/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q9P A particle of mass m is in the s... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

A particle of mass m is in the state:

ψ(x,t)=Ae−a[(mx2/h)+it]

where A and a are positive real constants.

(a) Find A.

(b) For what potential energy function, V(x), is this a solution to the Schrödinger equation?

(c) Calculate the expectation values of x,x2 , p, andp2 .

(d) Find σx and σp. Is their product consistent with the uncertainty principle?

Short Answer

Expert verified

a. A=2amπh1/4

b.V(x,t)=2ma2x2

c. ⟨x⟩=0, ⟨x2⟩=h4am, ⟨p⟩=0,⟨p2⟩=ham

d. Yes, it’s consistent with the uncertainty principle

Step by step solution

01

Normalizing the wave equation (a)

Calculating for A by normalizing the wave function.

1=∫−∞∞|ψ(x,t)|2dx1=∫−∞∞ψ*(x,t)ψ(x,t)dx1=∫−∞∞(Ae−a[(mx2/h)+it])(Ae−a[(mx2/h)−it])dx1=A2∫−∞∞e−2amx2/hdx

Further solving above equation,

1=2A2∫0∞e−x2/[h/(2am)]2dx1=2A2.Ï€h/2am21=A2Ï€³ó2amA2=2amÏ€h1/2A=2amÏ€h1/4

Thus, the value of A is 2amπh1/4.

02

Finding the potential energy for which it is a solution of the Schrödinger equation (b)

Schrodinger equation is given by,

∂ψ∂t=ih2m∂2ψ∂x2−ihV(x,t)ψ(x,t)

Solving for V(x,t),

V(x,t)=hi1ψ(x,t)ih2m∂2ψ∂x2−∂ψ∂tV(x,t)=hi2amπh1/4ea[(mx2/h)+it]ih2m2amπh1/4∂2∂x2(e−a[(mx2/h)+it])−2amπh1/4(e−a[(mx2/h)+it])(−ia)V(x,t)=hea[(mx2/h)+it]ih2m∂2∂x2(e−a[(mx2/h)+it])−ae−a[(mx2/h)+it]V(x,t)=hea[(mx2/h)+it]ih2m−2amh1−2amhx2e−a[(mx2/h)+it]+ae−a[(mx2/h)+it]

Further solving above equation,

V(x,t)=ha2amhx2−1+aV(x,t)=2ma2x2

Thus, the potential energy function isV(x,t)=2ma2x2 .

03

Calculating the expectation values of x (c)

Solving for the expectation values.

⟨x⟩=∫−∞∞x|ψ(x,t)|2dx∫−∞∞|ψ(x,t)|2dx⟨x⟩=∫−∞∞³æÏˆ*(x,t)ψ(x,t)dx⟨x⟩=∫−∞∞x2amÏ€h1/4e−a[(mx2/h)+it]2amÏ€h1/4e−a[(mx2/h)−it]dx⟨x⟩=2amÏ€h∫−∞∞xe−2amx2/hdx

Since, integral of an odd function over a symmetric interval is zero.

Therefore, the expectation value is zero ⟨x⟩=0.

Now, for ⟨x2⟩

⟨x2⟩=∫−∞∞x2|ψ(x,t)|2dx∫−∞∞|ψ(x,t)|2dx⟨x2⟩=∫−∞∞x2ψ(x,t)ψ*(x,t)dx⟨x2⟩=∫−∞∞x22amπh1/4e−a[(mx2/h)+it]2amπh1/4e−a[(mx2/h)−it]dx⟨x2⟩=2amπh∫−∞∞x2e−2max2/hdx

⟨x2⟩=22amπh∫0∞x2e−x2/[h/(2am)]2dx⟨x2⟩=22amπh.π2!1h/2am23⟨x2⟩=h4am

Therefore, the value of ⟨x2⟩ is h4am.

04

Calculating the expectation values for p (c)

Using the Ehrenfest’s theorem,

⟨p⟩=m⟨v⟩⟨p⟩=md⟨x⟩dt

Since ⟨x⟩=0.

Therefore, the value of ⟨p⟩ is zero.

