In a real semiconductor, the density of states at the bottom of the conduction band will differ from the model used in the previous problem by a numerical factor, which can be small or large depending on the material. Let us, therefore, write for the conduction band g(ϵ)=g0cϵ-ϵcwhere g0cis a new normalization constant that differs from g0by some fudge factor. Similarly, write gat the top of the valence band in terms of a new normalization constant g0v.

(a) Explain why, if g0vg0c, the chemical potential will now vary with temperature. When will it increase, and when will it decrease?

(b) Write down an expression for the number of conduction electrons, in terms of T,μ,candg0cSimplify this expression as much as possible, assuming ϵc-μkT.

(c) An empty state in the valence band is called a hole. In analogy to part (b), write down an expression for the number of holes, and simplify it in the limit μ-ϵvkT.

(d) Combine the results of parts (b) and (c) to find an expression for the chemical potential as a function of temperature.

(e) For silicon, g0cg0=1.09andg0vg0=0.44*.Calculate the shift inµ for silicon at room temperature.

Short Answer

Expert verified

(a) The chemical potential will varyNC=g0cϵCϵ-ϵCeϵ-ϵF/kT+1dϵ

(b) The number of conduction electronsNCg0cπ2(kT)3/2e-ϵC-μ/kT

(c) The valence bond isNv=g0vπ2e-μ-ϵv/kT(kT)3/2

(d) The chemical potential isμ=ϵC+ϵv2-kT2lng0cg0v

(e) The shift for silicon isμshift=-0.0118eV

Step by step solution

01

Part(a) Step 1: Given information

We have been given that g(ϵ)=g0cϵ-ϵC

02

Part(a) Step 2: Given information

The solution is as follows:

NC=ϵCg(ϵ)n¯FDdϵ

NC=g0cϵCϵ-ϵCeϵ-ϵF/kT+1dϵ

03

Part(b) Step 1: Given information

We have been given thatπ2

04

Part(b) Step 2: Simplify

The numbers of electrons in the conduction

0xe-xdx=π2

NCg0cπ2(kT)3/2e-ϵC-μ/kT

05

Part(c) Step 1: GIven information

We have been given that NCV

06

Part(c) Step 2: Simplify

The solution is as follows:

n¯FD=1e(ϵ-μ)/kT+1g(ϵ)=g0vϵv-ϵ

Nv=g0vπ2e-μ-ϵv/kT(kT)3/2

07

Part (d) Step 1: Given information

We have been givenNT3/2e-c/T

08

Part(d) Step 2:Simplify

The temperature increases

vQ=6.626×10-34J·s22π9.11×10-31kg1.38×10-23J/K(350K)3/2

=6.328×10-26m3

09

Given information

We have been given thatNCV

10

Simplify

The steps are given below

NCV=2m-3=28.00×10-26m3e-Δϵ/(0.052eV)

Δϵ=3.0eV

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

In the text I claimed that the universe was filled with ionised gas until its temperature cooled to about 3000 K. To see why, assume that the universe contains only photons and hydrogen atoms, with a constant ratio of 109 photons per hydrogen atom. Calculate and plot the fraction of atoms that were ionised as a function of temperature, for temperatures between 0 and 6000 K. How does the result change if the ratio of photons to atoms is 108 or 1010? (Hint: Write everything in terms of dimensionless variables such as t = kT/I, where I is the ionisation energy of hydrogen.)

In analogy with the previous problem, consider a system of identical spin0bosonstrapped in a region where the energy levels are evenly spaced. Assume that Nis a large number, and again let qbe the number of energy units.

(a) Draw diagrams representing all allowed system states from q=0up to q=6.Instead of using dots as in the previous problem, use numbers to indicate the number of bosons occupying each level.

(b) Compute the occupancy of each energy level, for q=6. Draw a graph of the occupancy as a function of the energy at each level.

(c) Estimate values of μand Tthat you would have to plug into the Bose-Einstein distribution to best fit the graph of part(b).

(d) As in part (d) of the previous problem, draw a graph of entropy vs energy and estimate the temperature at q=6from this graph.

Suppose you have a "box" in which each particle may occupy any of 10single-particle states. For simplicity, assume that each of these states has energy zero.

(a) What is the partition function of this system if the box contains only one particle?

(b) What is the partition function of this system if the box contains two distinguishable particles?

(c) What is the partition function if the box contains two identical bosons?

(d) What is the partition function if the box contains two identical fermions?

(e) What would be the partition function of this system according to equation 7.16?

(f) What is the probability of finding both particles in the same single particle state, for the three cases of distinguishable particles, identical bosom, and identical fermions?

In Section 6.5 I derived the useful relation F=-kTln(Z)between the Helmholtz free energy and the ordinary partition function. Use analogous argument to prove that ϕ=-kT×ln(Z^), where Z^ is the grand partition function and ϕis the grand free energy introduced in Problem 5.23.

Consider a collection of 10,000 atoms of rubidium- 87 , confined inside a box of volume (10-5m)3.

(a) Calculate ε0, the energy of the ground state. (Express your answer in both joules and electron-volts.)

(b) Calculate the condensation temperature, and compare kTctoε0.

(c) Suppose that T=0.9TcHow many atoms are in the ground state? How close is the chemical potential to the ground-state energy? How many atoms are in each of the (threefold-degenerate) first excited states?

(d) Repeat parts (b) and (c) for the case of 106atoms, confined to the same volume. Discuss the conditions under which the number of atoms in the ground state will be much greater than the number in the first excited state.

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