perturbed objective gives ⁡dxj⁡dj|j=0=K−1LT,ℬ″(0)=χ.\left.\frac{\mathop{}\!\mathrm dx_j}{\mathop{}\!\mathrm dj}\right|_{j=0}=K^{-1}L^T, \qquad \mathscr B''(0)=\chi. Consequently Vp,q(θ)=V0−θ22χ+O(θ4).V_{p,q}(\theta)=V_0-\frac{\theta^2}{2\chi}+O(\theta^4).(16.6) Evenness follows from the signed-cone continuation u↦−uu\mapsto-u. Comparison with the geometric calculation below yields LK−1LT=2|p+qτ|2ℑτ=2Q(p,q).\boxed{L K^{-1}L^T=\frac{2|p+q\tau|^2}{\Im\tau}=2Q(p,q).}(16.7) Equivalently, writing a=ℜτa=\Re\tau, PK−1PT=2B(1aa|τ|2),det⁡(PK−1PT)=4.\boxed{ P K^{-1}P^T=\frac2B \begin{pmatrix}1&a\\a&|\tau|^2\end{pmatrix},\qquad \det(P K^{-1}P^T)=4.}(16.8) Thus the peripheral response of the angle-volume Hessian determines the cusp shape. Although KK and PP depend on the triangulation, this two-by-two matrix depends only on the marked cusp. The formula assumes the nondegenerate positive angle maximum above; it is not a claim that an arbitrary chosen ideal triangulation has one.

16.4 An exact holomorphic critical-value identity

Define F(u)=∫0uv(t)⁡dt=τu22+c3u44+c5u66+O(u8).F(u)=\int_0^u v(t)\,\mathop{}\!\mathrm dt =\frac{\tau u^2}{2}+\frac{c_3u^4}{4} +\frac{c_5u^6}{6}+O(u^8).(16.9) With Neumann–Zagier’s convention ΦNZ′=2v\Phi_{\mathrm{NZ}}'=2v, this is F=ΦNZ/2F=\Phi_{\mathrm{NZ}}/2, after fixing the additive constant. Assume q≠0q\ne0 and set 𝒮p,q(u;θ)=F(u)+p2qu2−iθqu.\boxed{ \mathcal S_{p,q}(u;\theta) =F(u)+\frac{p}{2q}u^2-\frac{i\theta}{q}u.}(16.10) The quadratic term implements the change of peripheral polarization; the final term is linear in the boundary coordinate. Its critical equation is exactly pu+qv=iθpu+qv=i\theta. Let uθu_\theta denote the small critical solution, and write 𝒮*(θ)=𝒮p,q(uθ;θ)\mathcal S^*(\theta)=\mathcal S_{p,q}(u_\theta;\theta).

Proposition 16.1 (Local filling critical value). On the local geometric deformation branch through the complete cusp, with Vp,qV_{p,q} interpreted as its volume germ (or the volume of its geometric completion when this exists), Vp,q(θ)−V0=12ℑ𝒮*(θ).\boxed{V_{p,q}(\theta)-V_0=\frac12\Im\mathcal S^*(\theta).}(16.11) Moreover, ⁡d𝒮*⁡dθ=−iuθq,⁡d2𝒮*⁡dθ2=1q(p+qv′(uθ)).\frac{\mathop{}\!\mathrm d\mathcal S^*}{\mathop{}\!\mathrm d\theta}=-\frac{i u_\theta}{q},\qquad \frac{\mathop{}\!\mathrm d^2\mathcal S^*}{\mathop{}\!\mathrm d\theta^2} =\frac{1}{q\bigl(p+qv'(u_\theta)\bigr)}.(16.12)

Proof. Choose integers ρ,σ\rho,\sigma with pσ−qρ=1p\sigma-q\rho=1. The complementary peripheral holonomy is w=ρu+σv=iσθ−uq.w=\rho u+\sigma v=\frac{i\sigma\theta-u}{q}. When a geometric cone completion exists, in these orientation conventions the physical core complex length has positive real part when represented by −w-w, and therefore ℓcore=ℜ(u/q)\ell_{\mathrm{core}}=\Re(u/q) near the positive cone branch. The envelope theorem gives the first identity in (16.12). Its half imaginary part is −ℓcore/2-\ell_{\mathrm{core}}/2, exactly the Schläfli derivative of volume. Both sides of (16.11) vanish at θ=0\theta=0. Differentiating puθ+qv(uθ)=iθpu_\theta+qv(u_\theta)=i\theta gives the second identity in (16.12).

There is also an algebraic proof valid directly on the local holonomy branch. Neumann–Zagier’s volume formula is V(u)−V0=14ℑ(uv‾)+ℑ(12F(u)−14uv)=12ℑF(u)−12ℜuℑv.(16.13)\begin{aligned} V(u)-V_0 &=\frac14\Im(u\bar v) +\Im\left(\frac12F(u)-\frac14uv\right)\\ &=\frac12\Im F(u)-\frac12\Re u\,\Im v. \end{aligned} Substituting ℑv=(θ−pℑu)/q\Im v=(\theta-p\Im u)/q yields (16.11). This proof avoids assuming an independently constructed cone path. ◻

This is an exact identity of analytic germs, so it compares all orders of the two classical expansions. For q=0q=0, exchange the oriented basis to (μ′,λ′)=(λ,−μ)(\mu',\lambda')=(\lambda,-\mu); the new slope has q′=−p≠0q'=-p\ne0. The real angle optimization itself needs no such basis change. Primitive q=0q=0 slopes have p=±1p=\pm1 and do not occur in a long-slope sequence in a fixed basis. Figure 6 records the local intersection condition and the response at the complete structure.

