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Tunneling Splittings

A tunneling splitting is an energy difference between nearly degenerate bound states whose localized semiclassical configurations are separated by a classically forbidden region. For the lowest doublet of a symmetric one-dimensional double well,

ΔE≡Eodd−Eeven>0.\Delta E \equiv E_{\mathrm{odd}} - E_{\mathrm{even}} \gt0.

The splitting is a property of the spectrum of a closed Hermitian Hamiltonian. It is not a barrier-transmission probability and not a metastable decay rate. In the deep-well regime it is exponentially smaller than the intrawell excitation scale:

ΔE≪ℏωwell.\Delta E \ll \hbar\omega_{\mathrm{well}}.

This page owns the quantitative dictionary among the effective tunneling matrix element, the Herring flux formula, the WKB barrier action, the instanton sector sum, Euclidean kernels, and exact numerical eigenvalues. Double-Well Tunneling owns the physical two-well model. Coupled Wells and Avoided Crossings owns the generic biased two-level spectrum. Instantons in Quantum Mechanics and Fluctuation Determinants Preview own the saddle construction and determinant technology.

Double-Well Splitting applies this dictionary to a dimensionless quartic well, including its exact instanton, finite-energy WKB action, one-loop prefactor, and a converged seven-point spectral benchmark.

A symmetric double-well barrier action mapped to an even and odd spectral doublet separated by the tunneling splitting.

A localized state leaks through the forbidden interval between the inner turning points. Herring flux, WKB matching, and instanton calculus are different ways to determine the same low-energy coupling JJ. Diagonalizing the doublet gives ΔE=2J\Delta E=2J.

Let

H=−ℏ22md2dx2+V(x).H = - \frac{\hbar^2}{2m} \frac{d^2}{dx^2} + V(x).

The symmetry condition is

V(−x)=V(x),V(-x)=V(x),

with two well-separated minima. The exact eigenfunctions have definite parity. For the lowest doublet, write

H∣e⟩=Ee∣e⟩,P∣e⟩=+∣e⟩,H∣o⟩=Eo∣o⟩,P∣o⟩=−∣o⟩.\begin{gathered} H\lvert e\rangle = E_e\lvert e\rangle, \qquad \mathsf P\lvert e\rangle = +\lvert e\rangle, \\ H\lvert o\rangle = E_o\lvert o\rangle, \qquad \mathsf P\lvert o\rangle = -\lvert o\rangle. \end{gathered}

In one dimension the nodeless even ground state lies below the odd state, so

ΔE=Eo−Ee.\Delta E = E_o-E_e.

The mean doublet energy is

Eˉ=Ee+Eo2.\bar E = \frac{E_e+E_o}{2}.

A useful two-state description requires a separation of scales. If δintra\delta_{\mathrm{intra}} is the gap from this doublet to the next pair of levels, then

ΔE≪δintra.\Delta E \ll \delta_{\mathrm{intra}}.

The inequality says more than “the barrier is high.” It ensures that left-right mixing can be discussed without simultaneously mixing several intrawell excitations.

All exact eigenvalues of a closed, self-adjoint double-well Hamiltonian are real. A wavepacket initially localized in one well can oscillate, dephase among several doublets, and recur, but it does not possess an intrinsic exponential decay width.

By contrast:

  • open-barrier scattering asks for transmitted flux and gives a probability T(E)T(E);
  • a metastable well asks for a resonance width or decay rate γ\gamma;
  • a symmetric bound double well asks for an energy splitting ΔE\Delta E.

The same forbidden-region action can appear in all three problems, but boundary conditions determine whether the exponential enters an amplitude, a probability, a splitting, or a rate.

Within the exact two-dimensional subspace, define

∣L⟩=∣e⟩+∣o⟩2,∣R⟩=∣e⟩−∣o⟩2.\begin{aligned} \lvert L\rangle &= \frac{ \lvert e\rangle+\lvert o\rangle }{\sqrt2}, \\ \lvert R\rangle &= \frac{ \lvert e\rangle-\lvert o\rangle }{\sqrt2}. \end{aligned}

These states are exactly orthonormal. They become spatially localized only when the parity partners have nearly identical probability densities within either well, as happens for a high barrier.

