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Lagrangian Submanifolds, Generating Functions, and Semiclassical Phases

A Lagrangian submanifold is a half-dimensional submanifold on which the symplectic form vanishes. That compact definition unifies three objects that can look unrelated in coordinates: a family of classical solutions, the canonical relation defined by time evolution, and the phase carried by a semiclassical wave. A scalar generating function is only a local coordinate description of that geometry. It can become multivalued or singular when a projection develops a caustic even though the Lagrangian submanifold itself remains smooth.

This page develops that distinction carefully. It fixes the signs in endpoint generating functions, explains why auxiliary phase variables survive caustics, and derives the Van Vleck and Maslov data of semiclassical propagation. The discussion is finite-dimensional. Extending it to a QFT functional integral requires separate choices of regulator, measure, gauge treatment, and integration cycle.

Required background. Symplectic Forms, Hamiltonian Vector Fields, and Poisson Brackets supplies symplectic complements, Hamiltonian flow, and the canonical two-form sign convention; Stationary Phase, Coalescing Saddles, and Stokes Geometry supplies the regulated Fresnel factor, the Airy fold, and the rule that only contour-accessible stationary points contribute.

Let QQ be an nn-dimensional configuration manifold. In canonical coordinates on TQT^*Q, this page uses

θ=padqa,ω=dθ=dqadpa.\theta=p_a\,\mathrm dq^a, \qquad \omega=-\mathrm d\theta =\mathrm dq^a\wedge\mathrm dp_a.

The bar on a symplectic manifold reverses its symplectic form:

(M,ω)=(M,ω).\overline{(M,\omega)}=(M,-\omega).

We take >0\hbar>0 and use e+iΦ/e^{+i\Phi/\hbar} for oscillatory phases. Reversing that exponential conjugates every Fresnel and Maslov phase below.

Let ι:L(M,ω)\iota:L\hookrightarrow(M,\omega) be an embedded submanifold of a 2n2n-dimensional symplectic manifold. It is Lagrangian when

dimL=n,ιω=0.\dim L=n, \qquad \iota^*\omega=0.

Equivalently, at every xLx\in L,

TxL=(TxL)ω,T_xL=(T_xL)^\omega,

where the right-hand side is the symplectic complement. The vanishing condition alone says that LL is isotropic; the dimension condition makes it maximally isotropic. A merely half-dimensional submanifold need not be Lagrangian.

Cotangent bundles provide the basic examples.

For a one-form αΩ1(Q)\alpha\in\Omega^1(Q), let

sα:QTQ,q(q,αq).s_\alpha:Q\longrightarrow T^*Q, \qquad q\longmapsto(q,\alpha_q).

Because sαθ=αs_\alpha^*\theta=\alpha,

sαω=dα.s_\alpha^*\omega=-\mathrm d\alpha.

The graph of α\alpha is therefore Lagrangian exactly when α\alpha is closed. On a contractible coordinate neighborhood, α=dS\alpha=\mathrm dS, so the graph has the familiar form

pa=Sqa.p_a=\frac{\partial S}{\partial q^a}.

The local qualifier matters. For example, on Q=S1Q=S^1, the section pdφ=cdφp\,\mathrm d\varphi=c\,\mathrm d\varphi is Lagrangian, but for c0c\neq0 it has no single-valued real generating function on the whole circle. Its period is 2πc2\pi c. Lagrangian implies locally exact in a cotangent chart; it does not imply a global scalar SS.

These Lagrangian graph and local generating-function statements are treated in Cannas da Silva 2001, §§ 3.2–4.2, pp. 16–23, PDF.

A cotangent fiber TqQT_q^*Q is Lagrangian but is not a graph over any open subset of QQ. More generally, if YQY\subset Q is a submanifold, its conormal bundle

NY={(q,p)TQ:qY, p(v)=0 for every vTqY}N^*Y = \left\{ (q,p)\in T^*Q: q\in Y,\ p(v)=0\ \text{for every }v\in T_qY \right\}

is Lagrangian. Indeed, θ\theta vanishes on NYN^*Y, and

dimNY=dimY+codimY=n.\dim N^*Y = \dim Y+\operatorname{codim}Y =n.

