In models that naturally have a continuum, it is sometimes possible to find bound states with the application of a potential well. These states don’t come out of nowhere though and since they are combinations of continuum states, the continuum itself is altered. To begin to understand how the continuum is altered, we look at the simplest example here: A δ-function potential in one-dimension and with quadratic dispersion.

(1)12mψ(x)λδ(x)ψ(x)=Eψ(x).

The general strategy here is to convert this potential into a matching condition between left and right parts of space. In particular, if we integrate x from 0 to 0+, we get

(2)12m[ψ(0+)ψ(0)]=λψ(0).

The bound state solution to this problem is a simple exponential

(3)ψ0(x)=mλemλ|x|,E=12mλ2
Expand for derivation

We require the bound state to be square integrable, so ψ0(x)=Neκx for x>0 and ψ0(x)=Neκx for x<0. In both cases, we can evaluate (1)

(4)κ22mψ0(x)=Eψ0(x),κ=2mE.

Using our forms of ψ0(x) on either side of zero, we have ψ0(0+)=κψ0(0) and ψ0(0)=+κψ0(0). Putting these into (2), we have

(5)κmψ0(0)=λψ0(0).

This means that κ=λm, and matching this to (4) we find E=12mλ2. All that is left is normalization and simply

(6)1=dx|ψ0(x)|2=20dxN2e2κx=N2κ.

This gives us N=κ=λm, completing our derivation.


The delta function potential (red) along with the resulting bound state (gray).

But what about the continuum? First, sine waves automatically satisfy (1), and we have

(7)ψks(x)=sin(kx),E=k22m.

It is worth noting that these wave functions are normalized such that

(8)dxψks(x)ψks(x)=πδ(kk)

The continuum states that are modified are the cosine waves

(9)ψkc(x)=11+λ2m2/k2[cos(kx)λmksin|kx|],E=k22m.

This is again chosen such that dxψkc(x)ψkc(x)=πδ(kk).

Expand for derivation

First, ψks(x)=sin(kx) is a complete basis for antisymmetric wavefunctions, and therefore, we know that ψkc(x)=ψkc(x) in order to maintain orthogonality with ψks(x). This implies that if for x>0 we have ψkc(x)=Acos(kx)+Bsin(kx), then for x<0, ψkc(x)=Acos(kx)Bsin(kx) justifying our functional form.

We have already guaranteed continuity across x=0, so now we just need to satisfy the matching conditions (2) for which we have ψkc(0+)=Bk and ψkc(0)=Bk and therefore by (2)

(10)Bkm=AλB=λmkA

All that is left is normalization (fixing A). For this, we introduce a regulator eδ|x| and take it to be small

(11)dxψkc(x)ψpc(x)eδ|x|=2A20dx(coskxλmksinkx)(cospxλmpsinpx)eδx=2A2δ(k2+p2+δ22δλ2m2+2λ4m4)(k2p2)2+2(k2+p2)δ2+δ4

If kp, then this expression goes to zero as δ0, and it appears to diverge with 1/δ if k=p, a hallmark of a Dirac delta function. In fact, making sure this integrates to π when we integrate with respect to k or p gives us exactly

(12)0dp2A2δ(k2+p2+δ22δλ2m2+2λ4m4)(k2p2)2+2(k2+p2)δ2+δ4=A2π(λ2m2+k2λmδ+δ2)k2+δ2

As δ0 then, we obtain

(13)A=11+λ2m2/k2,

completing this derivation.


Taken together, we can now define the (local) density of states for the continuum

(14)ρ(E;x)=0dkπ(|ψkc(x)|2+|ψks(x)|2)δ(Ek2/(2m))

To address this, we want to find the difference from the continuum which we call

(15)ρ0(E;x)=0dkπ(cos2(kx)+sin2(kx))δ(Ek2/(2m))

Subtracting these

(16)Δρ(E;x)=ρ(E;x)ρ0(E;x),

With a bit of work, we can find

(17)Δρ(k22m;x)=mkπ(mλ)2cos(2kx)+mλksin|2kx|(mλ)2+k2.

We can finally, integrate this over all energies

(18)0dEΔρ(E;x)=mλe2mλ|x|=|ψ0(x)|2.

As you might suspect: the continuum is depleted in the exact way to compensate the bound state. This is known as the Friedel sum rule. But which continuum states are playing the largest roles? For this, we can take

Δρ(E)limδ0+dxΔρ(E,x)eδ|x|,

from which we find

(19)Δρ(E)dE=[12δ(k0+)1πmλ(mλ)2+k2]dk,E=k22m

We can tell from this that half of the weight comes from the k=0 (constant) mode. The rest of the weight comes from higher k’s distributed like a Lorentzian. If we include the ground state as a positive δ-function, we get:

The change in density of states for with delta functions artificially broadened to make them visible. This function integrates to zero: the Friedel sum rule in action.

This is a simple example of how charge can be pulled from the continuum to make a bound state: leaving a depletion of density in the continuum.