In this basis,

Heff=(Eˉ−J−JEˉ),J=ΔE2.H_{\mathrm{eff}} = \begin{pmatrix} \bar E & -J\\ -J & \bar E \end{pmatrix}, \qquad J = \frac{\Delta E}{2}.

The sign of the off-diagonal entry is a phase convention chosen so that J>0J\gt0 and the even state is lower. The spectral statement is invariant:

ΔE=2J.\Delta E=2J.

If the system begins in ∣L⟩\lvert L\rangle and remains within this doublet,

PR(t)=sin⁡2(ΔE t2ℏ).P_R(t) = \sin^2 \left( \frac{\Delta E\,t}{2\hbar} \right).

The first complete transfer occurs at

ttransfer=πℏΔE.t_{\mathrm{transfer}} = \frac{\pi\hbar}{\Delta E}.

This dynamics is derived in the introductory Double-Well Potential page. Here the central task is to determine JJ rather than assume it.

Localized trial functions constructed independently in the two wells generally overlap. Let

⟨ℓ∣ℓ⟩=⟨r∣r⟩=1,s≡⟨ℓ∣r⟩,h≡⟨ℓ∣H∣r⟩,Ed≡⟨ℓ∣H∣ℓ⟩=⟨r∣H∣r⟩,\begin{gathered} \langle \ell\vert\ell\rangle = \langle r\vert r\rangle = 1, \\ s \equiv \langle \ell\vert r\rangle, \qquad h \equiv \langle \ell\vert H\vert r\rangle, \\ E_d \equiv \langle \ell\vert H\vert\ell\rangle = \langle r\vert H\vert r\rangle, \end{gathered}

where phases have been chosen so that ss and hh are real. The normalized even and odd combinations are

∣ψ±⟩=∣ℓ⟩±∣r⟩2(1±s).\lvert \psi_\pm\rangle = \frac{ \lvert \ell\rangle \pm \lvert r\rangle }{ \sqrt{2(1\pm s)} }.

Their variational energies are

E±=Ed±h1±s.E_\pm = \frac{E_d\pm h}{1\pm s}.

Therefore

E−−E+=2(Eds−h)1−s2.E_--E_+ = \frac{ 2(E_ds-h) }{ 1-s^2 }.

The effective coupling inferred from nonorthogonal trial states is

Jeff=Eds−h1−s2.J_{\mathrm{eff}} = \frac{E_ds-h}{1-s^2}.

Only after orthogonalization, or when ss is negligible at the requested accuracy, may one identify JJ with −h-h. Because ss and h/Edh/E_d can carry the same tunneling exponential, dropping overlap in one place but not the other can corrupt the leading prefactor.

For a smooth symmetric one-dimensional well, the splitting can be extracted from one localized wavefunction without matching solutions through all four turning points.

Let ψR(x)\psi_R(x) be a real approximate solution at energy ElocE_{\mathrm{loc}} that is localized in the right well, decays through the central barrier, and is normalized by

∫0∞∣ψR(x)∣2 dx≃1.\int_0^\infty |\psi_R(x)|^2\,dx \simeq 1.

Then the leading splitting is

ΔE≃2ℏ2mψR(0)ψR′(0).\Delta E \simeq \frac{2\hbar^2}{m} \psi_R(0)\psi_R'(0).

For a right-localized nodeless state, ψR(0)>0\psi_R(0)\gt0 and ψR′(0)>0\psi_R'(0)\gt0. The formula measures probability-current capacity across the dividing point, even though each real stationary state separately carries no net current.

Let ueu_e and uou_o be the exact normalized even and odd eigenfunctions. Subtracting their Schrödinger equations after cross multiplication gives

ΔE∫0∞ueuo dx=ℏ22m×ue(0)uo′(0).\begin{aligned} \Delta E \int_0^\infty u_eu_o\,dx &= \frac{\hbar^2}{2m} \\ &\quad\times u_e(0)u_o'(0). \end{aligned}

The boundary terms at infinity vanish, while

ue′(0)=0,uo(0)=0.u_e'(0)=0, \qquad u_o(0)=0.