Dehn filling in peripheral phase space
Figure 6. Local Dehn filling as an intersection in the complex peripheral holonomy space. The drawing records the intersection condition; it is not a real slice of the complex deformation curve. Here u,vu,v are logarithms of multipliers, θ=0\theta=0 is the complete structure, and θ=2π\theta=2\pi gives smooth filling when the branch has that geometric completion. The Hessian response formula assumes the nondegenerate positive angle maximum specified in the text.

16.5 The Neumann–Zagier coefficients through sixth order

Series inversion of (16.2) gives uθ=iθA+iqc3θ3A4+iθ5(3q2c32A7−qc5A6)+⋯.u_\theta=\frac{i\theta}{A} +\frac{iqc_3\theta^3}{A^4} +i\theta^5\left(\frac{3q^2c_3^2}{A^7} -\frac{qc_5}{A^6}\right)+\cdots.(16.14) Substitution in the action, or integration of the envelope derivative, gives 𝒮*(θ)=θ22qA+c3θ44A4+θ66(3qc32A7−c5A6)+⋯.\mathcal S^*(\theta)=\frac{\theta^2}{2qA} +\frac{c_3\theta^4}{4A^4} +\frac{\theta^6}{6} \left(\frac{3qc_3^2}{A^7}-\frac{c_5}{A^6}\right)+\cdots.(16.15) Taking half its imaginary part yields the volume loss V0−Vp,q(θ)=Bθ24|A|2−θ48ℑc3A4−θ612ℑ(3qc32A7−c5A6)+O(|A|−8).(16.16)\begin{aligned} V_0-V_{p,q}(\theta) ={}&\frac{B\theta^2}{4|A|^2} -\frac{\theta^4}{8}\Im\frac{c_3}{A^4}\\ &-\frac{\theta^6}{12} \Im\left(\frac{3qc_3^2}{A^7}-\frac{c_5}{A^6}\right) +O(|A|^{-8}). \end{aligned} Here the displayed remainder is a long-slope estimate for bounded θ\theta, on the common holonomy neighborhood constructed above. The uniform analytic inverse expands in iθ/Ai\theta/A with coefficients analytic in the bounded parameter q/Aq/A; the next volume terms are therefore O(|A|−8)O(|A|^{-8}). Since q/Aq/A is bounded, the three displayed terms have orders |A|−2,|A|−4,|A|−6|A|^{-2},|A|^{-4},|A|^{-6}. For a fixed slope and θ→0\theta\to0, the corresponding Taylor remainder is O(θ8)O(\theta^8).

For the smooth hyperbolic filling Mp/qM_{p/q} this becomes V0−Vol⁡(Mp/q)=π2B|A|2−2π4ℑc3A4−16π63ℑ(3qc32A7−c5A6)+O(|A|−8).(16.17)\begin{aligned} \boxed{\begin{aligned} V_0-\mathop{\mathrm{Vol}}(M_{p/q}) ={}&\frac{\pi^2B}{|A|^2} -2\pi^4\Im\frac{c_3}{A^4}\\ &-\frac{16\pi^6}{3} \Im\left(\frac{3qc_3^2}{A^7}-\frac{c_5}{A^6}\right) +O(|A|^{-8}). \end{aligned}} \end{aligned} These are the Neumann–Zagier coefficients, with the multiplier normalization fixed explicitly [36, Section 6]. In particular the leading loss is π2/Q(p,q)\pi^2/Q(p,q), and the quartic term detects the first nonlinear deformation coefficient c3c_3.

16.6 Computing the quartic coefficient from angle-volume derivatives

The comparison supplies a more detailed computational identity. Keep K,L,χK,L,\chi as above, and write T3=D3𝒱(0),T4=D4𝒱(0),e=K−1LTχ,R=K−1−K−1LTLK−1χ.T_3=D^3\mathscr V(0),\qquad T_4=D^4\mathscr V(0),\qquad e=\frac{K^{-1}L^T}{\chi},\qquad R=K^{-1}-\frac{K^{-1}L^TLK^{-1}}{\chi}. Let t=T3(e,e,⋅)t=T_3(e,e,\cdot) be the resulting column covector. Solving the constrained stationary equation to second order gives xθ=θe+θ22Rt+O(θ3).x_\theta=\theta e+\frac{\theta^2}{2}Rt+O(\theta^3). Indeed Le=1Le=1, LR=0LR=0, and RKRK is the identity on ker⁡L\ker L. Inserting this expression into the Taylor expansion of 𝒱\mathscr V gives Vp,q(θ)=V0−θ22χ+θ36T3[e,e,e]+θ424(T4[e,e,e,e]+3tTRt)+O(θ5).(16.18)\begin{aligned} V_{p,q}(\theta)={}&V_0-\frac{\theta^2}{2\chi} +\frac{\theta^3}{6}T_3[e,e,e]\\ &+\frac{\theta^4}{24} \left(T_4[e,e,e,e]+3t^TRt\right)+O(\theta^5). \end{aligned} The cross term with the unknown cubic displacement vanishes because that displacement is in ker⁡L\ker L and Ke=LT/χKe=L^T/\chi. The remaining quadratic-displacement terms combine to tTRt/8t^TRt/8. Evenness of the geometric branch then removes the odd coefficients and improves the remainder to O(θ6)O(\theta^6). Comparison with (16.16) yields T3[e,e,e]=0,T4[e,e,e,e]+3tTRt=3ℑc3(p+qτ)4.\boxed{T_3[e,e,e]=0,\qquad T_4[e,e,e,e]+3t^TRt =3\Im\frac{c_3}{(p+q\tau)^4}.}(16.19) Thus c3c_3 can be accessed from derivatives of the angle-volume functional by varying the slope. The correction 3tTRt3t^TRt accounts for readjustment of all other angles. Keeping only the raw fourth derivative would miss that response.