Now, solving for ⟨p2⟩.

⟨p2⟩=∫−∞∞ψ*(x,t)−ih∂∂x2ψ(x,t)dx⟨p2⟩=−h2∫−∞∞ψ*(x,t)∂2ψ∂x2dx⟨p2⟩=−h2∫−∞∞2amπh1/4e−a[(mx2/h)−it]∂2∂x22amπh1/4e−a[(mx2/h)+it]dx

Further solving above equation,

⟨p2⟩=−h22amπh2amh∫−∞∞1−2amhx2e−2amx2/hdx⟨p2⟩=−h22amπh2amh∫−∞∞e−2amx2/hdx−2amh∫−∞∞x2e−2amx2/hdx⟨p2⟩=−h22amπh4amh∫0∞e−x2/[h/2am]2dx−2amh∫0∞x2e−x2/[h/2am]2dx⟨p2⟩=−h22amπh4amhπh/2am2−2amhπ2!1!h/2am23

Further solving above equation,

⟨p2⟩=h24amh12−14⟨p2⟩=ham

Therefore, the value of ⟨p2⟩ is ham.

05

Checking the consistency with Heisenberg Uncertainty Principle

The standard variation of an observable gives the uncertainty, hence,

σx=Δ³æÎ”³æ=⟨x2⟩−⟨x⟩2Δ³æ=h4am−0Δ³æ=12ham

The calculation of standard deviation σp is,

σp=Δ±èΔ±è=⟨p2⟩−⟨p⟩2Δ±è=ham−0Δ±è=ham

The uncertainty can be written as,

Δ³æÎ”±è=12hamhamΔ³æÎ”±è=h2

And Heisenberg Uncertainty Principle states that

Δ³æÎ”±è≥h2

Therefore, it is consistent with the Heisenberg Uncertainty Principle.

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 91Ó°ÊÓ!

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

Why can’t you do integration-by-parts directly on the middle expression in Equation -1.29 pull the time derivative over onto x, note that∂x/∂t=0 , and conclude thatd<x>/dt=0 ?

We consider the same device as the previous problem, but this time we are interested in thex-coordinate of the needle point-that is, the "shadow," or "projection," of the needle on the horizontal line.

(a) What is the probability density ÒÏ(x)? Graph data-custom-editor="chemistry" ÒÏ(x) as a function of x, from -2rto +2r , where ris the length of the needle. Make sure the total probability is . Hint: data-custom-editor="chemistry" ÒÏ(x)dx is the probability that the projection lies between data-custom-editor="chemistry" xand data-custom-editor="chemistry" (x+dx). You know (from Problem 1.11) the probability that data-custom-editor="chemistry" θ is in a given range; the question is, what interval data-custom-editor="chemistry" dxcorresponds to the interval data-custom-editor="chemistry" »åθ?

(b) Compute data-custom-editor="chemistry" <x>, data-custom-editor="chemistry" <x2>, and data-custom-editor="chemistry" σ, for this distribution. Explain how you could have obtained these results from part (c) of Problem 1.11.

Consider the first 25 digits in the decimal expansion of π (3, 1, 4, 1, 5, 9, . . .).

(a) If you selected one number at random, from this set, what are the probabilities of getting each of the 10 digits?

(b) What is the most probable digit? What is the median digit? What is the average value?

(c) Find the standard deviation for this distribution.

The needle on a broken car speedometer is free to swing, and bounces perfectly off the pins at either end, so that if you give it a flick it is equally likely to come to rest at any angle between 0 tox.

  1. What is the probability density? Hint: ÒÏ(θ)dθ is the probability that the needle will come to rest betweenθ andθ+dθ .
  2. Compute⟨θ⟩ ,⟨θ2⟩ , andσ , for this distribution.
  3. Compute⟨sinθ⟩ ,⟨cosθ⟩ , and⟨cos2θ⟩

For the distribution of ages in the example in Section 1.3.1:

(a) Compute⟨j2⟩ and⟨j⟩2 .

(b) Determine ∆j for each j, and use Equation 1.11 to compute the standard deviation.

(c) Use your results in (a) and (b) to check Equation 1.12.

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.