Prove the famous "(your name) uncertainty principle," relating the uncertainty in positionA=x to the uncertainty in energyB=p2/2m+v:

σxσHh2m|p|

For stationary states this doesn't tell you much-why not?

Short Answer

Expert verified

The uncertainty principle isσxσHh2mp

Step by step solution

01

Concept used

The generalized uncertainty principle for two observables A and B is given by:

σA2σB212iA^,B^2

02

Calculate the uncertainty principle

The generalized uncertainty principle for two observables A and B is given by:

σA2σB212iA^,B^2

The position-energy uncertainty relation is:

σx2σH212ix^,H^2 ....(1)

So, we need to find the commutatorx^,H^as:

X^,H^g=-h22m×2gX2+xVg+-h22m2x2xg-xVg=h22m-x2gX2+2gx+x2gX2=h2mgx=ihmpg

Substitute in equation 1:

σx2σH212ix^,H^]2=h24m2p2

So, the uncertainty principle here becomes

σxσHh2mp

For stationary states, this doesn't tell you much because the average position of the particle doesn't change, σH=0andp=0.

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

Prove the famous "(your name) uncertainty principle," relating the uncertainty in position (A=x)to the uncertainty in energy(B=p2/2m+V): σxσH2m|p|

For stationary states this doesn't tell you much-why not?

(a) For what range of vis the function f(x)=x''in Hilbert space, on the interval (0.1)? Assume vis real, but not necessarily positive.

(b) For the specific case v=1/2, is f(x)in this Hilbert space? What aboutxf(x)? How about (d/dx)f(x)?

(a) For a function f(x)that can be expanded in a Taylor series, show that f(x+x0)=eip^x0Ihf(x)

wherex_{0}

is any constant distance). For this reason, p^/his called the generator of translations in space. Note: The exponential of an operator is defined by the power series expansion: eQ^1+Q^+(1/2)Q^2+(1/3!)Q^3+...

(b) If ψ(x,t)satisfies the (time-dependent) Schrödinger equation, show that ψ(x,t+t0)=e-iH^t0/hψ(x,t)

where t_{0}is any constant time); -H^/his called the generator of translations in time.

(c) Show that the expectation value of a dynamical variableQ(x,p,t), at time , t+t0can be written34

<Q>t+t0=<ψx,t|eiH^t0/hQ^x^,p^,t+t0e-iH^t0/h|ψx,t>

Use this to recover Equation 3.71. Hint: Lett0=dt, and expand to first order in dt.

Test the energy-time uncertainty principle for the wave function in Problem2.5and the observable x, by calculatingσHσXandd<x>/dtexactly.

(a) Write down the time-dependent "Schrödinger equation" in momentum space, for a free particle, and solve it. Answer: exp(-ip2t/2mh)Φ(p,0).

(b) Find role="math" localid="1656051039815" Φ(p,0)for the traveling gaussian wave packet (Problem 2.43), and construct Φ(p,t)for this case. Also construct |Φ(p,t)|2, and note that it is independent of time.

(c) Calculaterole="math" localid="1656051188971" pandrole="math" localid="1656051181044" p2by evaluating the appropriate integrals involvingΦ, and compare your answers to Problem 2.43.

(d) Show thatrole="math" localid="1656051421703" <H>=<p>2/2m+<H>0(where the subscript denotes the stationary gaussian), and comment on this result.

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