16.7 The closed quantum-volume statement and its local consequence

A precise closed-manifold analogue is the Chen–Yang volume conjecture. At the specified root ζr=e2πi/r\zeta_r=e^{2\pi i/r}, with rr odd, its absolute-growth statements are 4πrlog⁡|RTr(N;ζr)|→Vol⁡(N),2πrlog⁡TVr(N;ζr)→Vol⁡(N).\frac{4\pi}{r}\log|\mathrm{RT}_r(N;\zeta_r)|\longrightarrow\mathop{\mathrm{Vol}}(N), \qquad \frac{2\pi}{r}\log\mathrm{TV}_r(N;\zeta_r)\longrightarrow\mathop{\mathrm{Vol}}(N).(16.20) The root and normalization matter; these are the Chen–Yang versions for hyperbolic manifolds [38]. We use absolute growth to avoid mixing the different Chern–Simons sign conventions in the literature.

For a boundary state whose geometric semiclassical phase satisfies Φ(u)=Φ0+12F(u),ℑΦ0=V0,\Phi(u)=\Phi_0+\frac12F(u),\qquad \Im\Phi_0=V_0, the filling phase is 𝒯θ(u)=Φ0+12𝒮p,q(u;θ).\mathcal T_\theta(u)=\Phi_0+\frac12\mathcal S_{p,q}(u;\theta).(16.21) Possible real framing constants do not alter its imaginary part. With ℏr=4πi/r\hbar_r=4\pi i/r, Proposition 16.1 immediately gives |e𝒯θ(uθ)/ℏr|=exp⁡(r4πVp,q(θ)).\left|e^{\mathcal T_\theta(u_\theta)/\hbar_r}\right| =\exp\left(\frac{r}{4\pi}V_{p,q}(\theta)\right).(16.22) In particular, the deformation of the geometric exponential is log⁡|e𝒯θ(uθ)/ℏreΦ0/ℏr|=−r4π(V0−Vp,q(θ)).\log\left|\frac{e^{\mathcal T_\theta(u_\theta)/\hbar_r}} {e^{\Phi_0/\hbar_r}}\right| =-\frac{r}{4\pi}\bigl(V_0-V_{p,q}(\theta)\bigr).(16.23) Every classical coefficient in (16.16) therefore appears with precisely the required quantum exponential coefficient. At θ=2π\theta=2\pi, Yoshida’s complex-volume formula has this normalization; see the unnumbered filling formula and the potential normalization (5.9) on [40, p. 456]. Quadratic and linear filling kernels also appear explicitly in [39, equations (12)–(14)]; their boundary coordinates and level conventions must be converted before numerical coefficients are compared.

Proposition 16.2 (Conditional local quantum transfer). Suppose an exact surgery representation for a specified quantum invariant has, near the geometric branch, phase 𝒯θ\mathcal T_\theta and a uniform classical-symbol expansion of its amplitude. Suppose the geometric critical point is nondegenerate, its steepest-descent cycle occurs with nonzero coefficient in the specified integration cycle, the net leading stationary-phase coefficient of that geometric sector is uniformly bounded away from zero, and the remaining integral or sum is exponentially smaller, uniformly on a chosen compact deformation interval. Then stationary phase gives the volume exponent (16.22) for the full invariant, with a uniform expansion on that interval. Without the last global condition, the same statement holds for the specified local geometric contribution.

Proof. At the geometric critical point, 𝒯θ″(uθ)=p+qv′(uθ)2q≠0.\mathcal T_\theta''(u_\theta) =\frac{p+qv'(u_\theta)}{2q}\ne0. Uniform stationary phase on the stipulated cycle gives a nonzero amplitude times e𝒯θ(uθ)/ℏre^{\mathcal T_\theta(u_\theta)/\hbar_r}, with powers of r−1r^{-1} and a Gaussian power of rr according to the normalization of the kernel. Such powers contribute only O(log⁡r/r)O(\log r/r) to normalized logarithmic growth. The exponential gap permits the addition of the remaining terms without changing the leading growth. The critical-value proposition identifies the exponent with the geometric volume. ◻

For a general knot this proposition identifies the needed analytic input; it does not establish that input from a complete-point Kashaev asymptotic alone. A value at u=0u=0 does not provide a uniform boundary-state expansion near 00, and a local critical point does not by itself specify its coefficient in the global surgery sum. The regular tetrahedral Airy formula in Section 15 concerns a different integral and does not supply that missing manifold-level information.

16.8 The Gaussian factor and the torsion surgery formula

The derivative of the filling map is D*:=p+qv′(uθ),⁡duθ⁡dθ=iD*,𝒮uu(uθ;θ)=D*q.D_*:=p+qv'(u_\theta),\qquad \frac{\mathop{}\!\mathrm du_\theta}{\mathop{}\!\mathrm d\theta}=\frac{i}{D_*},\qquad \mathcal S_{uu}(u_\theta;\theta)=\frac{D_*}{q}.(16.24) Thus the same quantity controls the classical susceptibility and the Gaussian surgery integral. With the usual square-root normalization of the boundary Fourier kernel, its contribution has dependence D*−1/2D_*^{-1/2}, up to the common normalization and phase choices. A full amplitude also contains the boundary-state torsion and a solid-torus factor.

