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Double Delta Potential

The double delta potential is the simplest exactly solvable model of two coupled attractive wells. It has enough structure to show tunneling splitting, even and odd parity states, and the bonding-antibonding pattern familiar from molecules, while remaining algebraically much simpler than a smooth double well.

Take two identical attractive delta wells separated by distance 2a2a:

V(x)=−g[δ(x−a)+δ(x+a)],g>0.V(x) =-g\left[ \delta(x-a)+\delta(x+a) \right], \qquad g\gt0.

The parameter aa is half the separation, and gg is the integrated strength of each well. Define

κ0=mgℏ2.\kappa_0=\frac{mg}{\hbar^2}.

For a single attractive delta well of strength gg, the bound-state decay constant is κ0\kappa_0. In the double-well problem, the two delta wells communicate through the evanescent tails between them. That communication splits the two one-well states into a lower even state and, when the separation and strength are large enough, an upper odd state.

The stationary Schrödinger equation is

−ℏ22mψ′′(x)−g[δ(x−a)+δ(x+a)]ψ(x)=Eψ(x).-\frac{\hbar^2}{2m}\psi''(x) -g\left[ \delta(x-a)+\delta(x+a) \right]\psi(x) =E\psi(x).

Away from x=±ax=\pm a, the particle is free. A bound state has E<0E\lt0, so write

E=−ℏ2κ22m,κ>0.E=-\frac{\hbar^2\kappa^2}{2m}, \qquad \kappa\gt0.

At each delta well the wavefunction is continuous, while the derivative jumps. For a well at x=x0x=x_0,

ψ(x0−)=ψ(x0+)=ψ(x0),\psi(x_0^-)=\psi(x_0^+)=\psi(x_0),

and

ψ′(x0+)−ψ′(x0−)=−2κ0ψ(x0).\psi'(x_0^+)-\psi'(x_0^-) =-2\kappa_0\psi(x_0).

These matching conditions are inherited directly from the Delta-Function Potential. The only new feature is that the two singular points must be matched simultaneously.

The potential is symmetric:

V(x)=V(−x).V(x)=V(-x).

Therefore bound states can be chosen with definite parity. The even state is lower because it has no node between the wells. The odd state, when it exists, has a node at the origin and is higher in energy.

This parity reduction is not just a convenience. It turns one coupled matching problem into two scalar equations:

κe=κ0(1+e−2κea),\kappa_{\mathrm e} =\kappa_0\left(1+e^{-2\kappa_{\mathrm e}a}\right),

for the even state, and

κo=κ0(1−e−2κoa),\kappa_{\mathrm o} =\kappa_0\left(1-e^{-2\kappa_{\mathrm o}a}\right),

for the odd state. The rest of the page derives and interprets these equations.

For an even bound state, choose the form

ψe(x)={Be−κ(x−a),x>a,Acosh⁡(κx),−a<x<a,Beκ(x+a),x<−a.\psi_{\mathrm e}(x) = \begin{cases} B e^{-\kappa(x-a)}, & x\gt a,\\ A\cosh(\kappa x), & -a\lt x\lt a,\\ B e^{\kappa(x+a)}, & x\lt-a. \end{cases}

Continuity at x=ax=a gives

B=Acosh⁡(κa).B=A\cosh(\kappa a).

The derivative just outside the right well is

ψe′(a+)=−κB,\psi_{\mathrm e}'(a^+)=-\kappa B,

while the derivative just inside is

ψe′(a−)=Aκsinh⁡(κa).\psi_{\mathrm e}'(a^-)=A\kappa\sinh(\kappa a).

The jump condition at x=ax=a gives

−κB−Aκsinh⁡(κa)=−2κ0B.-\kappa B-A\kappa\sinh(\kappa a) =-2\kappa_0B.

Using B=Acosh⁡(κa)B=A\cosh(\kappa a),

κ[1+tanh⁡(κa)]=2κ0.\kappa\left[ 1+\tanh(\kappa a) \right] =2\kappa_0.

Equivalently,

κ=κ0(1+e−2κa).\kappa =\kappa_0\left(1+e^{-2\kappa a}\right).

This equation has one positive solution for every g>0g\gt0 and a>0a\gt0. The even bound state therefore always exists.

The energy is

Ee=−ℏ2κe22m.E_{\mathrm e} =-\frac{\hbar^2\kappa_{\mathrm e}^2}{2m}.

Because κe>κ0\kappa_{\mathrm e}\gt\kappa_0, the even state is more deeply bound than the bound state of a single isolated delta well of strength gg.

For an odd bound state, use

ψo(x)={Be−κ(x−a),x>a,Asinh⁡(κx),−a<x<a,−Beκ(x+a),x<−a.\psi_{\mathrm o}(x) = \begin{cases} B e^{-\kappa(x-a)}, & x\gt a,\\ A\sinh(\kappa x), & -a\lt x\lt a,\\ -B e^{\kappa(x+a)}, & x\lt-a. \end{cases}

Continuity at x=ax=a gives

B=Asinh⁡(κa).B=A\sinh(\kappa a).

