For a particle in a one-dimensional (ID) box, Enis proportional to a single quantum number n. Let us simplify things by ignoring the proportionality factor: En=n2 . For a 3D box, Enx,ny,nz=nx2+ny2+nz2, and the 2D box is fairly obvious.

(a) The table shows a start on accounting for allowed states. Complete the table, stopping after the 10th state (state, not energy) for all three cases.

(b) Find the number of states per energy difference for the first five states and the last five states for all three cases. For instance, for the first five in the ID case, it is 5 states per energy difference of 24, or5/24 .

(c) Overlooking the obviously crude aspects of this accounting, does the "density of states" seem to increase with energy, decrease with energy, or stay about the same?

Short Answer

Expert verified

(a). Complete table is given in the solution

(b). The number of states for first five and last five in1Dare524and564respectively, in 2D are58and57respectively and in 3D are56and52respectively.

c). The density of the states tends to decrease with the energy.

Step by step solution

01

Formula used 

The expression of number of states is given by,

N=nE2E1

02

Complete the table 

a)

Given information is

The En is proportional to single quantum number n.

To complete the table up to 10th state, n should varies such that it gives the lowest amount of energy. The complete table is

role="math" localid="1660026759024" 1D
2D
3D

States (n)

Energy (n2)

States (nx,ny)

Energy (nx2+ny2)

States

(nx,ny,nz)

Energy

(nx2+ny2+nz2)

1
1
1,1
2
1,1,1
3

2

4

1,2

5

1,1,2

6

3

9

2,1

5

1,2,1

6

4

16

2,2

8

2,1,1

6

5

25

1,3

10

1,2,2

9

6

36

3,1

10

2,1,2

role="math" localid="1660028505713" 9

7

49

2,3

13

2,2,1

9

8

64

3,2

13

1,1,3

11

9

81

1,4

17

1,3,1

11

10

100

4,1

17

3,1,1

11

03

Calculate the number of states per energy difference.

(b)

The expression of number of states is given by,

N=nE2E1

The number of states for first five in 1D is calculated as,

N=nE2E1N(firstfive)=5251=524

The number of states for last five in 1Dis calculated as,

N=nE2E1N(lastfive)=510036=564

The number of states for first five in 2Dis calculated as,

N=nE2E1

N(firstfive)=5102=58

The number of states for last five in 2Dis calculated as,

N=nE2E1N(lastfive)=51710=57

The number of states for first five in 3Dis calculated as,

N=nE2E1N(firstfive)=593=56

The number of states for last five in 3Dis calculated as,

N=nE2E1N(lastfive)=5119=52

Therefore, the number of states for first five and last five in 1D are 524 and 564 respectively, in 2D are 58 and 57 respectively and in 3D are 56 and 52 respectively.

04

The change in density of states with the energy

c)

From part (b), the density of the states tends to increase with the dimensionality but decrease with the energy.

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

Given an arbitrary thermodynamic system, which is larger. the number of possible macro-states. or the numberof possible microstates, or is it impossible to say? Explain your answer. (For most systems, both are infinite, but il is still possible to answer the question,)

A particle subject to a planet's gravitational pull has a total mechanical energy given by Emechanical=12mv2-GMmr, whereis the particle's mass.M the planet's mass, and Gthe gravitational constant6.67×10-11N·m3/kg2. It may escape if its energy is zero that is, if its positive KE is equal in magnitude to the negative PE holding if to the surface. Suppose the particle is a gas molecule in an atmosphere.

(a) Temperatures in Earth's atmosphere may reach 1000K. Referring to the values obtained in Exercise 45 and given that REarth=6.37×106mand MEarth=5.98×1024kg. should Earth be able to "hold on" to hydrogen (1g/mol)? 10 nitrogens (28g/mol)? (Note: An upper limit on the number of molecules in Earth's atmosphere is about 10-18).

(b) The moon's mass is 0.0123times Earth's. its radius 0.26 times Earth's, and its surface temperatures rise to 370K. Should it be able to hold on to these gases?

The Fermi energy in a quantum gas depends inversely on the volume, Basing your answer on Simple Chapter 5 type quantum mechanics (not such quaint notions as squeezing classical particles of finite volume into a container too small). Explain why.

The temperature of our Sun’s surface is ~6000K.(a) At what wavelength is the spectral emission of the Sun is maximum? (Refer to Exercise 79.) (b) Is there something conspicuous about this wavelength?

The fact that a laser's resonant cavity so effectively sharpens the wavelength can lead to the output of several closely spaced laser wavelengths, called longitudinal modes. Here we see how. Suppose the spontaneous emission serving as the seed for stimulated emission is of wavelength , but somewhat fuzzy, with a line width of roughly0.001nm either side of the central value. The resonant cavity is exactly60cm long. (a) How many wavelengths fit the standing-wave condition'? (b) If only u single wavelength were desired, would change the length of the cavity help? Explain.

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