These examples already show why a single position-space function cannot be the definition: some perfectly regular Lagrangians are vertical, and others have nontrivial topology.

A canonical relation from (Mi,ωi)(M_i,\omega_i) to (Mf,ωf)(M_f,\omega_f) is a Lagrangian submanifold

CMi×MfC\subset\overline{M_i}\times M_f

for the product form

Ω=ωi+ωf.\Omega=-\omega_i+\omega_f.

A canonical transformation F:MiMfF:M_i\to M_f gives the special case C=ΓFC=\Gamma_F, its graph. Pulling back the product form to that graph gives

ΩΓF=ωi+Fωf,\Omega|_{\Gamma_F} = -\omega_i+F^*\omega_f,

so ΓF\Gamma_F is Lagrangian exactly when FF is symplectic. A general canonical relation need not be the graph of a single-valued map; this flexibility is essential at caustics and in composition.

For generating families, caustics, Maslov correction, and canonical relations, see Bates and Weinstein 1997, §§ 4.2–4.3, pp. 41–55, and § 5.2, pp. 76–78, PDF.

Suppose now that Mi=TQiM_i=T^*Q_i and Mf=TQfM_f=T^*Q_f. Define

β=θfθi=pfdqfpidqi.\beta=\theta_f-\theta_i = p_f\,\mathrm dq_f-p_i\,\mathrm dq_i.

Since

Ω=dβ,\Omega=-\mathrm d\beta,

the restriction βC\beta|_C is closed. It is locally exact, so on CC there is a local function SS satisfying

dS=pfdqfpidqi.\mathrm dS = p_f\,\mathrm dq_f-p_i\,\mathrm dq_i.

This does not yet make SS a function of the two endpoints. That step requires the projection

πif:CQi×Qf\pi_{if}:C\longrightarrow Q_i\times Q_f

to be a local diffeomorphism. In such a type-I chart,

S=S(qf,qi),S=S(q_f,q_i),

and coefficient matching fixes the signs:

pf=Sqf,pi=Sqi.\boxed{ p_f=\frac{\partial S}{\partial q_f}, \qquad p_i=-\frac{\partial S}{\partial q_i}. }

The minus sign on the initial momentum comes from the barred initial phase space. It is not optional notation.

When the endpoint projection fails, another polarization may still work. Here a polarization means a choice of which half of the canonical variables serve as independent coordinates. For example, if qiq_i can be eliminated in favor of pip_i, the (qf,pi)(q_f,p_i) choice is described by the partial Legendre transform

F2(qf,pi)=S(qf,qi)+piqiF_2(q_f,p_i) = S(q_f,q_i)+p_iq_i

obeys

dF2=pfdqf+qidpi.\mathrm dF_2 = p_f\,\mathrm dq_f+q_i\,\mathrm dp_i.

Thus pf=qfF2p_f=\partial_{q_f}F_2 and qi=piF2q_i=\partial_{p_i}F_2. Changing polarization changes the coordinate chart, not the underlying canonical relation.

Generating families with auxiliary variables

Section titled “Generating families with auxiliary variables”

Ordinary generating functions are not flexible enough near a caustic. Let ϑ=(ϑ1,,ϑk)\vartheta=(\vartheta^1,\ldots,\vartheta^k) be auxiliary variables and let

Φ:Q×RkR.\Phi:Q\times\mathbb R^k\longrightarrow\mathbb R.

Its fiber-critical set is

CΦ={(q,ϑ):ϑαΦ(q,ϑ)=0}.C_\Phi = \left\{ (q,\vartheta): \partial_{\vartheta^\alpha}\Phi(q,\vartheta)=0 \right\}.

