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Imagine a particle that can be in only three states, with energies -0.05 eV, 0, and 0.05 eV. This particle is in equilibrium with a reservoir at 300 K.

(a) Calculate the partition function for this particle.

(b) Calculate the probability for this particle to be in each of the three states.

(c) Because the zero point for measuring energies is arbitrary, we could just as well say that the energies of the three states are 0, +0.05 eV, and +0.10 eV, respectively. Repeat parts (a) and (b) using these numbers. Explain what changes and what doesn't.

Short Answer

Expert verified

Therefore,

(a) the partition function is Z=8.063

(b) the probability for this particle is P1=0.858P2=0.124P3=0.018

(c)Z=1.165P1=0.858P2=0.124P3=0.018

Step by step solution

01

Given information

A particle that can be in only three states, with energies -0.05 eV, 0, and 0.05 eV. This particle is in equilibrium with a reservoir at 300 K.

02

Explanation

(a) The partition function is equal to the total of all Boltzmann factors, i.e.

Z=∑se-E(s)/kT

Consider a particle that can exist in three states, each with an energy of ϵ1=-0.05 eV, ϵ2= 0 eV, and ϵ3= 0.05 eV; the partition function is:

Z=e-ϵ1/kT+e-ϵ2/kT+e-ϵ3/kT

Substitute the energies and Boltzmann's constant

Z=e0.05eV/0.025851eV+e0+e-0.05eV/0.025851eVZ=8.063

(b)The probability is given by:

P=1Ze-E(s)/kT

For first state,

P1=1Ze-ϵ1/kT=18.063e0.05eV/0.025851eVP1=0.858

For second state,

P2=1Ze-ϵ2/kT=18.063P2=0.124

For third state,

P3=1Ze-ϵ3/kT=18.063e-0.05eV/0.025851eVP3=0.018

03

Explanation

(c) Now imagine a particle that can exist in three states with energies of ϵ1= 0 eV, ϵ2= 0.05 eV, and ϵ3= 0.10 eV; the partition function is:Z=e-ϵ1/kT+e-ϵ2/kT+e-ϵ3/kT

Substitute with energies and Boltzmann's constant:

role="math" localid="1647298423935" Z=e0+e-0.05eV/0.025851eV+e-0.10eV/0.025851eVZ=1.165

For first state

P1=1Ze-ϵ1/kT=11.165P1=0.858

For second state:

P2=1Ze-ϵ2/kT=11.165e-0.05eV/0.025851eVP2=0.124

For third state

P3=1Ze-ϵ3/kT=11.165e-0.10eV/0.025851eVP3=0.018

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Most popular questions from this chapter

Apply the result of Problem 6.18 to obtain a formula for the standard deviation of the energy of a system of N identical harmonic oscillators (such as in an Einstein solid), in the high-temperature limit. Divide by the average energy to obtain a measure of the fractional fluctuation in energy. Evaluate this fraction numerically for N = 1, 104, and 1020. Discuss the results briefly.

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11-x=1+x+x2+x3+⋯

For what values of x does this series have a finite sum?

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(c) Use formula 6.25 to find an expression for the average energy of a single oscillator at temperature T. Simplify your answer as much as possible.

(d) What is the total energy of the system of N oscillators at temperature T? Your result should agree with what you found in Problem 3.25.

(e) If you haven't already done so in Problem 3.25, compute the heat capacity of this system and check t hat it has the expected limits as T→0 and T→∞.

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