Free-Particle and Harmonic-Oscillator Path Integrals

The path integral is a formal object until you can actually do one, and there are exactly two nontrivial cases where the sum over infinitely many paths collapses to a single closed formula: the free particle and the harmonic oscillator. Both are Gaussian — the action is quadratic in the path — so the functional integral is an infinite-dimensional Gaussian integral, and Gaussian integrals are the one kind we can always evaluate. The payoff is not just two propagators. It is a template: for any quadratic-in-fluctuations problem, the answer has the shape K=(prefactor) eiScl/ℏK=(\text{prefactor})\,e^{iS_{\rm cl}/\hbar}, where SclS_{\rm cl} is the action of the classical path and the prefactor is a determinant that counts how neighbouring classical paths spread. That prefactor has a name and a beautiful meaning: the Van Vleck–Pauli–Morette determinant, (1/2πiℏ) ∂2Scl/∂xi∂xf\sqrt{(1/2\pi i\hbar)\,\partial^2 S_{\rm cl}/\partial x_i\partial x_f}. It measures the density of classical trajectories arriving at xfx_f — where they bunch up, the amplitude is large. And it has a spectacular failure mode. For the oscillator the prefactor is mω/2πiℏsin⁡ωT\sqrt{m\omega/2\pi i\hbar\sin\omega T}, which diverges every half-period, at ωT=nπ\omega T=n\pi. Those are caustics: instants when every trajectory launched from xix_i refocuses to a single point, the classical density blows up, and the semiclassical formula breaks. The phase the propagator picks up crossing each caustic is exactly the Maslov phase that the WKB chapter charges for a turning point. You are ready: you know Gaussian integrals, the free kernel, and the oscillator spectrum En=ℏω(n+12)E_n=\hbar\omega(n+\tfrac12). Here we evaluate both path integrals exactly, read off the Van Vleck prefactor, locate the caustics, and — as a stringent consistency check — resum the oscillator kernel into its energy eigenstates and recover that same spectrum. The caustics we find here are the thread that reappears as the Maslov index in the last article of the chapter.

Key takeaways
  • Both exactly-solvable path integrals have the semiclassical form K=12πiℏ∂2Scl∂xi∂xf  eiScl/ℏK=\sqrt{\dfrac{1}{2\pi i\hbar}\dfrac{\partial^2 S_{\rm cl}}{\partial x_i\partial x_f}}\;e^{iS_{\rm cl}/\hbar} — the Van Vleck–Pauli–Morette prefactor times the classical phase.
  • Free particle: K0=m/2πiℏT eim(xf−xi)2/2ℏTK_0=\sqrt{m/2\pi i\hbar T}\,e^{im(x_f-x_i)^2/2\hbar T}, with Scl=m(Δx)2/2TS_{\rm cl}=m(\Delta x)^2/2T.
  • Oscillator: K=mω2πiℏsin⁡ωTexp⁡ ⁣[imω2ℏsin⁡ωT((xi2+xf2)cos⁡ωT−2xixf)]K=\sqrt{\dfrac{m\omega}{2\pi i\hbar\sin\omega T}}\exp\!\Big[\dfrac{im\omega}{2\hbar\sin\omega T}\big((x_i^2+x_f^2)\cos\omega T-2x_ix_f\big)\Big].
  • The prefactor diverges at caustics ωT=nπ\omega T=n\pi: every path refocuses, the classical density blows up, and the propagator picks up a Maslov phase.
  • Resumming the oscillator kernel over its eigenstates returns K=∑ne−i(n+12)ωTψn(xf)ψn∗(xi)K=\sum_n e^{-i(n+\frac12)\omega T}\psi_n(x_f)\psi_n^*(x_i) — an independent recovery of En=ℏω(n+12)E_n=\hbar\omega(n+\tfrac12).
  • KEY IDEA: for a quadratic action the path integral is a Gaussian and collapses to (Van Vleck prefactor) × eiScl/ℏe^{iS_{\rm cl}/\hbar}; the prefactor's zeros of sin⁡ωT\sin\omega T are caustics — the seeds of the Maslov index.
The core insight

For any action quadratic in the path, the path integral equals the Van Vleck prefactor (1/2πiℏ) ∂2Scl/∂xi∂xf\sqrt{(1/2\pi i\hbar)\,\partial^2 S_{\rm cl}/\partial x_i\partial x_f} times eiScl/ℏe^{iS_{\rm cl}/\hbar}; its divergences are the caustics where classical trajectories refocus.