The phase is nondegenerate in the relevant sense when

d(ϑ1Φ),,d(ϑkΦ)\mathrm d(\partial_{\vartheta^1}\Phi),\ldots, \mathrm d(\partial_{\vartheta^k}\Phi)

are linearly independent on CΦC_\Phi. This regular-value condition makes CΦC_\Phi a smooth nn-dimensional manifold. The map

ιΦ:CΦTQ,(q,ϑ)(q,qΦ(q,ϑ))\iota_\Phi:C_\Phi\longrightarrow T^*Q, \qquad (q,\vartheta) \longmapsto \left(q,\partial_q\Phi(q,\vartheta)\right)

is then a Lagrangian immersion. The proof contains the main idea. On CΦC_\Phi,

ιΦθ=qΦdq=d ⁣(ΦCΦ),\begin{aligned} \iota_\Phi^*\theta &= \partial_q\Phi\,\mathrm dq\\ &= \mathrm d\!\left(\Phi|_{C_\Phi}\right), \end{aligned}

because ϑΦ=0\partial_\vartheta\Phi=0 there. Hence ιΦω=0\iota_\Phi^*\omega=0, and the regularity condition supplies the correct dimension and immersion rank. After restricting to a neighborhood on which ιΦ\iota_\Phi is an embedding, its image is an exact Lagrangian.

The condition is not

detΦϑϑ0.\det\Phi_{\vartheta\vartheta}\neq0.

That stronger condition says that the stationary auxiliary variable can be solved smoothly as a function of qq. It is precisely what can fail at a caustic while the full phase remains nondegenerate. Conversely, every smooth Lagrangian in a cotangent bundle has a local generating-family description after sufficiently many auxiliary variables are introduced. A global description may still require several charts and transition data. The local existence statement is proved in Guillemin and Sternberg 2010, §§ 5.1–5.2, pp. 133–138, and § 5.9, pp. 153–157, PDF.

Consider

Φ(x,ϑ)=xϑϑ33.\Phi(x,\vartheta) = x\vartheta-\frac{\vartheta^3}{3}.

The fiber-critical equation and its differential are

ϑΦ=xϑ2=0,d(ϑΦ)=dx2ϑdϑ.\partial_\vartheta\Phi=x-\vartheta^2=0, \qquad \mathrm d(\partial_\vartheta\Phi) = \mathrm dx-2\vartheta\,\mathrm d\vartheta.

The differential never vanishes, including at ϑ=0\vartheta=0. The generated Lagrangian is therefore the smooth parabola

Λ={(x,p):x=p2},p=xΦ=ϑ.\Lambda = \left\{ (x,p):x=p^2 \right\}, \qquad p=\partial_x\Phi=\vartheta.

Along its critical set,

ΦCΦ=23ϑ3,pdx=d ⁣(23ϑ3).\Phi|_{C_\Phi} = \frac23\vartheta^3, \qquad p\,\mathrm dx = \mathrm d\!\left(\frac23\vartheta^3\right).

The projection ΛRx\Lambda\to\mathbb R_x folds at ϑ=0\vartheta=0. For x>0x>0 it has two graph charts,

p±=±x,S±(x)=±23x3/2,p_\pm=\pm\sqrt{x}, \qquad S_\pm(x)=\pm\frac23x^{3/2},

but neither graph extends smoothly through x=0x=0. The auxiliary phase does.

The associated Abel-prescribed oscillatory integral is

I(x)=limϵ0Reϵϑ2exp ⁣[i(xϑϑ33)]dϑ=2π1/3Ai ⁣(x2/3).\begin{aligned} I_\hbar(x) &= \lim_{\epsilon\downarrow0} \int_{\mathbb R} e^{-\epsilon\vartheta^2} \exp\!\left[ \frac{i}{\hbar} \left( x\vartheta-\frac{\vartheta^3}{3} \right) \right]\mathrm d\vartheta\\ &= 2\pi\hbar^{1/3} \operatorname{Ai}\!\left( -\frac{x}{\hbar^{2/3}} \right). \end{aligned}

For fixed x>0x>0, stationary phase at ϑ±=±x\vartheta_\pm=\pm\sqrt{x} gives

I(x)2πx1/4cos ⁣(2x3/23π4).I_\hbar(x) \sim 2\sqrt{\pi\hbar}\,x^{-1/4} \cos\!\left( \frac{2x^{3/2}}{3\hbar}-\frac{\pi}{4} \right).

The two graph amplitudes diverge as x1/4x^{-1/4} when the fold is approached, whereas the Airy expression remains finite on the x=O(2/3)x=O(\hbar^{2/3}) scale. The divergence belongs to the projected graph chart, not to Λ\Lambda or to the uniform oscillatory integral. The Airy integral normalization and the asymptotic matching used here are recorded in NIST DLMF 2026, §§ 9.5 and 9.7.