More precisely, suppose θ=2π\theta=2\pi gives a smooth hyperbolic filled manifold and the representation is its holonomy. Assume its adjoint representation is acyclic and its restriction to the compact core is regular for both μ\mu and pμ+qλp\mu+q\lambda: the peripheral invariant vector paired with either curve supplies a basis of the one-dimensional twisted H1H_1, with the compatible boundary basis in H2H_2. In the local holonomy chart this requires D*≠0D_*\ne0; the core is loxodromic, so sinh⁡(w/2)≠0\sinh(w/2)\ne0. The change-of-peripheral-curve and surgery formulas for adjoint Reidemeister torsion then give Tor⁡pμ+qλ(Mu)=(p+qv′(u))Tor⁡μ(Mu),Tor⁡(Mp/q)=Tor⁡pμ+qλ(Mu)4sinh⁡2(w/2),w=ρu+σv.(16.25)\begin{aligned} \operatorname{Tor}_{p\mu+q\lambda}(M_u) &=\bigl(p+qv'(u)\bigr)\operatorname{Tor}_\mu(M_u),\\ \operatorname{Tor}(M_{p/q}) &=\frac{\operatorname{Tor}_{p\mu+q\lambda}(M_u)} {4\sinh^2(w/2)},\qquad w=\rho u+\sigma v. \end{aligned} These are understood up to the standard torsion signs and consistent choices of square root. They are the identities used in [40, equations (5.16) and (5.23)]. For the general regularity and change-of-curve statements, see [129, Propositions 5.13–5.14]; its Proposition 4.23(b), specialized to the adjoint representation (k1,k2)=(2,0)(k_1,k_2)=(2,0), gives the surgery factor up to the torsion sign. Consequently the expected full geometric amplitude is proportional to 2sinh⁡(w/2)(p+qv′(u))Tor⁡μ(Mu)=1Tor⁡(Mp/q).\boxed{ \frac{2\sinh(w/2)} {\sqrt{\bigl(p+qv'(u)\bigr)\operatorname{Tor}_\mu(M_u)}} =\frac{1}{\sqrt{\operatorname{Tor}(M_{p/q})}}.}(16.26) The identity shows what must accompany the boundary Hessian. Matching the Gaussian factor alone would leave out both the cusp torsion and the solid-torus amplitude. This one-loop comparison uses more information than the classical volume exponent. The closed-manifold torsion in this formula is evaluated at smooth filling; it is not being assigned to a generic cone holonomy. At the cusp endpoint θ=0\theta=0 the solid-torus factor vanishes, so a uniform quantum statement including that endpoint requires a separate normalization and analysis. The compact parameter interval in Proposition 16.2 is subject to its nonvanishing-amplitude hypothesis.

16.9 A figure-eight benchmark and the scope of the conclusion

For the figure-eight knot complement, in the standard peripheral basis Neumann–Zagier compute [36, equation (68)] v(u)=23i(u+u33+23u5180+O(u7)).v(u)=2\sqrt3\,i\left(u+\frac{u^3}{3} +\frac{23u^5}{180}+O(u^7)\right).(16.27) Thus τ=23i\tau=2\sqrt3\,i, c3=2i/3c_3=2i/\sqrt3, and c5=23i/(303)c_5=23i/(30\sqrt3). The first two volume-loss terms are V0−Vol⁡(Mp/q)=23π2p2+12q2−4π43p4−72p2q2+144q4(p2+12q2)4+O((p2+q2)−3).(16.28)\begin{aligned} V_0-\mathop{\mathrm{Vol}}(M_{p/q})={}&\frac{2\sqrt3\,\pi^2}{p^2+12q^2}\\ &-\frac{4\pi^4}{\sqrt3} \frac{p^4-72p^2q^2+144q^4}{(p^2+12q^2)^4} +O\bigl((p^2+q^2)^{-3}\bigr). \end{aligned} This agrees directly with the expansion following equation (68) in [36]. The angle-Hessian response is correspondingly χ=p2+12q23.\chi=\frac{p^2+12q^2}{\sqrt3}.

An independent calculation starts with the two regular ideal tetrahedra and their Lobachevsky volume. In the Neumann–Zagier presentation their shapes z1,z2z_1,z_2 satisfy z1z2(z1−1)(z2−1)=1,u=log⁡(z2(1−z1)),v=2log⁡(z1(1−z1)).z_1z_2(z_1-1)(z_2-1)=1,\qquad u=\log\bigl(z_2(1-z_1)\bigr),\qquad v=2\log\bigl(z_1(1-z_1)\bigr). Eliminating the shapes from these equations gives the local peripheral relation cosh⁡(v/2)=1+cosh⁡u−cosh⁡(2u).\cosh(v/2)=1+\cosh u-\cosh(2u). Equivalently, with the eigenvalue variables m=eu/2m=e^{u/2} and l=−ev/2l=-e^{v/2}, it is l+l−1=m4−m2−2−m−2+m−4l+l^{-1}=m^4-m^2-2-m^{-2}+m^{-4}, the nonabelian figure-eight AA-polynomial relation in this choice of signs. The sign in ll is essential: its complete value is −1-1 whereas v(0)=0v(0)=0. The equation and the chosen tangent v′(0)=23iv'(0)=2\sqrt3\,i recover the cubic and quintic coefficients above. This is a local branch calculation, not a classification of the global curve or of fillings.

