(a) Use Equation 10.42 to calculate the geometric phase change when the infinite square well expands adiabatically from width w1to width w2. Comment on this result.

(b) If the expansion occurs at a constant rate(dw/dt=v), what is the dynamic phase change for this process?

(c) If the well now contracts back to its original size, what is Berry's phase for the cycle?

Short Answer

Expert verified

(a) The geometric phase isγnt=0.

(b) The dynamic phase change for this process islocalid="1656067997518" θnt=n2ττ2h2mv1w21w1.

(c) The Berry’s phase is zero.

Step by step solution

01

Define Geometric phase.

Geometric phase is a phase difference gained during the course of a cycle when a system is subjected to cyclic adiabatic processes, which derives from the geometrical features of the Hamiltonian's parameter space in both classical and quantum mechanics.

02

Obtain the geometric phase.

(a)

Let an infinite square well whose right wall moves as its position is a function of time be,ψnx=2wsinnττwx… (1)

The equation 10.42 is given by, γnt=iRiRIψnIψnRdR… (2)

In this case, the width of the well isrole="math" localid="1656068288003" Rt=wt. So,

ψnR=2121w3/2sinnττwx+2wnττw2xcosnττwx

Thus,

ψn|ψnR&=0wψnψnRdx=1w20wsin2nττwxdx2nττw30wxsinnττwxcosnττwxdx=1w2w2nττw30wxsin2nττwxdx=12wnττw3w2nττ2sin2nττwxwx2nττcos2nττwx0w=12w+12w=0

Substitute the value in the equation (2) to get:

γnt0

03

Obtain the dynamic phase.

(b)

The dynamic phase change for this process is given by,θnt=1h0tEnt'dt'… (3)

But the energy in this case isEn=nττh22mw2 . Thus,

θnt=1h0tn2ττ2h22mw2dt'=n2ττ2h2m1w2dt'dwdw=n2ττ2h2mw1w21w2dt'dwdw=n2ττ2h2m1w21w1θnt=n2ττ2h2mv1w21w1

(c)

The Berry’s phase for the cycle will be zero.

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Most popular questions from this chapter

Work out to analog to Equation 10.62 for a particle of spin I.

The adiabatic approximation can be regarded as the first term in an adiabatic series for the coefficientsCm(t)in Equation. Suppose the system starts out in theth state; in the adiabatic approximation, it remains in theth state, picking up only a time-dependent geometric phase factor (Equation):

Cm(t)=δmneiyn(t)

(a) Substitute this into the right side of Equationto obtain the "first correction" to adiabaticity:

Cm(t)=cm(0)-0t<Ψmt'lt'Ψn(t')>eiyn(t')ei(θn(t')-θt!(t'))dt'.[10.95]

This enables us to calculate transition probabilities in the nearly adiabatic regime. To develop the "second correction," we would insert Equationon the right side of Equation, and so on.


(b) As an example, apply Equationto the driven oscillator (Problem). Show that (in the near-adiabatic approximation) transitions are possible only to the two immediately adjacent levels, for which

Cn+1(t)=-2hn+10tf˙(t')eiωtdt'Cn+1(t)=-2hn0tf˙(t')eiωtdt'

(a) Derive the equation 10.67 from Equation 10.65.

(b) Derive Equation 10.79, starting with Equation 10.78.

The delta function well (Equation 2.114) supports a single bound state (Equation 2.129). Calculate the geometric phase change whengradually increases fromα1toα2. If the increase occurs at a constant rate, (/dt=c)what is the dynamic phase change for this process?

The driven harmonic oscillator. Suppose the one-dimensional harmonic oscillator (mass m, frequency ω) is subjected to a driving force of the form F(t) = m ω² f(t) , where f(t) is some specified function. (I have factored out m ω² for notational convenience; f(t) has the dimensions of length.) The Hamiltonian is

H(t)=-h22m2x2+12mω2x2-mω2xf(t) (10.90).

Assume that the force was first turned on at time t=0:f(t)=0fort0t=0.This system can be solved exactly, both in classical mechanics and in quantum mechanics.

(a)Determine the classical position of the oscillator, assuming it started from rest at the origin (xc0=xc˙0=0). Answer:

xc(t)=ω0tf(t')sin[t-t']dt'.(10.91).

(b) Show that the solution to the (time-dependent) Schrödinger equation for this oscillator, assuming it started out in the nth state of the undriven oscillator (ψx,0=ψnx)whereψn(x)is given by Equation 2.61), can be written as

ψn(x)=An(a^+)nψ0(x),withEn=(n+12)hω (2.61).

localid="1656143246748" ψ(x,1)=ψn(x-xc)eih[-(n+12)hωt+mx˙c(x-xc2)+mω220tf(t')xx(t')dt'](10.92).

(c) Show that the Eigen functions and Eigenvalues of H(t) are

ψn(x,t)=ψn(x-f);En(t)=(n+12)hω-12mω2f2 (10.93).

(d) Show that in the adiabatic approximation the classical position (Equation 10.91) reduces to xc(t)f(t)State the precise criterion for adiabaticity, in this context, as a constraint on the time derivative of f. Hint: Write sin[ωt-t']as(1/dt')cos[ωt-t']and use integration by parts.

(e) Confirm the adiabatic theorem for this example, by using the results in (c) and (d) to show that

ψ(x,t)ψn(x,t)eiθn(t)eiγn(t)(10.94).

Check that the dynamic phase has the correct form (Equation 9.92). Is the geometric phase what you would expect?

eiθn(t),whereθn(t)1hhtEn(t')dt'(9.92).

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