A local semiclassical state associated with a Lagrangian can be written as

u(q)=(2π)k/2a(q,ϑ;)eiΦ(q,ϑ)/dkϑ,u_\hbar(q) = (2\pi\hbar)^{-k/2} \int a(q,\vartheta;\hbar) e^{i\Phi(q,\vartheta)/\hbar} \,\mathrm d^k\vartheta,

with a specified contour or oscillatory prescription. Its fiber-critical points map to

(q,p=qΦ)Λ.\left(q,p=\partial_q\Phi\right)\in\Lambda.

If Φϑϑ\Phi_{\vartheta\vartheta} is invertible, stationary phase removes the auxiliary variables locally. For the convention used here, a real auxiliary Hessian HH contributes

eiπsigH/41detHe^{i\pi\operatorname{sig}H/4} \frac{1}{\sqrt{|\det H|}}

apart from powers of 2π2\pi\hbar and the transformed amplitude. Different phase functions can describe the same Lagrangian, so these signature factors must be included in their transition rules.

The resulting integer phase bookkeeping is the Maslov index. With the short-time propagator chosen as the baseline, this page denotes it by ν\nu. At a simple crossing where one Hessian eigenvalue changes from positive to negative,

eiπ/4e+iπ/4=eiπ/2.\frac{e^{-i\pi/4}}{e^{+i\pi/4}} = e^{-i\pi/2}.

Thus that crossing contributes π/2-\pi/2 and increases ν\nu by one; the reverse crossing has the opposite sign. For ordinary positive-kinetic mechanical propagation forward in time, these crossings are conjugate points: losses of rank of the endpoint map from initial momentum to final position, counted with the rank loss as multiplicity. In a general Hamiltonian flow, the crossing form determines the sign instead. Reversing the oscillatory sign or the index orientation reverses the phase rule. An unqualified formula involving a symbol μ\mu is therefore incomplete unless its baseline and crossing convention are stated.

Geometrically, the Maslov index records how the tangent Lagrangian planes meet the locus where the chosen projection becomes singular. It is what lets local phase charts glue into a global semiclassical object even when no global single-valued S(q)S(q) exists.

Hamilton’s principal function and the propagator

Section titled “Hamilton’s principal function and the propagator”

Let a regular classical trajectory γ\gamma join qiq_i to qfq_f in time TT. Its on-shell action is

Sγ(qf,qi;T)=0T(paq˙aH(q,p))dt.S_\gamma(q_f,q_i;T) = \int_0^T \left( p_a\dot q^a-H(q,p) \right)\mathrm dt.

Varying the endpoints at fixed TT gives

dSγ=pfdqfpidqi.\mathrm dS_\gamma = p_f\,\mathrm dq_f-p_i\,\mathrm dq_i.

For an autonomous Hamiltonian, varying the final time also gives

SγT+H ⁣(qf,Sγqf)=0.\frac{\partial S_\gamma}{\partial T} + H\!\left( q_f,\frac{\partial S_\gamma}{\partial q_f} \right) =0.

Hamilton’s principal function is therefore a type-I generating function for the graph of Hamiltonian time evolution wherever the endpoint projection is regular.

Choose endpoint coordinate charts and refer the kernel to their coordinate measures. For isolated classical trajectories, define the Van Vleck matrix

Dγ=2Sγqfqi.D_\gamma = -\frac{\partial^2S_\gamma} {\partial q_f\,\partial q_i}.

The real-time quantum propagator is the position-space kernel

K(qf,qi;T)=qf|eiH^T/|qi.K(q_f,q_i;T) = \left\langle q_f \middle| e^{-i\widehat H T/\hbar} \middle| q_i \right\rangle.

Invariantly, its leading amplitude is a bi-half-density; the determinant below is that amplitude’s representative in the chosen coordinates.

