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Instantons in Quantum Mechanics

In quantum mechanics, an instanton is a finite-action classical solution of the Euclidean equations of motion. It gives a semiclassical estimate of tunneling effects that are exponentially small and invisible to ordinary perturbation theory around a single classical minimum.

The Euclidean action for one coordinate is

SE[x]=∫dτ[m2(dxdτ)2+V(x)].S_E[x] = \int d\tau \left[ \frac{m}{2} \left(\frac{dx}{d\tau}\right)^2 + V(x) \right].

Euclidean path integrals are weighted schematically by

e−SE[x]/ℏ,e^{-S_E[x]/\hbar},

so finite-action saddle points can dominate exponentially small effects.

Double-Well Splitting evaluates the quartic trajectory and S0=4/3S_0=4/3 in a convention designed for direct comparison with numerical spectral gaps. The reusable saddle construction remains here.

Stationarity of SES_E gives

md2xdτ2=dVdx.m\frac{d^2x}{d\tau^2} = \frac{dV}{dx}.

This differs in sign from the real-time Newton equation. Equivalently, Euclidean motion in V(x)V(x) resembles real-time motion in the inverted potential −V(x)-V(x).

For finite action, the path must approach minima of VV as τ→±∞\tau\to\pm\infty, so that both the kinetic and potential contributions remain integrable.

For a degenerate double well with minima at x=−ax=-a and x=ax=a, an instanton satisfies

x(τ)→−aasτ→−∞,x(\tau)\to -a \quad \text{as} \quad \tau\to-\infty,

and

x(τ)→aasτ→+∞.x(\tau)\to a \quad \text{as} \quad \tau\to+\infty.

The anti-instanton has the opposite orientation. Multi-instanton configurations describe repeated tunneling events in Euclidean time.

For a double well whose minima have V=0V=0, the Euclidean energy

m2(dxdτ)2−V(x)\frac{m}{2} \left(\frac{dx}{d\tau}\right)^2 - V(x)

is conserved. The finite-action boundary conditions set this conserved value to zero, so

m2(dxdτ)2=V(x).\frac{m}{2} \left(\frac{dx}{d\tau}\right)^2 = V(x).

Therefore the instanton action can be written as

S0=∫x−x+dx 2mV(x).S_0 = \int_{x_-}^{x_+} dx\, \sqrt{2mV(x)}.

This is the same under-barrier action that appears in WKB estimates of tunneling exponents.

For

V(x)=λ(x2−a2)2,V(x)=\lambda(x^2-a^2)^2,

the minima are at x=±ax=\pm a. The small-oscillation frequency near a minimum is

ω=8λa2m.\omega = \sqrt{\frac{8\lambda a^2}{m}}.

The instanton solution can be written

xinst(τ)=atanh⁡[ω2(τ−τ0)].x_{\mathrm{inst}}(\tau) = a \tanh \left[ \frac{\omega}{2} (\tau-\tau_0) \right].

The parameter τ0\tau_0 is the instanton center. Translating the instanton in Euclidean time costs no action, so τ0\tau_0 is a collective coordinate.

The action is

S0=∫−aadx 2mλ(a2−x2)=43a32mλ.S_0 = \int_{-a}^{a} dx\, \sqrt{2m\lambda}(a^2-x^2) = \frac{4}{3} a^3 \sqrt{2m\lambda}.

For the symmetric double well, instantons produce a splitting between even and odd low-energy states:

ΔE∼Ae−S0/ℏ.\Delta E \sim A e^{-S_0/\hbar}.

The exponent S0S_0 comes from the classical Euclidean saddle. The prefactor AA comes from quadratic fluctuations around the saddle, normalization of the zero mode, and multi-instanton combinatorics.

For many purposes, the exponent is the main physical information. Precise prefactors require more careful analysis than the leading saddle picture.

Tunneling Splittings derives how the dilute instanton sum becomes an even–odd spectral splitting and matches that result to Herring and WKB formulas.

Double-Well Instanton Numerical Check tests the normalized one-loop formula against converged parity gaps while keeping exponent accuracy, prefactor accuracy, and numerical resolution separate.