In the high-barrier limit,

∫0∞ueuo dx≃12.\int_0^\infty u_eu_o\,dx \simeq \frac12.

Moreover,

ue(0)≃2 ψR(0),uo′(0)≃2 ψR′(0).\begin{aligned} u_e(0) &\simeq \sqrt2\,\psi_R(0), \\ u_o'(0) &\simeq \sqrt2\,\psi_R'(0). \end{aligned}

Substitution yields Herring’s formula. Its usefulness is conceptual as well as computational: the spectral splitting is linear in a tunneling amplitude measured at the barrier, not quadratic like a transmission probability.

The formula assumes an isolated nearly degenerate doublet and reflection symmetry. Multidimensional versions replace the midpoint expression by a flux integral over a dividing surface, but then the tunneling path, transverse fluctuations, and coordinate-dependent mass metric require separate control.

Let EnE_n be the energy of the nnth state localized in either isolated well. If x1(En)x_1(E_n) and x2(En)x_2(E_n) are the inner turning points bounding the forbidden interval, define the one-way barrier action

Wn=∫x1(En)x2(En)dx 2m[V(x)−En].W_n = \int_{x_1(E_n)}^{x_2(E_n)} dx\, \sqrt{ 2m[V(x)-E_n] }.

In the semiclassical regime,

Wnℏ≫1,\frac{W_n}{\hbar}\gg1,

and the splitting has the structure

ΔEn∼Ane−Wn/ℏ.\Delta E_n \sim A_n e^{-W_n/\hbar}.

Here AnA_n has dimensions of energy and is algebraic rather than exponential in the semiclassical parameter. It is often of order ℏωwell\hbar\omega_{\mathrm{well}}, but its numerical coefficient is not universal.

Exponential accuracy and prefactor accuracy

Section titled “Exponential accuracy and prefactor accuracy”

At exponential accuracy, the claim is only that

−ℏlog⁡(ΔEnEref)∼Wn,- \hbar \log \left( \frac{\Delta E_n}{E_{\mathrm{ref}}} \right) \sim W_n,

where ErefE_{\mathrm{ref}} is an energy scale with no tunneling exponential. This level of accuracy is robust and often physically sufficient.

A normalized asymptotic formula for ΔEn\Delta E_n requires the prefactor. For the lowest doublet, ordinary linear-turning-point connection formulas combined with a naive harmonic “attempt frequency” can miss an order-one coefficient. Controlled matching to the quadratic well bottom, a Herring calculation, or a correctly normalized instanton determinant resolves that issue.

This is why two statements must not be conflated:

  1. WKB correctly identifies the barrier exponential.
  2. Every compact textbook prefactor is automatically correct for the ground doublet.

The first is standard. The second is false without specifying the matching scheme and asymptotic regime.

Across the barrier, a one-way wave amplitude scales as

tbarrier∼e−Wn/ℏ.t_{\mathrm{barrier}} \sim e^{-W_n/\hbar}.

A scattering probability squares that amplitude:

T∼e−2Wn/ℏ.T \sim e^{-2W_n/\hbar}.

The bound-state splitting is linear in the off-diagonal amplitude:

ΔEn∼e−Wn/ℏ.\Delta E_n \sim e^{-W_n/\hbar}.

Importing the scattering-probability exponent into a splitting formula therefore produces an erroneous factor of two. Barrier Penetration and Tunneling is the canonical home for the scattering calculation.

Normalize the degenerate minima to

V(±a)=0.V(\pm a)=0.

The Euclidean instanton connecting −a-a to +a+a has action

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

This is the zero-reference-energy version of the same geometric barrier action. The explicit quartic solution and its action are derived in Instantons in Quantum Mechanics Preview.

Define the one-dimensional fluctuation operators

LI=−d2dτ2+1mV′′(xI),L0=−d2dτ2+ω2.\begin{aligned} \mathscr L_I &= - \frac{d^2}{d\tau^2} + \frac{1}{m} V''(x_I), \\ \mathscr L_0 &= - \frac{d^2}{d\tau^2} + \omega^2. \end{aligned}

At one loop, the one-instanton density can be written schematically as

K1=(S02πℏ)1/2[det⁡L0det⁡′LI]1/2.\mathcal K_1 = \left( \frac{S_0}{2\pi\hbar} \right)^{1/2} \left[ \frac{ \det\mathscr L_0 }{ \det{}'\mathscr L_I } \right]^{1/2}.