Use αi=arg⁡zi\alpha_i=\arg z_i, βi=−arg⁡(1−zi)\beta_i=-\arg(1-z_i), and γi=π−αi−βi\gamma_i=\pi-\alpha_i-\beta_i. Choose the independent variations ξ=(δα1,δβ1,δα2)\xi=(\delta\alpha_1,\delta\beta_1,\delta\alpha_2). The edge equation then makes the six angle variations Eξ=(ξ1,ξ2,−ξ1−ξ2,ξ3,ξ1−ξ2+ξ3,−ξ1+ξ2−2ξ3).E\xi=(\xi_1,\xi_2,-\xi_1-\xi_2, \xi_3,\xi_1-\xi_2+\xi_3,-\xi_1+\xi_2-2\xi_3). At the complete structure all six angles are π/3\pi/3. Since Λ″(α)=−cot⁡α\Lambda''(\alpha)=-\cot\alpha, direct differentiation gives K=13(4−13−14−33−36),P=(0−112−20),PK−1PT=13(10012).K=\frac1{\sqrt3} \begin{pmatrix}4&-1&3\\-1&4&-3\\3&-3&6\end{pmatrix},\qquad P=\begin{pmatrix}0&-1&1\\2&-2&0\end{pmatrix},\qquad P K^{-1}P^T=\frac1{\sqrt3} \begin{pmatrix}1&0\\0&12\end{pmatrix}.(16.29) This recovers the cusp shape directly from the optimizer. Put D0=p2+12q2D_0=p^2+12q^2. The unit angular-response vector is e=(6q−p,−6q−p,p−6q)T2D0.e=\frac{(6q-p,-6q-p,p-6q)^T}{2D_0}. Using Λ‴(π/3)=43,Λ⁗(π/3)=−833,\Lambda'''(\pi/3)=\frac43,\qquad \Lambda''''(\pi/3)=-\frac8{3\sqrt3}, the six entries of EeEe occur in opposite pairs, so T3[e,e,e]=0T_3[e,e,e]=0. Direct contraction of the fourth derivative and the constrained inverse-Hessian correction gives T4[e,e,e,e]+3tTRt=23(p4−72p2q2+144q4)D04.T_4[e,e,e,e]+3t^TRt =\frac{2\sqrt3\,(p^4-72p^2q^2+144q^4)}{D_0^4}.(16.30) Multiplying by θ4/24\theta^4/24 and setting θ=2π\theta=2\pi gives the quartic filled-volume term in (16.28) with the opposite sign, as required for volume rather than volume loss. Thus the real optimization and the holomorphic series agree in a calculation made directly from the tetrahedral volume derivatives.

For this example there is also a theorem about the actual quantum invariants: Wong–Yang prove the leading RT asymptotic with relative error O(r−1)O(r^{-1}), and the RT/TV volume conjectures for every hyperbolic rational Dehn filling of the figure-eight knot [40, Theorems 1.1 and 1.2]. Their leading amplitude is the inverse square root of adjoint torsion, with their specified overall constant. Thus the local consistency calculation above is contained in a stronger result in that example. The present discussion reorganizes the comparison around volume optimization and its derivatives; it does not produce a new case of the quantum-volume conjecture.

For a general knot, the unconditional results here are the classical critical-value identity and its coefficient dictionary. The quantum conclusion for a specified local geometric contribution follows under the stated stationary-phase hypotheses. Passing to the full invariant requires control of its exact surgery representation and all competing contributions. One should first keep the filling slope fixed while taking r→∞r\to\infty, and then study the long-slope coefficients. A simultaneous limit in which the slope grows with rr requires uniform estimates not supplied by separate fixed-slope expansions.

The computational companion in experiments/quantum_surgery/README.md, with output at artifacts/quantum_surgery/result.json, checks finite formal series, canonical-coordinate identities, and the figure-eight angle-Hessian contractions in exact arithmetic. These fixtures check the displayed coefficient algebra. They do not compute a filled hyperbolic manifold or an exact quantum invariant, and do not establish convergence, a global integration cycle, or its noncancellation.

16.10 The symplectic pairing behind the calculation

The pairing in Neumann–Zagier is the structure behind the preceding formulas. It identifies the peripheral variables as conjugate coordinates, makes the geometric deformation locus Lagrangian, and fixes the canonical transformation for Dehn filling. We record the normalization explicitly, since interchanging meridian and longitude or using eigenvalue rather than multiplier logarithms changes the displayed signs or factors.

16.10.1 From the tetrahedra to the boundary intersection form

For nn ideal tetrahedra introduce independent ambient coordinates Zj=log⁡zj,Wj=log⁡(1−zj),Ωtet=∑j=1n⁡dZj∧⁡dWj.Z_j=\log z_j,\qquad W_j=\log(1-z_j),\qquad \Omega_{\mathrm{tet}}=\sum_{j=1}^n\mathop{}\!\mathrm dZ_j\wedge\mathop{}\!\mathrm dW_j. The actual shapes satisfy eZj+eWj=1e^{Z_j}+e^{W_j}=1. Their product is a complex Lagrangian of dimension nn in this 2n2n-dimensional phase space. The logarithmic edge equations and peripheral holonomies are affine linear functions of X=(Z1,…,Zn,W1,…,Wn)TX=(Z_1,\ldots,Z_n,W_1,\ldots,W_n)^T.

Let Cλ,CμC_\lambda,C_\mu be the longitude and meridian coefficient rows, let RER_E be the edge-equation matrix, and set J2n=(0In−In0),U=(CλCμRE).J_{2n}=\begin{pmatrix}0&I_n\\-I_n&0\end{pmatrix},\qquad U=\begin{pmatrix}C_\lambda\\C_\mu\\R_E\end{pmatrix}. For a triangulated manifold with hh torus cusps, the original matrix identity is UJ2nUT=2(0Ih0−Ih00000).\boxed{U J_{2n}U^T =2\begin{pmatrix}0&I_h&0\\-I_h&0&0\\0&0&0\end{pmatrix}.}(16.31) This is [36, Theorem 2.2, equation (21)], in their longitude–meridian row order. They normalize the coefficient-row pairing as ⟨a,b⟩=12aJ2nbT\langle a,b\rangle=\tfrac12aJ_{2n}b^T. Equivalently, the unnormalized coefficient pairing of peripheral curves is twice their oriented intersection number; edge rows pair to zero with one another and with all peripheral rows. The topological interpretation is proved in their Section 3. A geometric construction of symplectic bases is given in [42].

