Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Check the Equation 10.31 satisfies the time-dependent Schrodinger equation for the Hamiltonian in Equation 10.25. Also confirm Equation 10.33, and show that the sum of the squares of the coefficients is 1, as required for normalization.

Short Answer

Expert verified

Hence showed thatih𝜕x𝜕t=Hx

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 derivative of the function.

To show that : ih𝜕x𝜕t=Hx..(1)

Here, Equation 10.25....H=hω12cosαeiωtsinαeiωtsinα-cosα....(2)and

Equation10.31....x(t)=cos(λt/2)-i(ω1-ω)λsin(λt/2)cos(α/2)e-iωt/2cos(λt/2)-i(ω1+ω)λsin(λt/2)sin(α/2)e+iωt/2.....(3)

The derivative of the equation (3) with respect to t is,

role="math" localid="1656062904380" ih𝜕x𝜕t=ihλ2-sinλt2-i(ω1-ω)λcosλt2cosα2e-iωt/2-iω2cosλt2-i(ω1-ω)λsinλt2cosα2e-iωt/2λ2-sinλt2-i(ω1-ω)λcosλt2sinα2eiωt/2+λ2cosλt2-i(ω1-ω)λsinλt2sinα2eiωt/2

From (2) and (3), the equation (1) becomes,

Hx(t)=hω12cosαcosλt2-i(ω1-ω)λsinλt2cosα2e-iωt/2+e-iωtsinαcosλt2-i(ω1-ω)λsinλt2cosα2eiωt/2e-iωtcosαcosλt2-i(ω1-ω)λsinλt2cosα2e-iωt/2-cosαcosλt2-i(ω1-ω)λsinλt2sinα2eiωt/2

03

Show that the two matrices are identical.

Start the upper element:

ihλ2-sinλt2-i(ω1-ω)λcosλt2cosα2e-iωt/2-iω2cosλt2-i(ω1-ω')λsinλt2cosα2e-iωt/2=hω12cosαcosλt2-i(ω1-ω)λsinλt2cosα2eiωt/2+e-iωtcosλt2-i(ω1-ω)λsinλt2sinα2eiωt/2

Cancel the like terms and substitute sinα=2sinα2cosα2in the last term to get:

role="math" localid="1656064057976" iλ-sinλt2-i(ω1-ω)λcosλt2-iω2cosλt2-i(ω1-ω')λsinλt2..........(4)=ω1cosαcosλl2-i(ω1-ω)λsinλt2+2sin2α2cosλt2-i(ω1-ω)λsinλt2

The sum of sine’s terms is zero, hence,

iλsinλt2[-ω2-ω12+2ωω1cosα-ω1+ω2+(ω12-ωω1)cosα+(ω12+ωω1)(1-cosα)]=-iλsinλt2[-ω12-2ωω1cosα-ω1ω2+ω12cosα-ωω1cosα+ω12+ωω1-ω12cosα-ωω1cosα=0Similarly,thesamethinforthelowertermisih𝜕x𝜕tHx.

04

Confirm the equation 10.33.

Let the equation 10.33 be, x(t)=cosλt2-i(ω1-ωcosα)λsinλt2e-iωt/2x+(t)+iωλsinαsinλt2e-iωt/2x-(t)

Here, x+(t)=cos(α/2)eiωtsin(α/2),x-(t)=e-iωtsin(α/2)cos(α/2).Thus,

cosλt2-i(ω1-ωcosα)λsinλt2e-iωt/2cosα2-eiωtsinα2iωλsinαsinλt2e-iωt/2sinα2-eiωtcosα2=αβ

Here, localid="1656067456488" α=cosλt2-iω1λsinλt2cosα2+iωλcosαcosα2+sinαsinα2sinλt2e-iωt/2butcosαcosα2+sinαsinα2=cosα-α2=cosα2.α=cosλt2-i(ω1-ω)λsinλt2cosα2e-iωt/2

Hence, the upper term of the equation (3) is confirmed.

Forβ:β=cosλt2-iω1λλt2sinα2+iωλcosαsinα2-sinαcosα2sinλt2eiωt/2

role="math" localid="1656068970462" But,cosαcosα2-sinαcosα2=sinα2-α=-sinα2.So,β=cosλt2-i(ω1+ω)λsinλt2sinα2eiωt/2

Hence, the lower term of the equation (3) is confirmed.

The coefficients are normalized. Hence,

c+2+c-2=cos2λt2+(ω1-ωcosα)2λ2sin2λt2+ωλsinαsinλt22=cos2λt2+sin2λt2(ω1-ωcosα)2λ2+ωλsinα2=cos2λt2+sin2λt2ω1+ω12-2ωω1cosαλ2=cos2λt2+sin2λt2ω2+ω12-2ωω1cosαω2+ω12-2ωω1cosα

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

The case of an infinite square well whose right wall expands at a constant velocity (v) can be solved exactly. A complete set of solutions isΦn(x,t)2wsin(ux)ei(mvx22Enint)/2w

Where w(t)a+vtis the (instantaneous) width of the well andEnin2π22/2ma2 is the nthallowed energy of the original well (width). The general solution is a linear combination of theΦ's:

Ψ(x,t)=n=1cnΦn(x,t)

the coefficients cnare independent oft

a. Check that Equation \(10.3\) satisfies the time-dependent Schrödinger equation, with the appropriate boundary conditions.


(b) Suppose a particle starts outrole="math" localid="1659010978273" (t=0) in the ground state of the initial well:

role="math" localid="1659011031703" Ψ(x,0)=2asin(πax)

Show that the expansion coefficients can be written in the form

cn=2π0πeiα2sin(nz)sin(z)dz

Where αmva/2π2is a dimensionless measure of the speed with which the well expands. (Unfortunately, this integral cannot be evaluated in terms of elementary functions.)

(c) Suppose we allow the well to expand to twice its original width, so the "external" time is given byw(Te)=2a The "internal" time is the period of the time-dependent exponential factor in the (initial) ground state. Determine TeandTi show that the adiabatic regime corresponds to α1sothatexp(iαz2)1over the domain of integration. Use this to determine the expansion coefficients,Cn Construct Ψ(x,t)and confirm that it is consistent with the adiabatic theorem.

(d) Show that the phase factor inrole="math" localid="1659011579812" Ψ(x,t) can be written in the form

θ(t)=10tE1(t')dt'.

WhereEn(t)n2π22/2mw2 is the instantaneous eigenvalue, at timet Comment on this result.

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'

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?

Show that if ψn is real, the geometric phase vanishes. (Problems 10.3 and 10.4 are examples of this.) You might try to beat the rap by tacking an unnecessary (but perfectly legal) phase factor onto the eigenfunctions: ψn(t)eiφnψn(t), whereϕn(R) is an arbitrary (real) function. Try it. You'll get a nonzero geometric phase, all right, but note what happens when you put it back into Equation 10.23. And for a closed loop it gives zero. Moral: For nonzero Berry's phase, you need (i) more than one time-dependent parameter in the Hamiltonian, and (ii) a Hamiltonian that yields nontrivially complex eigenfunctions.

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).

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free