The prime removes the translation zero mode. With consistent boundary conditions and determinant normalization, K1\mathcal K_1 has units of inverse time.

From an instanton gas to an energy doublet

Section titled “From an instanton gas to an energy doublet”

Let

ζ≡K1e−S0/ℏ.\zeta \equiv \mathcal K_1 e^{-S_0/\hbar}.

In a dilute gas, paths beginning and ending in the same well contain an even number of transitions, while paths ending in the opposite well contain an odd number. Summing those sectors gives

ZLL(T)≃Ne−EpertT/ℏcosh⁡(ζT),ZRL(T)≃Ne−EpertT/ℏsinh⁡(ζT).\begin{aligned} Z_{LL}(T) &\simeq \mathcal N e^{-E_{\mathrm{pert}}T/\hbar} \cosh(\zeta T), \\ Z_{RL}(T) &\simeq \mathcal N e^{-E_{\mathrm{pert}}T/\hbar} \sinh(\zeta T). \end{aligned}

Using

cosh⁡(ζT)=12(eζT+e−ζT),\cosh(\zeta T) = \frac12 \left( e^{\zeta T} + e^{-\zeta T} \right),

one reads off

Ee=Epert−ℏζ,Eo=Epert+ℏζ.\begin{aligned} E_e &= E_{\mathrm{pert}} - \hbar\zeta, \\ E_o &= E_{\mathrm{pert}} + \hbar\zeta. \end{aligned}

Thus

ΔE=2ℏK1e−S0/ℏ.\Delta E = 2\hbar\mathcal K_1 e^{-S_0/\hbar}.

The factor of two is now transparent: one instanton determines the off-diagonal coupling

J=ℏK1e−S0/ℏ,J = \hbar\mathcal K_1 e^{-S_0/\hbar},

and diagonalizing the two-state Hamiltonian gives ΔE=2J\Delta E=2J.

For the ground doublet, WKB naturally uses the turning-point action at Eloc≃ℏω/2E_{\mathrm{loc}}\simeq\hbar\omega/2, whereas the zero-energy instanton uses S0S_0. Since Eloc=O(ℏ)E_{\mathrm{loc}}=O(\hbar), shifting the action to zero energy changes terms that can migrate between the exponent and prefactor.

Consequently:

  • at leading exponential order, WKB and the instanton give the same suppression;
  • at prefactor accuracy, endpoint matching and determinant normalization must be compared in the same convention;
  • substituting E=0E=0 into one formula while retaining the prefactor from another is not a controlled hybrid.

Correctly executed WKB and instanton calculations agree. Fluctuation Determinants Preview explains why that agreement is technically subtler than matching the actions alone.

ViewPrimary inputQuantity computedMain caveat
Exact spectrumFull Hamiltonian and boundary conditionsΔE=Eo−Ee\Delta E=E_o-E_eSubtractive loss when the gap is extremely small
Effective doubletOrthonormal localized basisΔE=2J\Delta E=2JJJ is an input until derived microscopically
Herring fluxOne normalized localized barrier tailMidpoint flux and ΔE\Delta ERequires an isolated nearly symmetric doublet
WKBTurning points and forbidden action WnW_nExponential and, with matching, prefactorGround-state prefactors need quadratic-well matching
Instanton gasEuclidean saddle, zero mode, determinantJJ and the parity doubletRequires a valid dilute sector sum and normalized measure

These are not competing explanations. They are different projections of the same spectral problem:

barrier leakage⟶J⟶ΔE=2J\boxed{ \text{barrier leakage} \longrightarrow J \longrightarrow \Delta E=2J }

The box is useful here because it is the organizing identity of the page; most intermediate formulas are not boxed.