The vanishing edge-edge pairings say that the linear constraints Poisson-commute. Since rank⁡RE=n−h\operatorname{rank}R_E=n-h, their coisotropic reduction has complex dimension 2h2h. Corollary 2.4 of [36] identifies the reduced form as Ω∂=12∑i=1h⁡dvi∧⁡dui,α∂=12∑i=1hvi⁡dui,⁡dα∂=Ω∂.\boxed{\Omega_\partial=\frac12\sum_{i=1}^h \mathop{}\!\mathrm dv_i\wedge\mathop{}\!\mathrm du_i,\qquad \alpha_\partial=\frac12\sum_{i=1}^h v_i\,\mathop{}\!\mathrm du_i, \qquad \mathop{}\!\mathrm d\alpha_\partial=\Omega_\partial.}(16.32) Locally near the regular geometric point, imposing the edge equations on the tetrahedral Lagrangian and reducing gives the geometric deformation Lagrangian ℒM\mathcal L_M in boundary holonomy space. For a modern formulation of the reduction, see [41]. The symplectic form lives on the ambient boundary phase space; its pullback to ℒM\mathcal L_M is zero.

16.10.2 The potential and the volume primitive

Writing v=v(u)v=v(u) on the geometric branch, Lagrangianity gives ∑i⁡dvi∧⁡dui=0⇔∂vi∂uj=∂vj∂ui.\sum_i\mathop{}\!\mathrm dv_i\wedge\mathop{}\!\mathrm du_i=0 \quad\Longleftrightarrow\quad \frac{\partial v_i}{\partial u_j} =\frac{\partial v_j}{\partial u_i}.(16.33) Thus ∑ivi⁡dui=⁡dF\sum_i v_i\,\mathop{}\!\mathrm du_i=\mathop{}\!\mathrm dF locally, and α∂|ℒM=⁡d(F/2)\alpha_\partial|_{\mathcal L_M}=\mathop{}\!\mathrm d(F/2). This is the reciprocity and potential statement of [36, Theorem 3]. For one cusp the existence of a primitive is automatic once v=v(u)v=v(u); the substantial content is the triangulation-level pairing and, for several cusps, the symmetry of the mixed derivatives. In the original normalization, ΦNZ=2F\Phi_{\mathrm{NZ}}=2F, whereas the complex-volume phase used above is Φ=Φ0+F/2\Phi=\Phi_0+F/2.

For one cusp write u=x+iy,v=r+is.u=x+iy,\qquad v=r+is. The real volume one-form is an exact modification of the imaginary part of the symplectic primitive: β=12(r⁡dy−x⁡ds)=ℑα∂−12⁡d(xs),⁡dβ=ℑΩ∂.\beta=\frac12(r\,\mathop{}\!\mathrm dy-x\,\mathop{}\!\mathrm ds) =\Im\alpha_\partial-\frac12\mathop{}\!\mathrm d(xs),\qquad \mathop{}\!\mathrm d\beta=\Im\Omega_\partial.(16.34) It is therefore closed on ℒM\mathcal L_M. Integrating it gives exactly (16.13). The factor 1/21/2 can also be seen from the leading–trailing angle variations: angular holonomy varies by twice the boundary intersection number, while volume varies by the real holonomy [37, Lemma 4.4 and Proposition 5.4]. The same pairing thus supplies the real optimization differential and the holomorphic generating function.

16.10.3 Filling as a canonical transformation

Choose ρ,σ∈ℤ\rho,\sigma\in\mathbb Z with pσ−qρ=1p\sigma-q\rho=1 and use the filling slope as the new meridian: a=pu+qv,b=ρu+σv,12⁡db∧⁡da=12⁡dv∧⁡du.a=pu+qv,\qquad b=\rho u+\sigma v,\qquad \frac12\mathop{}\!\mathrm db\wedge\mathop{}\!\mathrm da=\frac12\mathop{}\!\mathrm dv\wedge\mathop{}\!\mathrm du.(16.35) For q≠0q\ne0, the type-I generating function is G(u,a)=p4qu2−ua2q+σ4qa2.\boxed{G(u,a)=\frac{p}{4q}u^2-\frac{ua}{2q} +\frac{\sigma}{4q}a^2.}(16.36) Indeed, v=(a−pu)/qv=(a-pu)/q and b=(σa−u)/qb=(\sigma a-u)/q give the exact identity ⁡dG=12b⁡da−12v⁡du.\mathop{}\!\mathrm dG=\frac12b\,\mathop{}\!\mathrm da-\frac12v\,\mathop{}\!\mathrm du.(16.37) Thus Φ̃(a)=crit⁡u(Φ(u)+G(u,a))satisfiesΦ̃′(a)=b2.\widetilde\Phi(a)=\operatorname{crit}_u\bigl(\Phi(u)+G(u,a)\bigr) \quad\text{satisfies}\quad \widetilde\Phi'(a)=\frac b2. The stationary equation is a=pu+qva=pu+qv. Setting a=iθa=i\theta gives Φ̃(iθ)=Φ0+12𝒮p,q*(θ)−σθ24q.\widetilde\Phi(i\theta) =\Phi_0+\frac12\mathcal S^*_{p,q}(\theta) -\frac{\sigma\theta^2}{4q}.(16.38) The last term is real, hence invisible to the volume. At θ=2π\theta=2\pi it is −π2σ/q-\pi^2\sigma/q, the framing term in the Yoshida normalization used in [40, p. 456, formula preceding (5.9)]. The quadratic and linear terms of the surgery action are therefore fixed by a symplectic change of coordinates.