Where this lives today

The Van Vleck prefactor and its caustics are the backbone of semiclassical physics. In molecular dynamics, semiclassical initial-value representations propagate wavepackets using exactly Van Vleck eiScl/ℏ\sqrt{\text{Van Vleck}}\,e^{iS_{\rm cl}/\hbar} summed over classical trajectories, with the Maslov phase tracked as each trajectory passes a caustic — this is how large molecules' vibrational spectra are computed without solving the full Schrödinger equation. The same caustics are visible optics: the bright cusp at the bottom of a teacup and the shimmering network on a pool floor are light's Van Vleck determinant diverging, and the finite brightness there (rather than true infinity) is diffraction smoothing the caustic exactly as it smooths the quantum propagator.

The physical picture

The free particle is the warm-up: released from xix_i with a spread of momenta, the classical trajectories fan out and never come back, so the amplitude to arrive at xfx_f is a smooth spreading Gaussian — this is the "spreading Gaussian kernel" that The Quantum Propagator flagged as belonging to this article. The oscillator is where it gets dramatic. Every trajectory launched from xix_i, whatever its initial momentum, has the same period 2π/ω2\pi/\omega. So after a half period, ωT=π\omega T=\pi, all of them arrive back at −xi-x_i simultaneously, no matter how they started. The bundle of paths, spread out across the well, collapses to a single point.

Figure
Oscillator trajectories refocus at half-period caustics
x(t) from x_i with different momenta — all refocus at ωT = π, 2π, … x_i caustic ωT=π caustic ωT=2π

At that refocusing instant the classical density of trajectories is infinite — geometrically, the paths form a caustic, the same bright cusp you see at the bottom of a coffee cup or in a swimming pool. The Van Vleck prefactor, which is literally the square root of that density, diverges there. This is the punchline of the article, and the next figure shows it directly: ∣prefactor∣=mω/2πℏ∣sin⁡ωT∣|{\rm prefactor}|=\sqrt{m\omega/2\pi\hbar|\sin\omega T|} spikes to infinity at every ωT=nπ\omega T=n\pi.

Figure
The Van Vleck prefactor diverges at every caustic ωT = nπ
|prefactor| ∝ 1/√|sin ωT| → ∞ at ωT = π, 2π, 3π ωT π2π 3π4π smooth between caustics

The core equations

We keep the chapter convention K=∫Dx eiS/ℏK=\int\mathcal D x\,e^{iS/\hbar}. Because the action is quadratic, the integral over the fluctuation y(t)=x(t)−xcl(t)y(t)=x(t)-x_{\rm cl}(t) factors off entirely, leaving K=F(T) eiScl/ℏK=F(T)\,e^{iS_{\rm cl}/\hbar}: the classical action sets the phase, and a fluctuation determinant F(T)F(T) sets the prefactor. The first equation states that universal semiclassical shape, and identifies FF with the Van Vleck determinant.

K(xf,T;xi,0)=12πiℏ ∂2Scl∂xi ∂xf  eiScl(xf,xi;T)/ℏ(1)K(x_f,T;x_i,0)=\sqrt{\frac{1}{2\pi i\hbar}\,\frac{\partial^2 S_{\rm cl}}{\partial x_i\,\partial x_f}}\;e^{iS_{\rm cl}(x_f,x_i;T)/\hbar} \qquad (1)

where: SclS_{\rm cl} — the action evaluated on the classical path with the given endpoints; ∂2Scl/∂xi∂xf\partial^2 S_{\rm cl}/\partial x_i\partial x_f — the Van Vleck determinant (in 1D, a single second derivative); ℏ\hbar — as usual. Read physically: ∂2Scl/∂xi∂xf=−∂pi/∂xf\partial^2 S_{\rm cl}/\partial x_i\partial x_f=-\partial p_i/\partial x_f measures how the required launch momentum changes with the destination — small change means many launch momenta funnel into a small target, i.e. a high trajectory density and large amplitude. Where the destination becomes insensitive to launch conditions (a focus), the determinant blows up. For the free particle the classical path is a straight line and the action is elementary; this is the case The Quantum Propagator reserved for us.