Suppose a control parameter λ\lambda changes the action and prefactor:

ΔE(λ)=A(λ)exp⁡[−S(λ)ℏ].\Delta E(\lambda) = A(\lambda) \exp \left[ - \frac{S(\lambda)}{\hbar} \right].

Then

dlog⁡ΔEdλ=dlog⁡Adλ−1ℏdSdλ.\frac{d\log\Delta E}{d\lambda} = \frac{d\log A}{d\lambda} - \frac{1}{\hbar} \frac{dS}{d\lambda}.

When S/ℏ≫1S/\hbar\gg1, a modest fractional change in barrier height, width, or effective mass can change the splitting by orders of magnitude.

If the potential and tunneling path are held fixed,

S∝m.S \propto \sqrt m.

Therefore

dlog⁡ΔEdlog⁡m=dlog⁡Adlog⁡m−S2ℏ.\frac{d\log\Delta E}{d\log m} = \frac{d\log A}{d\log m} - \frac{S}{2\hbar}.

The action term normally dominates. This explains the strong isotope dependence of molecular tunneling splittings. In a real polyatomic molecule, isotopic substitution can also alter normal-mode coupling, zero-point energies, and the effective multidimensional path, so a one-coordinate m\sqrt m law is a diagnostic rather than a universal exact formula.

Let a symmetry-breaking bias produce localized energies differing by ε=EL−ER\varepsilon=E_L-E_R. In an orthonormal basis,

Heff=(Eˉ+ε/2−J−JEˉ−ε/2).H_{\mathrm{eff}} = \begin{pmatrix} \bar E+\varepsilon/2 & -J\\ -J & \bar E-\varepsilon/2 \end{pmatrix}.

The level gap is

ΔEgap=ε2+4J2.\Delta E_{\mathrm{gap}} = \sqrt{ \varepsilon^2+4J^2 }.

At resonance, ε=0\varepsilon=0, the minimum gap is 2J2J. If

∣ε∣≫2J,|\varepsilon|\gg2J,

the eigenstates are mostly localized even when ∣ε∣|\varepsilon| is tiny compared with the intrawell scale. An algebraically small perturbation can therefore dominate an exponentially small tunneling matrix element. The full mixing-angle and avoided-crossing analysis belongs to Coupled Wells and Avoided Crossings.

This sensitivity does not constitute spontaneous symmetry breaking in a finite one-particle system. At exact symmetry and finite barrier, the nondegenerate ground state remains even. Localization arises from state preparation, bias, measurement, environmental coupling, or a limiting procedure in which the splitting tends to zero.

For a symmetric numerical Hamiltonian:

  1. diagonalize even and odd parity sectors separately;
  2. pair states by energy, nodal structure, and localization within each well;
  3. compute ΔEn=En,o−En,e\Delta E_n=E_{n,o}-E_{n,e};
  4. verify that ΔEn≪δintra\Delta E_n\ll\delta_{\mathrm{intra}};
  5. increase the spatial domain, barrier resolution, and basis size;
  6. compare −log⁡ΔEn-\log\Delta E_n with the semiclassical action.

Separate parity sectors prevent an eigensolver from returning arbitrary rotations within a nearly degenerate numerical subspace. They do not remove floating-point cancellation in En,o−En,eE_{n,o}-E_{n,e}; sufficiently small gaps require higher precision or an alternative flux or kernel extraction.

Within the isolated symmetric doublet,

ZRL(T)ZLL(T)≃tanh⁡(ΔE T2ℏ).\frac{Z_{RL}(T)}{Z_{LL}(T)} \simeq \tanh \left( \frac{\Delta E\,T}{2\hbar} \right).

Hence

ΔE≃2ℏTartanh⁡[ZRL(T)ZLL(T)].\Delta E \simeq \frac{2\hbar}{T} \operatorname{artanh} \left[ \frac{Z_{RL}(T)}{Z_{LL}(T)} \right].

There is a useful Euclidean-time window:

ℏδintra≪T≲ℏΔE.\frac{\hbar}{\delta_{\mathrm{intra}}} \ll T \lesssim \frac{\hbar}{\Delta E}.