The derivative jump at x=ax=a is

−κB−Aκcosh⁡(κa)=−2κ0B.-\kappa B-A\kappa\cosh(\kappa a) =-2\kappa_0B.

After dividing by BB,

κ[1+coth⁡(κa)]=2κ0.\kappa\left[ 1+\coth(\kappa a) \right] =2\kappa_0.

Equivalently,

κ=κ0(1−e−2κa).\kappa =\kappa_0\left(1-e^{-2\kappa a}\right).

This equation does not always have a positive solution. Near κ=0\kappa=0, the right-hand side behaves as

κ0(1−e−2κa)=2κ0a κ+O(κ2).\kappa_0\left(1-e^{-2\kappa a}\right) =2\kappa_0a\,\kappa+O(\kappa^2).

A nonzero positive intersection requires

2κ0a>1.2\kappa_0a\gt1.

Thus the odd bound state exists only when the wells are sufficiently strong or sufficiently separated:

2mgaℏ2>1.\frac{2mga}{\hbar^2}\gt1.

At the threshold 2κ0a=12\kappa_0a=1, the odd solution reaches κ=0\kappa=0 and is not a normalizable bound state. Below threshold, the model has only the even bound state.

The odd-state energy, when it exists, is

Eo=−ℏ2κo22m.E_{\mathrm o} =-\frac{\hbar^2\kappa_{\mathrm o}^2}{2m}.

Since κe>κo\kappa_{\mathrm e}\gt\kappa_{\mathrm o}, the odd state lies above the even state:

Eo>Ee.E_{\mathrm o}\gt E_{\mathrm e}.

When both states exist, the splitting is

ΔE=Eo−Ee=ℏ22m(κe2−κo2).\Delta E =E_{\mathrm o}-E_{\mathrm e} =\frac{\hbar^2}{2m} \left( \kappa_{\mathrm e}^2-\kappa_{\mathrm o}^2 \right).

For large separation, aκ0≫1a\kappa_0\gg1, the two wells are almost independent. The exponential overlap is small, and the two transcendental equations give

κe≈κ0(1+e−2κ0a),κo≈κ0(1−e−2κ0a).\kappa_{\mathrm e} \approx \kappa_0\left(1+e^{-2\kappa_0a}\right), \qquad \kappa_{\mathrm o} \approx \kappa_0\left(1-e^{-2\kappa_0a}\right).

Therefore

ΔE≈2ℏ2κ02me−2κ0a.\Delta E \approx \frac{2\hbar^2\kappa_0^2}{m} e^{-2\kappa_0a}.

This exponential dependence is the exact-model version of tunneling splitting. The two isolated wells would give degenerate states. Finite overlap through the middle region produces a lower even combination and a higher odd combination.

Let ϕL\phi_L and ϕR\phi_R denote approximate bound states localized near the left and right delta wells when aa is large. The exact low-energy states are approximately

ψe≈12(ϕL+ϕR),\psi_{\mathrm e} \approx \frac{1}{\sqrt2} \left( \phi_L+\phi_R \right),

and

ψo≈12(ϕL−ϕR).\psi_{\mathrm o} \approx \frac{1}{\sqrt2} \left( \phi_L-\phi_R \right).

The even state has constructive amplitude between the wells and no node at the center. It is the bonding state in the elementary molecular-orbital analogy. The odd state has destructive amplitude at the center and one node. It is the antibonding state.

The same structure is captured abstractly by a two-state Hamiltonian

Heff=(E0−K−KE0),K>0,H_{\mathrm{eff}} = \begin{pmatrix} E_0 & -K \\ -K & E_0 \end{pmatrix}, \qquad K\gt0,

whose eigenstates are the symmetric and antisymmetric combinations. The exact double-delta solution shows where this two-state picture comes from and when the splitting is exponentially small. The finite-dimensional version is developed in Two-State Hamiltonians.

When the two wells approach each other, the potential tends to a single delta well of twice the strength:

−g[δ(x−a)+δ(x+a)]⟶−2gδ(x).-g\left[ \delta(x-a)+\delta(x+a) \right] \longrightarrow -2g\delta(x).

The even equation becomes

κe→2κ0,\kappa_{\mathrm e}\to 2\kappa_0,

which is exactly the single-delta result for strength 2g2g. The energy approaches

Ee→−ℏ2(2κ0)22m=−2mg2ℏ2.E_{\mathrm e} \to -\frac{\hbar^2(2\kappa_0)^2}{2m} =-\frac{2mg^2}{\hbar^2}.