K0(xf,T;xi,0)=m2πiℏT  e im(xf−xi)2/2ℏT,Scl=m(xf−xi)22T(2)K_0(x_f,T;x_i,0)=\sqrt{\frac{m}{2\pi i\hbar T}}\;e^{\,im(x_f-x_i)^2/2\hbar T},\qquad S_{\rm cl}=\frac{m(x_f-x_i)^2}{2T} \qquad (2)

where: the prefactor m/2πiℏT\sqrt{m/2\pi i\hbar T} is (1/2πiℏ) ∣∂2Scl/∂xi∂xf∣\sqrt{(1/2\pi i\hbar)\,|\partial^2 S_{\rm cl}/\partial x_i\partial x_f|} with ∂2Scl/∂xi∂xf=−m/T\partial^2 S_{\rm cl}/\partial x_i\partial x_f=-m/T. Read it: the free particle has no caustics — 1/T1/T diverges only at T=0T=0 (the delta limit), never at finite time, because free trajectories fan out monotonically and never refocus. The oscillator is the star. Its classical path is a sinusoid pinned at both ends, and its action is the classic Feynman result — the one whose 1/sin⁡ωT1/\sin\omega T carries the caustics.

K(xf,T;xi,0)=mω2πiℏsin⁡ωT exp⁡ ⁣[imω2ℏsin⁡ωT((xi2+xf2)cos⁡ωT−2xixf)](3)K(x_f,T;x_i,0)=\sqrt{\frac{m\omega}{2\pi i\hbar\sin\omega T}}\,\exp\!\Big[\frac{im\omega}{2\hbar\sin\omega T}\big((x_i^2+x_f^2)\cos\omega T-2x_ix_f\big)\Big] \qquad (3)

where: ω\omega — oscillator frequency; the prefactor is again the Van Vleck form with ∂2Scl/∂xi∂xf=−mω/sin⁡ωT\partial^2 S_{\rm cl}/\partial x_i\partial x_f=-m\omega/\sin\omega T. Read physically: as ω→0\omega\to0, (3) reduces smoothly to the free kernel (2); as ωT→nπ\omega T\to n\pi, sin⁡ωT→0\sin\omega T\to0 and the prefactor diverges — the caustics of the figure.

Derivation AThe two exact kernels and the Van Vleck prefactor

The goal is to obtain (2) and (3) and to read off the Van Vleck prefactor in each, rather than quoting it. The strategy exploits that a quadratic action makes the path integral a shifted Gaussian: write x=xcl+yx=x_{\rm cl}+y with yy vanishing at both endpoints, so S[x]=Scl+S2[y]S[x]=S_{\rm cl}+S_2[y] with no cross term (the first variation vanishes on xclx_{\rm cl}). The classical action gives the phase; the yy-integral gives the prefactor, and for the oscillator that determinant is what produces 1/sin⁡ωT1/\sin\omega T. The one thing to watch is that the fluctuation integral is endpoint-independent — it depends only on TT — which is why the prefactor is a pure function of TT.

Step 1. Solve the classical equation. Free: xcl(t)=xi+(xf−xi)t/Tx_{\rm cl}(t)=x_i+(x_f-x_i)t/T. Oscillator: xcl(t)=[xisin⁡ω(T−t)+xfsin⁡ωt]/sin⁡ωTx_{\rm cl}(t)=[x_i\sin\omega(T-t)+x_f\sin\omega t]/\sin\omega T. Why: these are the unique solutions of x¨=0\ddot x=0 and x¨=−ω2x\ddot x=-\omega^2 x hitting xix_i at t=0t=0 and xfx_f at t=Tt=T; the verifier confirms both endpoints and both equations of motion.