The first inequality suppresses higher intrawell states. The second avoids driving the ratio exponentially close to one, where extraction of ΔE\Delta E becomes ill-conditioned. Euclidean Time and Imaginary-Time Action develops this separation of projection and resolution timescales.

Double Delta Potential supplies an exact transcendental benchmark in which the even and odd binding momenta can be compared directly. For smooth wells, a robust validation sequence is:

exact numerical spectrum⟷Herring flux from a localized state⟷WKB or instanton asymptotics.\begin{gathered} \text{exact numerical spectrum} \\ \longleftrightarrow \text{Herring flux from a localized state} \\ \longleftrightarrow \text{WKB or instanton asymptotics}. \end{gathered}

Agreement of the exponent is a weaker test than agreement of the prefactor. Always state which one has been checked.

Double-Well Instanton Numerical Check implements this hierarchy for the quartic well, including parity blocks, basis-scale variation, a finite-difference cross-check, and a documented floating-point stopping point.

In ammonia, the two localized configurations correspond approximately to the nitrogen atom lying on opposite sides of the hydrogen plane. Tunneling produces inversion parity doublets visible in microwave and rovibrational spectroscopy. Isotopic substitution changes the effective masses and can strongly change the splitting.

The literal molecular problem is multidimensional: rotations, vibrations, and the inversion coordinate couple. A one-dimensional double well captures the origin of the doublet but not precision spectroscopy by itself.

In a persistent-current flux qubit, two low-energy circuit configurations carry currents in opposite directions. Magnetic flux controls their bias, while quantum tunneling through an effective circuit potential produces the minimum avoided-crossing gap.

The two-level Hamiltonian is genuinely useful, but the tunneling coordinate is a collective circuit degree of freedom rather than the position of one particle. Capacitance supplies the kinetic metric, Josephson energies shape the potential, and environmental noise limits coherent dynamics. A spectral gap may remain well defined even when dephasing prevents observation of many left-right oscillations.

Molecular conformers, proton transfer, and engineered wells

Section titled “Molecular conformers, proton transfer, and engineered wells”

The same structure appears in molecular conformations, hydrogen-transfer coordinates, semiconductor double wells, cold-atom double wells, and large-spin tunneling. Several qualifications can become decisive:

  • more than one tunneling path may contribute;
  • transverse zero-point energies modify the effective action;
  • Berry phases can make amplitudes interfere rather than simply add;
  • interactions can invalidate a one-particle two-state description;
  • dissipation can renormalize the tunneling coupling and destroy coherent oscillations.

The reusable statement is not a universal prefactor. It is the chain from localized configurations to an off-diagonal amplitude and then to a spectral splitting.

Before quoting a tunneling splitting, check:

  1. Observable: Is the target a bound-state energy difference rather than a transmission probability or resonance width?
  2. Doublet isolation: Is ΔE≪δintra\Delta E\ll\delta_{\mathrm{intra}}?
  3. Symmetry and bias: Are the wells truly degenerate to accuracy comparable with JJ?
  4. Basis: Were localized trial states orthogonalized, or was their overlap retained?
  5. Action: Are the turning points and reference energy appropriate to the state being split?
  6. Prefactor claim: Is the result exponential-only, one-loop, or numerically normalized?
  7. Instanton sectors: Does the observable require even, odd, or both transition-number sectors?
  8. Numerics: Can the method resolve the exponentially small difference without subtractive loss?
  9. Applications: Are multidimensional paths, interactions, and environmental decoherence negligible at the claimed accuracy?
  • Calling ΔE\Delta E a tunneling probability.
  • Squaring the WKB amplitude and using e−2W/ℏe^{-2W/\hbar} for a bound-state splitting.
  • Confusing the off-diagonal coupling JJ with the full symmetric splitting 2J2J.
  • Setting J=−⟨ℓ∣H∣r⟩J=-\langle\ell\vert H\vert r\rangle while ignoring nonzero overlap ss.
  • Treating localized states as exact stationary states at finite tunneling.
  • Using the zero-energy instanton action with an unrelated WKB prefactor.
  • Calling the gap away from resonance a pure tunneling splitting when bias dominates it.
  • Subtracting two double-precision eigenvalues after their difference has fallen below numerical resolution.
  • Inferring coherent oscillations from a spectral splitting without comparing the tunneling time with dephasing and leakage times.