With the square-root branch fixed by the positive short-time limit, the local semiclassical propagator is

Ksc(qf,qi;T)=1(2πi)n/2γdetDγ1/2×exp ⁣[iSγ(qf,qi;T)iπ2νγ].\boxed{ \begin{aligned} K_{\mathrm{sc}}(q_f,q_i;T) ={}& \frac{1}{(2\pi i\hbar)^{n/2}} \sum_\gamma \left| \det D_\gamma \right|^{1/2}\\ &\times \exp\!\left[ \frac{i}{\hbar}S_\gamma(q_f,q_i;T) -\frac{i\pi}{2}\nu_\gamma \right]. \end{aligned} }

The sum is over trajectories compatible with the prescribed boundary conditions. It is not a sum over every formal solution after complexification.

The determinant has a useful geometric interpretation. Parameterize the flow graph by (qi,pi)(q_i,p_i) and put

Bγ=qfpiqi.B_\gamma = \left. \frac{\partial q_f}{\partial p_i} \right|_{q_i}.

Where the type-I chart exists,

detDγ=detBγ1.\left|\det D_\gamma\right| = \left|\det B_\gamma\right|^{-1}.

A configuration-space caustic occurs when detBγ=0\det B_\gamma=0. Consequently the type-I Van Vleck matrix does not vanish there: it ceases to be a regular coordinate expression and typically diverges on approach. One must retain an auxiliary phase, change polarization, or use a uniform canonical integral. The relation among the Van Vleck determinant, Jacobi fields, caustics, and Morse-index phases is developed in Horváthy 2011, §§ 6–7, arXiv pp. 11–14.

For

H=p22m+12mω2q2,m,ω>0,H=\frac{p^2}{2m}+\frac12m\omega^2q^2, \qquad m,\omega>0,

and sinωT0\sin\omega T\neq0, the unique endpoint trajectory is

qcl(t)=qisin ⁣(ω(Tt))+qfsin(ωt)sin(ωT).q_{\mathrm{cl}}(t) = \frac{ q_i\sin\!\left(\omega(T-t)\right) + q_f\sin(\omega t) }{ \sin(\omega T) }.

Its action is

Scl=mω2sinωT[(qf2+qi2)cosωT2qfqi].S_{\mathrm{cl}} = \frac{m\omega}{2\sin\omega T} \left[ (q_f^2+q_i^2)\cos\omega T -2q_fq_i \right].

Direct differentiation checks all signs:

pf=mω(qfcosωTqi)sinωT,pi=mω(qfqicosωT)sinωT,D=2Sclqfqi=mωsinωT.\begin{aligned} p_f &= \frac{m\omega(q_f\cos\omega T-q_i)} {\sin\omega T},\\ p_i &= \frac{m\omega(q_f-q_i\cos\omega T)} {\sin\omega T},\\ D &= -\frac{\partial^2S_{\mathrm{cl}}} {\partial q_f\,\partial q_i} = \frac{m\omega}{\sin\omega T}. \end{aligned}

Meanwhile,

B=qfpiqi=sinωTmω,D=B1.B = \left. \frac{\partial q_f}{\partial p_i} \right|_{q_i} = \frac{\sin\omega T}{m\omega}, \qquad D=B^{-1}.

This quadratic system is especially valuable because the semiclassical answer is exact. For T>0T>0 away from a caustic, let

N=ωTπ.N=\left\lfloor\frac{\omega T}{\pi}\right\rfloor.

Then

K(qf,qi;T)=mω2πisinωTexp ⁣[iScliπN2].\boxed{ K(q_f,q_i;T) = \sqrt{ \frac{m\omega} {2\pi i\hbar\,|\sin\omega T|} } \exp\!\left[ \frac{i}{\hbar}S_{\mathrm{cl}} -\frac{i\pi N}{2} \right]. }

At T=Nπ/ωT=N\pi/\omega, with N1N\geq1, the coordinate formula must be replaced by its distributional limit:

K ⁣(qf,qi;Nπω)=eiπN/2δ ⁣(qf(1)Nqi).\boxed{ K\!\left( q_f,q_i;\frac{N\pi}{\omega} \right) = e^{-i\pi N/2} \delta\!\left(q_f-(-1)^Nq_i\right). }

Thus the first caustic gives iδ(qf+qi)-i\,\delta(q_f+q_i), while one full period gives δ(qfqi)-\delta(q_f-q_i). The vanishing of BB, the divergence of DD, the π/2-\pi/2 phase increment, and the delta-supported exact kernel are four views of the same projection failure. The exact propagator both between and at harmonic-oscillator caustics is checked independently in Funahashi 2010, pp. 2 and 6–8.