The complementary core holonomy bb is conjugate to the filling holonomy aa. Along a=iθa=i\theta, ⁡dℑΦ̃=ℑ(12bidθ)=12ℜb⁡dθ=−12ℓcore⁡dθ.\mathop{}\!\mathrm d\Im\widetilde\Phi =\Im\left(\frac12b\,i\mathop{}\!\mathrm d\theta\right) =\frac12\Re b\,\mathop{}\!\mathrm d\theta =-\frac12\ell_{\mathrm{core}}\,\mathop{}\!\mathrm d\theta. This gives Schläfli and the real source j=ℓcore/2j=\ell_{\mathrm{core}}/2 in the canonical coordinates.

On the canonical relation, G=(ab−uv)/4G=(ab-uv)/4, so Φ̃−ab4=Φ−uv4.\boxed{\widetilde\Phi-\frac{ab}{4} =\Phi-\frac{uv}{4}.}(16.39) Equivalently Φ̃NZ−ab=ΦNZ−uv\widetilde\Phi_{\mathrm{NZ}}-ab=\Phi_{\mathrm{NZ}}-uv, where Φ̃NZ=4(Φ̃−Φ0)\widetilde\Phi_{\mathrm{NZ}}=4(\widetilde\Phi-\Phi_0). The equality is local with consistently fixed logarithmic branches and additive constants. It explains why the combination of potential and peripheral product occurs in the complex-volume formula. The differential of the boxed expression is the invariant one-form 14(v⁡du−u⁡dv)\tfrac14(v\,\mathop{}\!\mathrm du-u\,\mathop{}\!\mathrm dv).

16.10.4 Covariance of the filling coefficients

The powers of p+qτp+q\tau in (16.17) also have a canonical-coordinate interpretation. Write the same geometric Lagrangian in the new coordinates as b(a)=τ̃a+c̃3a3+c̃5a5+O(a7).b(a)=\widetilde\tau a+\widetilde c_3a^3 +\widetilde c_5a^5+O(a^7). Using the inverse series of a=pu+qv(u)a=pu+qv(u) gives, with A=p+qτA=p+q\tau, τ̃=ρ+στp+qτ,ℑτ̃=ℑτ|p+qτ|2,c̃3=c3A4,c̃5=c5A6−3qc32A7.(16.40)\begin{aligned} \widetilde\tau&=\frac{\rho+\sigma\tau}{p+q\tau}, &\Im\widetilde\tau&=\frac{\Im\tau}{|p+q\tau|^2},\\ \widetilde c_3&=\frac{c_3}{A^4}, &\widetilde c_5&=\frac{c_5}{A^6}-\frac{3qc_3^2}{A^7}. \end{aligned} The cancellation in the cubic coefficient is σA−q(ρ+στ)=1.\sigma A-q(\rho+\sigma\tau)=1. It is exactly the symplectic determinant condition. Let F̃(0)=0\widetilde F(0)=0 and F̃′=b\widetilde F'=b. Since ℜa=0\Re a=0 on the cone locus, the real boundary correction in the new coordinates vanishes. Therefore Vp,q(θ)−V0=12ℑF̃(iθ)=−θ24ℑτ̃+θ48ℑc̃3−θ612ℑc̃5+⋯.V_{p,q}(\theta)-V_0 =\frac12\Im\widetilde F(i\theta) =-\frac{\theta^2}{4}\Im\widetilde\tau +\frac{\theta^4}{8}\Im\widetilde c_3 -\frac{\theta^6}{12}\Im\widetilde c_5+\cdots.(16.41) This is the previously computed volume expansion in filling coordinates. The cubic coefficient has a weight-−4-4 covariance law under a peripheral basis change; this alone does not assert that it is a modular form as a function of cusp shape. The pairing fixes the transformation laws, while the actual values of c3,c5,…c_3,c_5,\ldots describe nonlinear geometry of ℒM\mathcal L_M.