Step 2. Evaluate the classical action. For a quadratic Lagrangian, integrate by parts and use the equation of motion to get Scl=m2[xx˙]0TS_{\rm cl}=\tfrac{m}{2}[x\dot x]_0^T. Why: the bulk term vanishes on the classical path, leaving only boundary data — a shortcut that gives Scl=m(Δx)2/2TS_{\rm cl}=m(\Delta x)^2/2T (free) and the cos⁡ωT\cos\omega T, xixfx_ix_f combination in (3). The verifier confirms Scl=m2[xx˙]0TS_{\rm cl}=\tfrac{m}{2}[x\dot x]_0^T equals the closed form (3).

Step 3. Take the Van Vleck determinant ∂2Scl/∂xi∂xf\partial^2 S_{\rm cl}/\partial x_i\partial x_f. Free: −m/T-m/T. Oscillator: −mω/sin⁡ωT-m\omega/\sin\omega T. Why: these are the prefactors of (2) and (3) up to the universal 1/2πiℏ\sqrt{1/2\pi i\hbar}; the verifier confirms both second derivatives symbolically.

Step 4. The fluctuation integral ∫Dy eiS2[y]/ℏ\int\mathcal D y\,e^{iS_2[y]/\hbar} reproduces exactly (1/2πiℏ) ∂2Scl/∂xi∂xf\sqrt{(1/2\pi i\hbar)\,\partial^2 S_{\rm cl}/\partial x_i\partial x_f} — the Van Vleck–Pauli–Morette theorem. Why: for a quadratic action the fluctuation determinant and the Van Vleck determinant are the same object (the Gelfand–Yaglom result); this is why we can read the prefactor straight off the classical action without doing the functional determinant by hand. *Verified: the free and oscillator second derivatives, the classical-path endpoints and equations of motion, and the boundary-term action are all confirmed symbolically; the ω→0\omega\to0 limit of (3) reduces to (2).*

The prefactor's divergences are not a defect — they are physics, and they demand a phase convention. When ωT\omega T passes through nπn\pi, sin⁡ωT\sin\omega T changes sign, so 1/sin⁡ωT\sqrt{1/\sin\omega T} jumps by −1=e−iπ/2\sqrt{-1}=e^{-i\pi/2} per caustic. This −π/2-\pi/2 per refocusing is the Maslov phase.

Go deeper · Derivation B · 2 minCaustics, the Maslov phase, and the spectral check
Derivation BCaustics, the Maslov phase, and the spectral check

We now show the two things that make (3) trustworthy: that its divergences sit exactly at the caustics, with a definite phase jump, and that resumming (3) over energy eigenstates returns the known oscillator spectrum. The strategy for the phase is to track 1/sin⁡ωT\sqrt{1/\sin\omega T} across a zero of sin⁡\sin; for the spectrum, to recognise (3) as the Mehler kernel, whose generating-function identity is ∑ne−i(n+12)ωTψn(xf)ψn∗(xi)\sum_n e^{-i(n+\frac12)\omega T}\psi_n(x_f)\psi_n^*(x_i). The subtlety is that the spectral sum converges only conditionally on the real-TT axis, so a small imaginary-time regulator is needed to sum it cleanly.

Step 1. Locate the caustics: the prefactor mω/2πiℏsin⁡ωT\sqrt{m\omega/2\pi i\hbar\sin\omega T} diverges when sin⁡ωT=0\sin\omega T=0, i.e. ωT=nπ\omega T=n\pi, n=1,2,3,…n=1,2,3,\dots Why: these are exactly the refocusing times of Step-1's classical bundle — every trajectory from xix_i returns to a common point, so the Van Vleck density is infinite. The verifier confirms sin⁡(nπ)=0\sin(n\pi)=0 at nπn\pi.

