Show that in the Iimit of large numbers, the exact probability of equation (9-9) becomes the Boltzmann probability of (9-17). Use the fact that K!(K-k)!Kk, which holds when k<<K.

Short Answer

Expert verified

The expression forP is NM+Ne-ln1+NM.

Step by step solution

01

A concept:

The Boltzmann distribution (also called the Gibbs distribution) is a probability distribution or probability measure that gives the probability that a system will be in a certain state as a function of the energy of that state and the temperature of the system.

The Boltzmann probability in terms of Enand kBT.

P(En)=e-EnkBTe-EnkBTn=0

02

Boltzmann Probability:

For a system of Nharmonic oscillators, the allowed energy ENfor one oscillator is given by:

En=nhω0

Expression into P:

role="math" localid="1660135304939" PEn=e-nhω0kBTe-nhω0kBTn=0=e-nhω0kBTe-nhω0kBTnn=0

03

Denominator of P:

Use the following expression to solve further.

xnn=0=11-x

Applying denominator of P:

PEn=e-nhω0kBT11-e-nhω0kBT=1-e-nhω0kBTe-nhω0kBT

04

The is expressed in terms of N and M:

Use the following expression to solve further.

kBT=hω0ln1+NMhω0kBT=ln1+NM

Therefore,

role="math" localid="1660136050103" PEn=1-e-ln1+NMe-nln1+NM=1-1eln1+NMe-ln1+NM=1-11+NMe-ln1+NM=1+NM-11+NMe-ln1+NM

PEn=NMNMMe-ln1+NM=NM+Ne-ln1+NM

The expression for Pis NM+Ne-ln1+NM.

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Most popular questions from this chapter

Somehow you have a two-dimensional solid, a sheet of atoms in a square lattice, each atom linked to its four closest neighbors by four springs oriented along the two perpendicular axes. (a) What would you expect the molar heat capacity to be at very low temperatures and at very high temperatures? (b) What quantity would determine, roughly, the line between low and high?

Using the relationship between temperature and MandN given in (9-16) and that betweenE andn in (9-6), obtain equation (9-17) from (9- 12). The first sum given In Exercise 30 will be useful.

Example 9.2 obtains a ratio of the number of particles expected in the n = 2state lo that in the ground state. Rather than the n = 2state, consider arbitrary n.

(a) Show that the ratio is numberofenergyEnnumberofenergyE1=n2e-13.6cV(1-n-2)/kBT

Note that hydrogen atom energies are En=-13.6eV/st2.

(b) What is the limit of this ratio as n becomes very large? Can it exceed 1? If so, under what condition(s)?

(c) In Example 9.2. we found that even at the temperature of the Sun's surface(~6000K), the ratio for n = 2 is only 10-8 . For what value of nwould the ratio be 0.01?

(d) Is it realistic that the number of atoms with high n could be greater than the number with low n ?

There are more permutations of particle labels when two particles have energy0 and two have energy1 than when three particles have energy 0and one has energy . 2(The total energiesarethe same.) From this observation alone argue that the Boltzmann distribution should be lower than the Bose-Einstein at the lower energy level.

Exercise 52 gives the Boltzmann distribution for the special case of simple harmonic oscillators, expressed in terms of the constantε, Nω0/(2s+1)and Exercise 53 gives the two quantum distributions in that case. Show that both quantum distributions converge to the Boltzmann in the limitkBT.

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