Starting from exact parity states ∣e⟩\lvert e\rangle and ∣o⟩\lvert o\rangle, construct ∣L⟩\lvert L\rangle and ∣R⟩\lvert R\rangle. Show that the off-diagonal matrix element is −ΔE/2-\Delta E/2 and derive PR(t)P_R(t) for an initial left-localized state.

Solution

Define

∣L⟩=∣e⟩+∣o⟩2,∣R⟩=∣e⟩−∣o⟩2.\lvert L\rangle = \frac{\lvert e\rangle+\lvert o\rangle}{\sqrt2}, \qquad \lvert R\rangle = \frac{\lvert e\rangle-\lvert o\rangle}{\sqrt2}.

Then

⟨L∣H∣L⟩=⟨R∣H∣R⟩=Ee+Eo2=Eˉ,⟨L∣H∣R⟩=Ee−Eo2=−ΔE2.\begin{aligned} \langle L\vert H\vert L\rangle &= \langle R\vert H\vert R\rangle = \frac{E_e+E_o}{2} = \bar E, \\ \langle L\vert H\vert R\rangle &= \frac{E_e-E_o}{2} = - \frac{\Delta E}{2}. \end{aligned}

Thus J=ΔE/2J=\Delta E/2. Expanding the initial state in parity eigenstates gives

∣ψ(t)⟩=e−iEet/ℏ∣e⟩+e−iEot/ℏ∣o⟩2.\lvert\psi(t)\rangle = \frac{ e^{-iE_et/\hbar}\lvert e\rangle + e^{-iE_ot/\hbar}\lvert o\rangle }{\sqrt2}.

Projection onto ∣R⟩\lvert R\rangle yields

PR(t)=sin⁡2(ΔE t2ℏ).P_R(t) = \sin^2 \left( \frac{\Delta E\,t}{2\hbar} \right).

For real normalized trial states with overlap ss, diagonal energy EdE_d, and off-diagonal matrix element hh, derive the even and odd variational energies and the effective coupling.

Solution

The normalized combinations are

∣ψ±⟩=∣ℓ⟩±∣r⟩2(1±s).\lvert\psi_\pm\rangle = \frac{ \lvert\ell\rangle\pm\lvert r\rangle }{ \sqrt{2(1\pm s)} }.

Their expectation values are

E±=2Ed±2h2(1±s)=Ed±h1±s.E_\pm = \frac{ 2E_d\pm2h }{ 2(1\pm s) } = \frac{E_d\pm h}{1\pm s}.

Therefore

E−−E+=Ed−h1−s−Ed+h1+s=2(Eds−h)1−s2.\begin{aligned} E_--E_+ &= \frac{E_d-h}{1-s} - \frac{E_d+h}{1+s} \\ &= \frac{2(E_ds-h)}{1-s^2}. \end{aligned}

Identifying the splitting with 2Jeff2J_{\mathrm{eff}} gives

Jeff=Eds−h1−s2.J_{\mathrm{eff}} = \frac{E_ds-h}{1-s^2}.

Starting from

Hue=Eeue,Huo=Eouo,Hu_e=E_eu_e, \qquad Hu_o=E_ou_o,

derive the Wronskian identity on x≥0x\geq0 and obtain the midpoint formula in the high-barrier limit.

Solution

Multiply the even equation by uou_o, the odd equation by ueu_e, subtract, and integrate:

ΔE∫0∞ueuo dx=ℏ22m×[ueuo′−uoue′]x=0.\begin{aligned} \Delta E \int_0^\infty u_eu_o\,dx &= \frac{\hbar^2}{2m} \\ &\quad\times \left[ u_eu_o' - u_ou_e' \right]_{x=0}. \end{aligned}

Decay removes the boundary term at infinity. Parity gives

uo(0)=0,ue′(0)=0,u_o(0)=0, \qquad u_e'(0)=0,

so

ΔE∫0∞ueuo dx=ℏ22m×ue(0)uo′(0).\begin{aligned} \Delta E \int_0^\infty u_eu_o\,dx &= \frac{\hbar^2}{2m} \\ &\quad\times u_e(0)u_o'(0). \end{aligned}