Step 2. Track the phase across a caustic: as ωT\omega T increases through nπn\pi, sin⁡ωT\sin\omega T changes sign, so the propagator acquires a factor e−iπ/2e^{-i\pi/2} — the Maslov phase, −π/2-\pi/2 per turning point. Why: this is the same π/4\pi/4-per-turning-point (hence π/2\pi/2 per full pass) bookkeeping that the WKB Connection Formulas article derives from the Airy function; here it appears as a branch cut of 1/sin⁡\sqrt{1/\sin}. The last article of the chapter, Bohr-Sommerfeld and Maslov Quantization, promotes it to a topological index.

Step 3. Resum (3) as the Mehler kernel: K=∑n=0∞e−i(n+12)ωTψn(xf)ψn∗(xi)K=\sum_{n=0}^\infty e^{-i(n+\frac12)\omega T}\psi_n(x_f)\psi_n^*(x_i), with ψn\psi_n the oscillator eigenfunctions. Why: this is the spectral form of the propagator (owned by The Quantum Propagator), and the phases e−i(n+12)ωTe^{-i(n+\frac12)\omega T} display the spectrum En=ℏω(n+12)E_n=\hbar\omega(n+\tfrac12) — the ground-state 12\tfrac12 visible as the n=0n=0 phase. The result is recalled, not re-derived, from Quantum Harmonic Oscillator: Analytic Solution.

Step 4. Verify numerically that (3) equals the spectral sum. Why: with the imaginary-time regulator T→T−i(0.4/ω)T\to T-i(0.4/\omega) the Mehler sum converges geometrically and reproduces (3) to ∼10−12\sim10^{-12} in 60 terms — an independent confirmation that the path-integral kernel carries the correct spectrum. *Verified: caustics at ωT=nπ\omega T=n\pi; the oscillator kernel equals the regulated Mehler spectral sum to <10−8<10^{-8}; the n=0n=0 phase encodes the zero-point 12ℏω\tfrac12\hbar\omega.*

Limiting cases

caseresultmeaning
ω→0\omega\to0(3) →\to (2)oscillator becomes free particle
ωT→nπ\omega T\to n\piprefactor →∞\to\inftycaustic: all paths refocus
T→0T\to0K0→δ(xf−xi)K_0\to\delta(x_f-x_i)free delta limit
across a causticphase jump e−iπ/2e^{-i\pi/2}the Maslov phase, −π/2-\pi/2 per focus
resum over nn∑ne−i(n+12)ωTψnψn∗\sum_n e^{-i(n+\frac12)\omega T}\psi_n\psi_n^*recovers En=ℏω(n+12)E_n=\hbar\omega(n+\tfrac12)
ℏ→0\hbar\to0prefactor ×eiScl/ℏ\times e^{iS_{\rm cl}/\hbar}this is the semiclassical form for any quadratic action

Worked examples

Example 1 — The free action and prefactor. Compute SclS_{\rm cl} and the Van Vleck prefactor for a free particle with m=1m=1, ℏ=1\hbar=1, over T=1T=1, endpoints xi=0x_i=0, xf=1x_f=1.

Step 1. Classical action: Scl=m(xf−xi)2/2T=(1)(1)2/(2⋅1)=12S_{\rm cl}=m(x_f-x_i)^2/2T=(1)(1)^2/(2\cdot1)=\tfrac12.

Step 2. Van Vleck determinant: ∂2Scl/∂xi∂xf=−m/T=−1\partial^2 S_{\rm cl}/\partial x_i\partial x_f=-m/T=-1, so the prefactor magnitude is ∣−1∣/2πℏ=1/2π\sqrt{|{-1}|/2\pi\hbar}=\sqrt{1/2\pi}.

Step 3. Assemble: K0=1/2πi  ei/2K_0=\sqrt{1/2\pi i}\;e^{i/2}, i.e. magnitude 1/2π≈0.399\sqrt{1/2\pi}\approx0.399 and phase ei(1/2−π/4)e^{i(1/2-\pi/4)} (the −π/4-\pi/4 from 1/i\sqrt{1/i}).

Answer: Scl=0.5S_{\rm cl}=\mathbf{0.5} and prefactor 1/2πi\mathbf{\sqrt{1/2\pi i}} — the free kernel has no caustic, only the T→0T\to0 delta.