A metastable well poses a different boundary-value problem. Bounce Solutions develops the Euclidean round trip, its decay exponent, and the additional negative fluctuation mode.

Because the instanton can be centered at any τ0\tau_0, the quadratic fluctuation operator around the instanton has a zero mode proportional to

dxinstdτ.\frac{dx_{\mathrm{inst}}}{d\tau}.

This zero mode must not be treated like an ordinary Gaussian fluctuation. Instead, one integrates over the collective coordinate τ0\tau_0. This is the simplest example of a technical issue that becomes central in field-theory instanton calculations.

Perturbation theory around one minimum produces a series in local fluctuations. It does not connect the two classical minima at any finite order. The instanton contribution has the form

e−S0/ℏ,e^{-S_0/\hbar},

which is nonanalytic at ℏ=0\hbar=0. This is why tunneling splittings are called nonperturbative.

Quantum-mechanical instantons are instantons in 0+10+1 dimensions: one time coordinate and no spatial field profile. In quantum field theory, instantons are finite-action Euclidean field configurations. The same saddle-point logic appears, but new issues enter:

  • spatial dependence and topology;
  • gauge redundancy;
  • zero modes from symmetries;
  • fluctuation determinants over fields;
  • renormalization and scale dependence.

The quantum-mechanical case is the cleanest place to learn the mechanism before those complications enter.

  • Treating Wick rotation as a purely formal substitution without checking boundary conditions.
  • Forgetting that instantons are Euclidean, not real-time classical, solutions.
  • Confusing the instanton exponent with the full prefactor.
  • Ignoring zero modes when discussing fluctuation determinants.
  • Presenting instanton methods as replacing WKB rather than matching the same semiclassical exponent in one-dimensional tunneling.
  1. Derive the Euclidean equation of motion from SES_E.
Solution

Vary

SE=∫dτ[m2x˙2+V(x)].S_E = \int d\tau \left[ \frac{m}{2}\dot x^2+V(x) \right].

The variation is

δSE=∫dτ[mx˙ δx˙+V′(x)δx].\delta S_E = \int d\tau \left[ m\dot x\,\delta\dot x + V'(x)\delta x \right].

Integrating the first term by parts and taking endpoint variations to vanish gives

δSE=∫dτ[−mx¨+V′(x)]δx.\delta S_E = \int d\tau \left[ -m\ddot x+V'(x) \right]\delta x.

Stationarity for arbitrary δx\delta x gives

mx¨=V′(x).m\ddot x=V'(x).
  1. Show that the instanton action can be written as an integral over xx when the Euclidean energy is zero.
Solution

Zero Euclidean energy gives

m2x˙2=V(x).\frac{m}{2}\dot x^2=V(x).

Then

SE=∫dτ[m2x˙2+V(x)]=∫dτ 2V(x).S_E = \int d\tau \left[ \frac{m}{2}\dot x^2+V(x) \right] = \int d\tau\,2V(x).

Using

dτ=dxx˙=dxm2V(x),d\tau = \frac{dx}{\dot x} = dx \sqrt{\frac{m}{2V(x)}},

one obtains

S0=∫dx 2mV(x).S_0 = \int dx\,\sqrt{2mV(x)}.
  1. Why does the instanton center τ0\tau_0 lead to a zero mode?
Solution

The Euclidean action is invariant under translations of τ\tau. If xinst(τ)x_{\mathrm{inst}}(\tau) is a solution, then xinst(τ−τ0)x_{\mathrm{inst}}(\tau-\tau_0) is also a solution with the same action. Differentiating this family with respect to τ0\tau_0 gives a fluctuation proportional to dxinst/dτdx_{\mathrm{inst}}/d\tau, and the action does not change to quadratic order in that direction. Hence it is a zero mode.

  • S. Coleman, Aspects of Symmetry, Cambridge University Press, 1985.
  • R. Rajaraman, Solitons and Instantons, North-Holland, 1982.
  • J. Zinn-Justin, Path Integrals in Quantum Mechanics, Oxford University Press, 2005.
  • H. Kleinert, Path Integrals in Quantum Mechanics, Statistics, Polymer Physics, and Financial Markets, 5th ed., World Scientific, 2009.