For a well-isolated doublet,

∫0∞ueuo dx≃12,\int_0^\infty u_eu_o\,dx\simeq\frac12,

and the right-localized function obeys

ue(0)≃2 ψR(0),uo′(0)≃2 ψR′(0).\begin{aligned} u_e(0) &\simeq \sqrt2\,\psi_R(0), \\ u_o'(0) &\simeq \sqrt2\,\psi_R'(0). \end{aligned}

Hence

ΔE≃2ℏ2mψR(0)ψR′(0).\Delta E \simeq \frac{2\hbar^2}{m} \psi_R(0)\psi_R'(0).

The one-way forbidden action is WW. Explain why a transmission probability scales as e−2W/ℏe^{-2W/\hbar} while a tunneling splitting scales as e−W/ℏe^{-W/\hbar}.

Solution

The decaying barrier tail gives an amplitude proportional to

e−W/ℏ.e^{-W/\hbar}.

A transmission probability is a flux ratio quadratic in that amplitude, so

T∼e−2W/ℏ.T\sim e^{-2W/\hbar}.

The double-well splitting is linear in the off-diagonal matrix element JJ, and JJ is itself a tunneling amplitude:

J∼e−W/ℏ,ΔE=2J.J\sim e^{-W/\hbar}, \qquad \Delta E=2J.

Thus the splitting retains the one-way exponent.

5. Read the splitting from the instanton gas

Section titled “5. Read the splitting from the instanton gas”

Suppose

ZLL∝e−EpertT/ℏcosh⁡(ζT),ZRL∝e−EpertT/ℏsinh⁡(ζT).\begin{aligned} Z_{LL} &\propto e^{-E_{\mathrm{pert}}T/\hbar} \cosh(\zeta T), \\ Z_{RL} &\propto e^{-E_{\mathrm{pert}}T/\hbar} \sinh(\zeta T). \end{aligned}

Find the two energies and their splitting.

Solution

Using

cosh⁡(ζT)=12(eζT+e−ζT),\cosh(\zeta T) = \frac12 \left( e^{\zeta T} + e^{-\zeta T} \right),

the same-well kernel is a sum of two exponentials:

ZLL∝12[e−(Epert−ℏζ)T/ℏ+e−(Epert+ℏζ)T/ℏ].\begin{aligned} Z_{LL} &\propto \frac12 \Big[ e^{-(E_{\mathrm{pert}}-\hbar\zeta)T/\hbar} \\ &\qquad+ e^{-(E_{\mathrm{pert}}+\hbar\zeta)T/\hbar} \Big]. \end{aligned}

Therefore

Ee=Epert−ℏζ,Eo=Epert+ℏζ,E_e = E_{\mathrm{pert}}-\hbar\zeta, \qquad E_o = E_{\mathrm{pert}}+\hbar\zeta,

and

ΔE=2ℏζ.\Delta E=2\hbar\zeta.

For ζ=K1e−S0/ℏ\zeta=\mathcal K_1e^{-S_0/\hbar}, this is the one-instanton splitting formula.

Assume the potential and path are fixed, the prefactor change is negligible, and S(m)=CmS(m)=C\sqrt m. If m2=αm1m_2=\alpha m_1, estimate ΔE(m2)/ΔE(m1)\Delta E(m_2)/\Delta E(m_1).

Solution

Since

S(m2)=α S(m1),S(m_2) = \sqrt\alpha\,S(m_1),

the ratio is

ΔE(m2)ΔE(m1)≃exp⁡[−(α−1)S(m1)ℏ].\frac{\Delta E(m_2)}{\Delta E(m_1)} \simeq \exp \left[ - \left( \sqrt\alpha-1 \right) \frac{S(m_1)}{\hbar} \right].

Even when α\alpha is of order unity, the ratio can be extremely small if S(m1)/ℏ≫1S(m_1)/\hbar\gg1. In a molecule this estimate must be amended if isotope substitution changes the multidimensional path or transverse zero-point energies.

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