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The previous two problems dealt with pure semiconductors, also called intrinsic semiconductors. Useful semiconductor devices are instead made from doped semiconductors, which contain substantial numbers of impurity atoms. One example of a doped semiconductor was treated in Problem 7.5. Let us now consider that system again. (Note that in Problem 7.5 we measured all energies relative to the bottom of the conduction band, Ee. We also neglected the distinction between g0and g0c; this simplification happens to be ok for conduction electrons in silicon.)

(a) Calculate and plot the chemical potential as afunction of temperature, for silicon doped with 1017phosphorus atoms per cm3(as in Problem 7.5). Continue to assume that the conduction electrons can be treated as an ordinary ideal gas.

(b) Discuss whether it is legitimate to assume for this system that the conduction electrons can be treated asan ordinary ideal gas, as opposed to a Fermi gas. Give some numerical examples.

(c)Estimate the temperature at which the number of valence electrons excitedto the conduction band would become comparable to the number ofconduction electrons from donor impurities. Which source of conductionelectrons is more important at room temperature?

Short Answer

Expert verified

(a). The chemical potential as a function of temperature is:ฮผI=-tln2t3/20.0036xwherex=1-2eI/kTvQNd2V

And the plot of chemical potential as a function of temperature is

(b). Since, ฯต-ฮผkTโ‰ˆ3IkT=3ร—1.695โ‰ˆ5. The approximate Boltzmann distribution should be accurate.

(c). The temperature at which the number of valence electrons excitedto the conduction band would become comparable is T=520K.

Step by step solution

01

Part(a): Step 1: Given information:

We have been given silicon doped with phosphorus atoms.

02

Part(a): Step 2: Explanation

Chemical potential is given byฮผ=-kTlnVZintNcvQ

Due to two spin states ฮผ=-kTln2VNcvQ

Ratio of Conduction electrons to number of doner atoms is NcNd=x=1-2eI/kTvQNd2V

where ฮผ=-kTln2VxNdvQand x=1-2eI/kTvQNd2V

Let t=kTI

Therefore Quantum volume vQ=h22ฯ€mI3/21t3/2

Putting the vlaues of universal constants m,handI.vQ=6.626ร—10-34Jยทs22ฯ€9.11ร—10-31kg0.044ร—1.6ร—10-19J3/21t3/2=3.6ร—10-26t-3/2

Also it is known NdV=1ร—1023m3

EvalutingฮผI=-tln2x1ร—1023m33.6ร—10-26t-3/2

ThereforeฮผI=-tln2t3/20.0036xandx=1-(0.0036)e1/tt3/2.

03

Part(a): Step 3: Graph

Plotting a graph between ฮผI

04

Part(b): Step 1: Given information

We have to find whether the conduction elements can be treated as an ordinary ideal gas.

05

Part(b): Step 2: Explanation

Considering the denominator of Fermi Dirac that is much greater than 1 we treat it as gas.

Therefore energies of the conduction band ฯต-ฮผโ‰ซkT

The difference between edge energy of conduction band is 3, therefore localid="1650464758608" ฯต-ฮผโ‰ˆ3I.

Solving IkT=0.044eV0.026eV=1.695

ฯต-ฮผkTโ‰ˆ3IkT=3ร—1.695โ‰ˆ5

Therefore the value of exponential e5โ‰ˆ150which is much greater than 1.

Therefore approximating the Fermi Dirac distribution by Boltzmann distribution should be accurate.

06

Part(c): Step 1: Given Information

We have to find out the temperature for which number of valence electrons excited to the conduction band would become comparable to the number of conduction electrons from donor impurities.

07

Part(c): Step 2: Explanation

Saturation point of number of conduction electrons1017Patoms percm3

i.eNdV=1ร—1023m3

For temperature NCV=2vQe-ฮ”ฯต/2kT

Let this expression be equal to 1023; Solving-ฮ”ฯต2kT=lnvQNC2V

1T=-2kฮ”ฯตlnvQNC2V

Substituting 1T=-28.62ร—10-5eV1.11eVlnvQNC2V

Quantum volume is given by vQ=6.626ร—10-34Jยทs22ฯ€9.11ร—10-31kg1.38ร—10-23J/K3/21T3/2

=3.6ร—10-20T-3/2

Therefore

1T=-1.553ร—10-4ln(0.0018)T-3/2

08

Part(c): Step 3: Graph

Intersection in graph occurs at T=520K

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Most popular questions from this chapter

It's not obvious from Figure 7.19 how the Planck spectrum changes as a function of temperature. To examine the temperature dependence, make a quantitative plot of the functionu(ฯต) for T = 3000 K and T = 6000 K (both on the same graph). Label the horizontal axis in electron-volts.

Evaluate the integral in equation N=2ฯ€2ฯ€mh23/2Vโˆซ0โˆžฯตdฯตeฯต/kT-1numerically, to confirm the value quoted in the text.

At the center of the sun, the temperature is approximately 107K and the concentration of electrons is approximately 1032 per cubic meter. Would it be (approximately) valid to treat these electrons as a "classical" ideal gas (using Boltzmann statistics), or as a degenerate Fermi gas (with Tโ‰ˆ0 ), or neither?

Although the integrals (7.53and 7.54) forNand Ucannot be

carried out analytically for all T, it's not difficult to evaluate them numerically

using a computer. This calculation has little relevance for electrons in metals (for

which the limit kT<<EFis always sufficient), but it is needed for liquid H3eand

for astrophysical systems like the electrons at the center of the sun.

(a) As a warm-up exercise, evaluate theNintegral (7.53) for the casekT=ฮตF

and ฮผ=0, and check that your answer is consistent with the graph shown

above. (Hint: As always when solving a problem on a computer, it's best to

first put everything in terms of dimensionless variables. So let t=kTฮตFrole="math" localid="1649996205331" ,c=ฮผฮตF

, and x=ฮตkT. Rewrite everything in terms of these variables,

and then put it on the computer.)

(b) The next step is to varyฮผ holdingT fixed, until the integral works out to

the desired value,N. Do this for values of kTฮตFranging from 0.1 up to 2,

and plot the results to reproduce Figure7.16. (It's probably not a good idea

to try to use numerical methods when kTฮตF is much smaller than 0.1, since

you can start getting overflow errors from exponentiating large numbers.

But this is the region where we've already solved the problem analytically.)

(c) Plug your calculated values ofยต into the energy integral (7.54), and evaluate

that integral numerically to obtain the energy as a function of temperature

forkTup to 2ฮตF Plot the results, and evaluate the slope to obtain the

heat capacity. Check that the heat capacity has the expected behavior at

both low and high temperatures.

An atomic nucleus can be crudely modeled as a gas of nucleons with a number density of 0.18fm-3(where 1fm=10-15m). Because nucleons come in two different types (protons and neutrons), each with spin 1/2, each spatial wavefunction can hold four nucleons. Calculate the Fermi energy of this system, in MeV. Also calculate the Fermi temperature, and comment on the result.

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