The odd state disappears in this limit. Physically, an odd wavefunction vanishes at the origin, so it cannot benefit from a delta attraction concentrated at the origin after the two wells merge.

The double delta model is not meant to be a realistic molecular potential. Its value is conceptual:

  • it shows exactly how parity splits a pair of nearly degenerate localized states;
  • it gives an explicit exponential splitting at large separation;
  • it displays a threshold for the first odd bound state;
  • it separates matching-condition algebra from WKB approximation;
  • it provides a clean bridge from one-dimensional bound states to two-level systems.

The smoother Double-Well Potential page keeps the same physical ideas but drops exact solvability. Detailed WKB estimates for smooth barriers belong to Barrier Penetration and Tunneling.

  • Requiring ψ′\psi' to be continuous at x=±ax=\pm a.
  • Forgetting that the wavefunction itself remains continuous at each delta well.
  • Assuming the odd bound state always exists.
  • Confusing the half-separation aa with the full well separation 2a2a.
  • Calling the localized left and right states exact energy eigenstates when the potential is symmetric.
  • Missing the sign difference between the even equation and the odd equation.
  • Treating the large-separation exponential estimate as valid near the odd-state threshold.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics, Wiley, 1977.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • S. Flügge, Practical Quantum Mechanics, Springer, 1999.
  1. Derive the even-state equation for the double delta potential.
Solution

Use

ψe(x)={Be−κ(x−a),x>a,Acosh⁡(κx),−a<x<a,Beκ(x+a),x<−a.\psi_{\mathrm e}(x) = \begin{cases} B e^{-\kappa(x-a)}, & x\gt a,\\ A\cosh(\kappa x), & -a\lt x\lt a,\\ B e^{\kappa(x+a)}, & x\lt-a. \end{cases}

Continuity at x=ax=a gives

B=Acosh⁡(κa).B=A\cosh(\kappa a).

The derivative jump is

−κB−Aκsinh⁡(κa)=−2κ0B.-\kappa B-A\kappa\sinh(\kappa a) =-2\kappa_0B.

Divide by BB and use Asinh⁡(κa)/B=tanh⁡(κa)A\sinh(\kappa a)/B=\tanh(\kappa a):

κ[1+tanh⁡(κa)]=2κ0.\kappa\left[ 1+\tanh(\kappa a) \right] =2\kappa_0.

Since

1+tanh⁡z=21+e−2z,1+\tanh z =\frac{2}{1+e^{-2z}},

the equation becomes

κ=κ0(1+e−2κa).\kappa =\kappa_0\left(1+e^{-2\kappa a}\right).
  1. Show that the odd bound state requires 2κ0a>12\kappa_0a\gt1.
Solution

The odd-state equation is

κ=κ0(1−e−2κa).\kappa =\kappa_0\left(1-e^{-2\kappa a}\right).

For small κ\kappa,

1−e−2κa=2κa+O(κ2).1-e^{-2\kappa a} =2\kappa a+O(\kappa^2).

Thus the right-hand side initially has slope 2κ0a2\kappa_0a as a function of κ\kappa, while the left-hand side has slope 11. A positive nonzero intersection can emerge from threshold only if

2κ0a>1.2\kappa_0a\gt1.

At equality the solution is at κ=0\kappa=0, which is not a normalizable bound state.

  1. Find the small-separation limit of the even bound-state energy.
Solution

As a→0a\to0, the double delta potential tends to

V(x)→−2gδ(x).V(x)\to -2g\delta(x).

Equivalently, the even equation gives

κe=κ0(1+e−2κea)→2κ0.\kappa_{\mathrm e} =\kappa_0\left(1+e^{-2\kappa_{\mathrm e}a}\right) \to 2\kappa_0.

Therefore

Ee→−ℏ2(2κ0)22m=−2mg2ℏ2.E_{\mathrm e} \to -\frac{\hbar^2(2\kappa_0)^2}{2m} =-\frac{2mg^2}{\hbar^2}.
  1. Estimate the large-separation splitting.
Solution

For aκ0≫1a\kappa_0\gg1, insert κ≈κ0\kappa\approx\kappa_0 into the small exponential terms:

κe≈κ0(1+e−2κ0a),κo≈κ0(1−e−2κ0a).\kappa_{\mathrm e} \approx \kappa_0\left(1+e^{-2\kappa_0a}\right), \qquad \kappa_{\mathrm o} \approx \kappa_0\left(1-e^{-2\kappa_0a}\right).

Then

ΔE=ℏ22m(κe2−κo2)≈2ℏ2κ02me−2κ0a.\Delta E = \frac{\hbar^2}{2m} \left( \kappa_{\mathrm e}^2-\kappa_{\mathrm o}^2 \right) \approx \frac{2\hbar^2\kappa_0^2}{m} e^{-2\kappa_0a}.

The splitting is exponentially small in the separation measured in units of the single-well localization length.