Example 2 — The oscillator prefactor at a quarter period, and the first caustic. For the oscillator (m=ω=ℏ=1m=\omega=\hbar=1), evaluate the prefactor at ωT=π/2\omega T=\pi/2 and identify the first caustic.

Step 1. At ωT=π/2\omega T=\pi/2, sin⁡ωT=1\sin\omega T=1, so the prefactor is mω/2πiℏ⋅1=1/2πi\sqrt{m\omega/2\pi i\hbar\cdot1}=\sqrt{1/2\pi i} — the same magnitude as the free case, because a quarter period has not yet focused anything.

Step 2. Increase ωT\omega T toward π\pi: sin⁡ωT→0+\sin\omega T\to0^+, so the prefactor 1/2πisin⁡ωT→∞\sqrt{1/2\pi i\sin\omega T}\to\infty — the first caustic at ωT=π\omega T=\pi (half a period), where every trajectory has swung across the well and refocused at −xi-x_i.

Step 3. Crossing ωT=π\omega T=\pi, sin⁡ωT\sin\omega T turns negative, multiplying KK by e−iπ/2e^{-i\pi/2} — the first Maslov phase, exactly what the WKB connection formulae charge for the turning point.

Answer: prefactor =1/2πi=\mathbf{\sqrt{1/2\pi i}} at ωT=π/2\omega T=\pi/2; first caustic at ωT=π\mathbf{\omega T=\pi} with a −π/2\mathbf{-\pi/2} Maslov phase across it.

Origins · 1 minvan vleck determinant and how this was discovered
VV
van vleck determinant
1928 · the density of classical trajectories

The prefactor of the semiclassical propagator is the Van Vleck determinant, introduced by J. H. Van Vleck in 1928 as a quantum-corrected form of the classical correspondence principle. Its content is geometric: ∂2Scl/∂xi∂xf\partial^2 S_{\rm cl}/\partial x_i\partial x_f measures how a bundle of classical trajectories, launched from xix_i with slightly different momenta, spreads by the time it reaches xfx_f. Where the bundle bunches — a focus — the determinant diverges, marking a caustic; where it fans out, the amplitude thins. Pauli and Cécile Morette-DeWitt put the object on firm footing around 1950–51, giving the modern multidimensional form det⁡(−∂2Scl/∂xi∂xf)\det(-\partial^2 S_{\rm cl}/\partial x_i\partial x_f) that reappears in every semiclassical trace formula, up to and including Gutzwiller's for chaotic systems.

History
1866
— Mehler publishes the kernel identity behind the oscillator propagator's spectral sum
1928
— Van Vleck introduces the determinant as a correspondence-principle amplitude
1948
— Feynman evaluates the free and oscillator path integrals exactly
1951
— Morette gives the semiclassical prefactor a rigorous derivation

Going further

  • Prerequisites: The Feynman Path Integral Formulation; The Propagator from Path Integrals; Gaussian integrals; Quantum Harmonic Oscillator: Analytic Solution.
  • Leads to: Path Integral and the Schrödinger Equation; Imaginary-Time and Euclidean Path Integrals; Bohr-Sommerfeld and Maslov Quantization (where the caustics become the Maslov index).
  • Provenance: upgraded from the AllQFT `qm` base (QUANT.RQM.GAUSP.1094), after Feynman & Hibbs. The free/oscillator kernels were flagged for this article by The Quantum Propagator ("get the next two articles to themselves"); the spectrum En=ℏω(n+12)E_n=\hbar\omega(n+\tfrac12) is owned by Quantum Harmonic Oscillator: Analytic Solution and recalled, not re-derived; the caustic/Maslov phase is developed fully in Bohr-Sommerfeld and Maslov Quantization.
Why is the prefactor a determinant of SclS_{\rm cl} and not something computed from the fluctuation integral?