Let

C12M1×M2,C23M2×M3.C_{12}\subset\overline{M_1}\times M_2, \qquad C_{23}\subset\overline{M_2}\times M_3.

Their set-theoretic composition matches the two copies of the intermediate phase space and then forgets them. It is Lagrangian only under suitable transversality or clean-intersection hypotheses, together with a well-behaved projection of the matched set. Without those hypotheses, the result can be immersed, multiply covered, or singular.

In compatible type-I charts, this geometric operation becomes

S13(q3,q1)=statq2[S23(q3,q2)+S12(q2,q1)].S_{13}(q_3,q_1) = \operatorname*{stat}_{q_2} \left[ S_{23}(q_3,q_2)+S_{12}(q_2,q_1) \right].

The stationary equation is

q2S23+q2S12=0.\partial_{q_2}S_{23} + \partial_{q_2}S_{12} =0.

It says that the initial momentum of the second relation equals the final momentum of the first. Several stationary values of q2q_2 produce several branches; a degenerate stationary value signals that the scalar composition formula needs a uniform phase description. This is the geometric reason that semiclassical propagators compose by integrating over an intermediate configuration and then applying stationary phase.

For a field theory, the classical action plays the role of a phase functional, and its second variation supplies the formal analogue of the finite-dimensional Hessian and Van Vleck data. That analogy is useful but incomplete. Functional determinants require regularization and renormalization; gauge directions and collective coordinates must be separated; boundary conditions select the operator domain; and negative modes do not by themselves determine an integration cycle.

Likewise, a middle-dimensional contour in a complexified field space is not automatically the same object as a real Lagrangian submanifold in a cotangent phase space. A symplectic or Kähler structure, a reality condition, and a contour prescription must first be specified. The finite-dimensional Airy model and Chern–Simons application in Witten 2010, §§ 2.1–2.3, pp. 8–11 show how thimble coefficients depend on the original integration cycle, but that is additional global data rather than a consequence of the local generating-function equations.

Negative Modes and Instability Indices develops the physical Morse-index, contour-deformation, and instability questions. The present page supplies its finite-dimensional phase geometry; it does not preselect the physical saddle sectors.

Treating half-dimensional as sufficient. A half-dimensional submanifold is Lagrangian only if the symplectic form also restricts to zero.

Assuming every Lagrangian is a global graph. Cotangent fibers, conormals, folded projections, and closed nonexact sections are counterexamples. Use local charts or generating families.

Losing the initial minus sign. For CMi×MfC\subset\overline{M_i}\times M_f, dS=pfdqfpidqi\mathrm dS=p_f\,\mathrm dq_f-p_i\,\mathrm dq_i. Reversing the product order or the symplectic convention changes the displayed formulas and must be stated.

Calling a phase degenerate when its fiber Hessian vanishes. The relevant condition is independence of the full differentials d(ϑαΦ)\mathrm d(\partial_{\vartheta^\alpha}\Phi). The fold phase remains nondegenerate at its caustic.

Saying the Van Vleck determinant vanishes at a caustic. The endpoint Jacobian det(qf/pi)\det(\partial q_f/\partial p_i) vanishes. Its inverse determinant in the type-I Van Vleck formula becomes singular.

Identifying a phase-space Lagrangian with a QFT integration cycle. The two can be related only after additional geometric and analytic structures are specified.

1. A Lagrangian with no global scalar phase

Section titled “1. A Lagrangian with no global scalar phase”

On TS1T^*S^1, consider the section α=cdφ\alpha=c\,\mathrm d\varphi. Show that its graph is Lagrangian and decide when it has a single-valued real generating function on all of S1S^1.

Solution

Although φ\varphi itself is only a local real coordinate, the forms dφ\mathrm d\varphi on angular charts agree on overlaps and define a global one-form. Because

dα=cd(dφ)=0,\mathrm d\alpha = c\,\mathrm d(\mathrm d\varphi) =0,

the graph is Lagrangian. If α=dS\alpha=\mathrm dS globally, its integral around the circle must vanish. Instead,

S1α=2πc.\oint_{S^1}\alpha=2\pi c.

