The scattering matrix. The theory of scattering generalizes in a pretty obvious way to arbitrary localized potentials to the left (Region I),V(x)=0soψ(x)=Aeikx+Be-ikx,wherek2mE

To the right (Region III),V(x)is again zero, soψ(x)=Feikx+Ge-ikxIn between (Region II), of course, I can't tell you what is until you specify the potential, but because the Schrödinger equation is a linear, second-order differential equation, the general solution has got to be of the form

ψwhere f(x)and g(x)are two linearly independent particular solutions. 48 There will be four boundary conditions (two joining Regions I and II, and two joining Regions II and III). Two of these can be used to eliminate C and D, and the other two can be "solved" for B and F in terms of \(A\) and G

B=S11A+S12G.F=S21A+S22G

The four coefficientsSijwhich depend on k (and hence on E), constitute a2×2matrix s called the scattering matrix (or S-matrix, for short). The S-matrix tells you the outgoing amplitudes (B and F) in terms of the incoming amplitudes (A and G):

(BF)=(S11S21S21S22)(AG)

In the typical case of scattering from the left, G=0so the reflection and transmission coefficients are

Rl=|B|2|A|2|G=0=|S11|2.TI=|F|2|A|2|G=0=|S2|2.

For scattering from the right, and

Rr=|F|2|G|2A=0=|S22|2.Tr=|B|2|G|2A=0=|S12|2.

(a) Construct the S-matrix for scattering from a delta-function well (Equation 2.114). (b) Construct the S-matrix for the finite square well (Equation 2.145). Hint: This requires no new work, if you carefully exploit the symmetry of the problem.

Short Answer

Expert verified

(a) The required S matrix is11-iβiβ11iβ.

(b) The S-matrix for the finite square well is

S=e-2ikacos2la-ik2+l22klsin2lail2+k22klsin2la11il2+k22klsin2la

Step by step solution

01

Define the Schrödinger equation

A differential equation that describes matter in quantum mechanics in terms of the wave-like properties of particles in a field. Its answer is related to a particle's probability density in space and time.

02

Step 2: Construct the S-matrix

(a)

Given equation from 2.133 :

F+G=A+B …………….. (1)

Again from the equation 2.135 :

F-G=(1+2)A-(1-2)Bβ=/2k.(2)

Subtracting equations 1 and 2 as:

2G=-2A+21-iβBB=11-iβA+G

Then multiply equation 1 by(1-2iβ) as:

role="math" localid="1658292860542" 21-F-2iβG=2AF=11-A+iβGS=11-11

Hence, the S matrix is 11-iβiβ11iβ.

03

Form the matrix.

(b)

Given infinite square well:

S=11-11S21=e-2ikacos2la-ik2+l22klsin2laS11=il2+k22klsin2lae-2ikacos2la-ik2+l22klsin2laS=e-2ikacos2la-ik2+l22klsin2lail2+k22klsin2la11il2+k22klsin2la

Thus, the S-matrix for the finite square wellS=e-2ikacos2la-ik2+l22klsin2lail2+k22klsin2la11il2+k22klsin2la.

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Most popular questions from this chapter

Solve the time-independent Schrodinger equation with appropriate boundary conditions for the “centered” infinite square well: V(x)=0(for-a<x<+a), V(x)=α(otherwise). Check that your allowed energies are consistent with mine (Equation 2.30), and confirm that your ψ'scan be obtained from mine (Equation 2.31) by the substitution x → (x + a)/2 (and appropriate renormalization). Sketch your first three solutions, and compare Figure 2.2. Note that the width of the well is now 2a.

Although the overall phase constant of the wave function is of no physical significance (it cancels out whenever you calculate a measurable quantity), the relative phase of the coefficients in Equation 2.17 does matter. For example, suppose we change the relative phase of ψ1andψ2in problem 2.5:ψ(x,0)=A[ψ1x+eiϕψ2x]Where ϕis some constant. Find ψ(x,t),|ψx,t|2, and (x), and compare your results with what you got before. Study the special cases ϕ=π2andϕ=π.

Evaluate the following integrals:

(a)-3+1(x3-3x2+2x-1)δ(x+2)dx.

(b).0[cos(3x)+2]δ(x-π)dx

(c)_1+1exp(lxl+3)δ(x-2)dx

A particle of mass m is in the ground state of the infinite square well (Evaluation 2.19). Suddenly the well expands to twice its original size – the right wall moving from a to 2a – leaving the wave function (momentarily) undisturbed. The energy of the particle is now measured.

  1. What is the most probable result? What is the probability of getting that result?
  2. What is the next most probable result, and what is its probability?
  3. What is the expectation value of the energy? (Hint: if you find yourself confronted with an infinite series, try another method)

A particle in the infinite square well has as its initial wave function an even mixture of the first two stationary states:

Ψ(x,0)=A[ψ1(x)+ψ2(x)]

You can look up the series

116+136+156+=π6960

and

114+134+154+=π496

in math tables. under "Sums of Reciprocal Powers" or "Riemann Zeta Function."

(a) Normalize Ψ(x,0). (That is, find A. This is very easy, if you exploit the orthonormality of ψ1 and ψ2. Recall that, having ψnormalized at , t=0 , you can rest assured that is stays normalized—if you doubt this, check it explicitly after doing part(b).

(b) FindΨ(x,t) and|Ψ(x,t)|2 . Express the latter as a sinusoidal function of time. To simplify the result, letωπ22ma2

(c)Compute x . Notice that it oscillates in time. What is the angular frequency of the oscillation? What is the amplitude of the oscillation?(If your amplitude is greater than a2, go directly to jail.

(d) Compute p.

(e) If you measured the energy of this particle, what values might you get, and what is the probability of getting each of them? Find the expectation value ofH . How does it compare with E1 and E2

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