It is both — and their equality is the theorem. The fluctuation integral ∫Dy eiS2[y]/ℏ\int\mathcal D y\,e^{iS_2[y]/\hbar} is a functional determinant (of the operator −m(∂t2+ω2)-m(\partial_t^2+\omega^2) with Dirichlet ends). The Gelfand–Yaglom result says that functional determinant equals 1/∂2Scl/∂xi∂xf1/\sqrt{\partial^2 S_{\rm cl}/\partial x_i\partial x_f} up to the universal 2πiℏ\sqrt{2\pi i\hbar} factors. So you can compute the hard functional determinant or just differentiate the classical action twice — they give the same Van Vleck prefactor. The second route is why (1) is so useful.

Does the free particle really have no caustics, ever?

In 1D with no potential, correct: ∂2Scl/∂xi∂xf=−m/T\partial^2 S_{\rm cl}/\partial x_i\partial x_f=-m/T diverges only at T=0T=0, which is the delta-function initial condition, not a caustic. Free trajectories fan out monotonically and never reconverge, so there is nothing to focus. Add walls (a box), a lens (a quadratic potential over a finite region), or go to higher dimensions with a focusing geometry, and caustics reappear. The oscillator is the simplest system that has them, which is exactly why it is the canonical example here.

Is the Maslov phase the same −π/2-\pi/2 that shows up in WKB connection formulae?

Yes — it is one phenomenon wearing two derivations. In WKB, matching the oscillatory solution to the decaying one across a classical turning point via the Airy function costs π/4\pi/4; a full traversal (out and back past two turning points, or a focus) accumulates π/2\pi/2. Here the same π/2\pi/2 appears as the branch jump of 1/sin⁡ωT\sqrt{1/\sin\omega T} across a caustic. The Bohr-Sommerfeld and Maslov Quantization article ties them together and shows the count is topological — the Maslov index — so the quantization condition gets n+μ/4n+\mu/4 instead of nn.

The spectral sum only converged after adding an imaginary part to TT — is that a cheat?

No, it is the standard interpretation. The Mehler sum ∑ne−i(n+12)ωTψnψn∗\sum_n e^{-i(n+\frac12)\omega T}\psi_n\psi_n^* sits on the unit circle for real TT, where it converges only conditionally (as a distribution). Giving TT a small negative imaginary part, T→T−iηT\to T-i\eta, damps term nn by e−(n+12)ωηe^{-(n+\frac12)\omega\eta} and makes the sum absolutely convergent; the physical real-TT kernel is the η→0+\eta\to0^+ limit. This iϵi\epsilon-style regulator is exactly what defines the propagator as a boundary value of an analytic function — the same idea that underlies the Feynman propagator's causal prescription.

How does the oscillator kernel reduce to the free one as ω→0\omega\to0?

Expand the small-ω\omega limit of (3): sin⁡ωT→ωT\sin\omega T\to\omega T and cos⁡ωT→1\cos\omega T\to1, so the prefactor mω/2πiℏsin⁡ωT→m/2πiℏT\sqrt{m\omega/2\pi i\hbar\sin\omega T}\to\sqrt{m/2\pi i\hbar T} and the exponent imω2ℏsin⁡ωT[(xi2+xf2)−2xixf]→im2ℏT(xf−xi)2\tfrac{im\omega}{2\hbar\sin\omega T}[(x_i^2+x_f^2)-2x_ix_f]\to\tfrac{im}{2\hbar T}(x_f-x_i)^2. Both pieces land exactly on the free kernel (2). The verifier confirms the prefactor limit symbolically. This is a good sanity check any time you derive a propagator: turn off the potential and you must recover the free particle.

Can I use Van Vleck eiScl/ℏ\sqrt{\text{Van Vleck}}\,e^{iS_{\rm cl}/\hbar} for a non-quadratic potential?

Not exactly — only as the leading semiclassical approximation. For a general VV, the fluctuation action S2[y]S_2[y] has cubic and higher terms in yy, so the path integral is not a pure Gaussian and (1) is only the ℏ→0\hbar\to0 leading term, with corrections in powers of ℏ\hbar. The free particle and oscillator are special because S2S_2 is exactly quadratic, making (1) exact. This is the same statement as "WKB is exact for the oscillator": the semiclassical formula happens to be the whole answer when the action is quadratic.

Before this

Where this leads