Therefore a single-valued real SS exists only for c=0c=0. Every sufficiently small angular chart still has the local primitive S=cφS=c\varphi.

For a free particle in one dimension,

S(qf,qi;T)=m(qfqi)22T,T>0.S(q_f,q_i;T) = \frac{m(q_f-q_i)^2}{2T}, \qquad T>0.

Use the canonical-relation convention to recover the initial and final momenta.

Solution

Differentiate with respect to the final endpoint:

pf=Sqf=m(qfqi)T.p_f = \frac{\partial S}{\partial q_f} = \frac{m(q_f-q_i)}{T}.

At the initial endpoint,

pi=Sqi=m(qfqi)T.p_i = -\frac{\partial S}{\partial q_i} = \frac{m(q_f-q_i)}{T}.

The two momenta agree, as free motion requires. Omitting the initial minus sign would incorrectly reverse pip_i.

For

Φ(x,ϑ)=xϑϑ33,\Phi(x,\vartheta) = x\vartheta-\frac{\vartheta^3}{3},

find the critical set, its generated Lagrangian, and the point where the position projection fails. Why is the phase nevertheless nondegenerate?

Solution

The fiber-critical equation is xϑ2=0x-\vartheta^2=0, so

CΦ={x=ϑ2}.C_\Phi=\{x=\vartheta^2\}.

Since p=xΦ=ϑp=\partial_x\Phi=\vartheta, the image is

Λ={x=p2}.\Lambda=\{x=p^2\}.

The derivative of x=ϑ2x=\vartheta^2 vanishes at ϑ=0\vartheta=0, so the projection to xx folds there. However,

d(ϑΦ)=dx2ϑdϑ\mathrm d(\partial_\vartheta\Phi) = \mathrm dx-2\vartheta\,\mathrm d\vartheta

never vanishes. The fiber-critical set and the generated Lagrangian remain smooth even though Φϑϑ=0\Phi_{\vartheta\vartheta}=0 at the fold.

For the harmonic oscillator, compute

B=qfpiqiB=\left.\frac{\partial q_f}{\partial p_i}\right|_{q_i}

from the classical solution. What happens to BB, the type-I Van Vleck matrix, and the exact kernel at T=π/ωT=\pi/\omega?

Solution

The initial-value solution is

qf=qicosωT+pimωsinωT,q_f = q_i\cos\omega T + \frac{p_i}{m\omega}\sin\omega T,

so

B=sinωTmω.B=\frac{\sin\omega T}{m\omega}.

At T=π/ωT=\pi/\omega, B=0B=0: all initial momenta focus at qf=qiq_f=-q_i. Away from the caustic,

D=B1=mωsinωT,D=B^{-1} = \frac{m\omega}{\sin\omega T},

so the type-I expression diverges rather than vanishes. Its correct distributional limit is

K ⁣(qf,qi;πω)=iδ(qf+qi).K\!\left(q_f,q_i;\frac{\pi}{\omega}\right) = -i\,\delta(q_f+q_i).

The factor i=eiπ/2-i=e^{-i\pi/2} is the first Maslov increment in the convention of this page.

A Lagrangian submanifold is the invariant object; ordinary generating functions, mixed polarizations, and auxiliary phases are local descriptions. Canonical evolution becomes a Lagrangian relation with fixed endpoint signs. When a position projection folds, graph phases and type-I amplitudes fail while a nondegenerate auxiliary phase can remain smooth. Stationary-phase transition factors then assemble into Maslov data, and the Van Vleck determinant measures the inverse endpoint Jacobian. The harmonic oscillator checks these statements against an exact kernel, including its distributional value at a caustic.

WKB and Eikonal Methods and Turning-Point Matching applies the same Lagrangian projection and Airy-fold geometry to differential equations. Stationary Phase, Coalescing Saddles, and Stokes Geometry develops the local asymptotics behind the Fresnel and Airy formulas. The later Negative Modes and Instability Indices page supplies the field-theoretic stability and contour analysis that the finite-dimensional construction deliberately leaves open.