16.10.5 An exact Hessian and Monge–Ampere identity

There is a useful strengthening of (16.8). Eliminate internal angles at fixed peripheral angular holonomies, writing V¯(y,s)=maxPξ=(y,s)𝒱(ξ).\overline V(y,s)=\max_{P\xi=(y,s)}\mathscr V(\xi). All statements are local in the positive geometric neighborhood, where the maximum is interior and nondegenerate. Let K(ξ)=−D2𝒱(ξ)>0K(\xi)=-D^2\mathscr V(\xi)>0 at the maximizing point. The boundary intersection pairing gives rank⁡P=2\operatorname{rank}P=2, so the constrained implicit-function theorem supplies a unique nearby interior maximizer for every sufficiently small (y,s)(y,s). Stationarity in the internal directions enforces real edge gluing, so this maximizer lies on the same deformation branch v=v(u)v=v(u). The map u=x+iy↦(y,ℑv(u))u=x+iy\mapsto(y,\Im v(u)) is locally invertible because ℑv′(0)=B>0\Im v'(0)=B>0. It therefore identifies the angular boundary parameters with that geometric branch, rather than with an unrelated constrained family. The Schur-complement identity for the linear constraints is −D2V¯=(PK(ξ)−1PT)−1.-D^2\overline V=(P K(\xi)^{-1}P^T)^{-1}.(16.42) Set T=v′(u)=A0+iB0T=v'(u)=A_0+iB_0, with B0>0B_0>0 near the complete point. The volume differential and Cauchy–Riemann equations give V¯y=r2,V¯s=−x2,⁡ds=B0⁡dx+A0⁡dy,⁡dr=A0⁡dx−B0⁡dy.\overline V_y=\frac r2,\qquad \overline V_s=-\frac x2,\qquad \mathop{}\!\mathrm ds=B_0\mathop{}\!\mathrm dx+A_0\mathop{}\!\mathrm dy,\qquad \mathop{}\!\mathrm dr=A_0\mathop{}\!\mathrm dx-B_0\mathop{}\!\mathrm dy. Solving these two linear differential equations yields −D2V¯=12B0(|T|2−A0−A01),det⁡(−D2V¯)=14.\boxed{-D^2\overline V =\frac1{2B_0}\begin{pmatrix}|T|^2&-A_0\\-A_0&1\end{pmatrix}, \qquad \det(-D^2\overline V)=\frac14.}(16.43) Equivalently, PK(ξ)−1PT=2ℑv′(u)(1ℜv′(u)ℜv′(u)|v′(u)|2).P K(\xi)^{-1}P^T =\frac2{\Im v'(u)} \begin{pmatrix}1&\Re v'(u)\\ \Re v'(u)&|v'(u)|^2\end{pmatrix}.(16.44) The determinant-44 identity holds throughout this local branch. At u=0u=0 it reduces to the cusp formula already derived. For a filling path it gives the exact response Vp,q″(θ)=−ℑv′(uθ)2|p+qv′(uθ)|2,V_{p,q}''(\theta) =-\frac{\Im v'(u_\theta)} {2|p+qv'(u_\theta)|^2},(16.45) in agreement with (16.12).

For a geometric interpretation of the positive Hessian metric g=−D2V¯g=-D^2\overline V, multiplication by ii in the uu-coordinate induces, in coordinates (y,s)(y,s), JT=1B0(−A01−|T|2A0),JT2=−I.J_T=\frac1{B_0} \begin{pmatrix}-A_0&1\\-|T|^2&A_0\end{pmatrix}, \qquad J_T^2=-I. Then ωang=−12⁡dy∧⁡ds,g(X,Y)=ωang(X,JTY),g=B02(⁡dx2+⁡dy2).\omega_{\mathrm{ang}}=-\frac12\mathop{}\!\mathrm dy\wedge\mathop{}\!\mathrm ds,\qquad g(X,Y)=\omega_{\mathrm{ang}}(X,J_TY),\qquad g=\frac{B_0}{2}(\mathop{}\!\mathrm dx^2+\mathop{}\!\mathrm dy^2).(16.46) This real area form comes from the angular polarization and the positive complex tangent. It is not the pullback of Ω∂\Omega_\partial, which vanishes on the geometric Lagrangian. Nor has it been identified with the earlier Thurston–Deligne–Mostow complex hyperbolic metric.

For completeness, assume the same positive complete triangulation and regular deformation hypotheses with hh torus cusps, and use all 2h2h peripheral angular constraints. Their matrix PP has rank 2h2h by the boundary intersection pairing. Let T=(∂vi/∂uj)=A0+iB0T=(\partial v_i/\partial u_j)=A_0+iB_0. It is symmetric, and B0>0B_0>0 near the complete point. In coordinates (y,s)=(ℑu,ℑv)(y,s)=(\Im u,\Im v) the same calculation gives −D2V¯=12(B0+A0B0−1A0−A0B0−1−B0−1A0B0−1),det⁡(−D2V¯)=4−h.-D^2\overline V =\frac12\begin{pmatrix} B_0+A_0B_0^{-1}A_0&-A_0B_0^{-1}\\ -B_0^{-1}A_0&B_0^{-1} \end{pmatrix},\qquad \det(-D^2\overline V)=4^{-h}.(16.47) At the complete structure TT is diagonal, with the individual cusp shapes on the diagonal. Coupling between distinct cusps appears in higher derivatives of the even Neumann–Zagier potential, for example through terms ui2uj2u_i^2u_j^2.

16.10.6 The quantum Gaussian as a half-density transformation

Let a geometric boundary state have leading form A0(u)eΦ(u)/ℏA_0(u)e^{\Phi(u)/\hbar}, with Φ′=v/2\Phi'=v/2. A quantization of the canonical transformation uses the exponential kernel eG(u,a)/ℏe^{G(u,a)/\hbar} and its mixed-derivative normalization. The relevant derivatives are −Gua=12q,(Φ+G)uu=p+qv′(u)2q.-G_{ua}=\frac1{2q},\qquad (\Phi+G)_{uu}=\frac{p+qv'(u)}{2q}. The kernel normalization divided by the stationary Gaussian therefore has the dependence −Gua(Φ+G)uu=1p+qv′(u)=⁡du⁡da.\boxed{\sqrt{\frac{-G_{ua}}{(\Phi+G)_{uu}}} =\frac1{\sqrt{p+qv'(u)}} =\sqrt{\frac{\mathop{}\!\mathrm du}{\mathop{}\!\mathrm da}}.}(16.48) Universal powers of ℏ\hbar, phases, and square-root branches are fixed by the chosen integral convention. The displayed dependence is the transformation law for a half-density along ℒM\mathcal L_M. It is exactly the law obeyed by the inverse square root of peripheral torsion in (16.25). The extra 2sinh⁡(b/2)2\sinh(b/2) factor comes from the solid torus and is additional input. Explicit quantum filling kernels appear in [39, equations (12)–(14)].

The symplectic structure fixes the conjugate variables, the canonical generating function, and this Gaussian Jacobian. It does not select the integration cycle or prove that the geometric contribution survives cancellation in the exact quantum invariant. The analytic hypotheses in Proposition 16.2 remain necessary for that conclusion.