Consider a classical "degree of freedom" that is linear rather than quadratic E=cqfor some constant c. (As example would be the kinetic energy of a highly relativistic particle in one dimension, written in terms of its momentum.) Repeat derivation of the equipartition theorem for this system, and show that the average energy isrole="math" localid="1646903677918" E-=kT.

Short Answer

Expert verified

The average energy is given byE-=kT.

Step by step solution

01

Step 1. Given information

The classical degree of freedom is described byE=cq, wherecis a constant.

02

Step 2. Calculation of Partition function

The formula to calculate the partition function is given by

Z=qe-βEq..................(1)

Here, Zis the partition function and β=1kTis the Boltzmann factor, kbeing Boltzmann constant and Tbeing the absolute temperature.

Substitute cqfor Einto equation (1) and change the summation by integral sign to obtain the partition function.

Z=1q-e-βcqdq.................(2)

03

Step3. Evaluation of partition function

Simplify equation (2) in step 2 to obtain an expression for the partition function.

Z=1q-0eβcqdq+0e-βcqdq=1q1βceβcq-0-1βce-βcq0=2qβc..................(3)

04

Step4. Evaluation of the average energy

The formula to calculate the average energy is given by

E-=-1ZZβ.................(4)

Here, E-is the average energy.

Substitute the value of Zfrom equation (3) into equation (4) and simplify to obtain the required average energy.

role="math" localid="1646905279668" E-=-12qβcβ2qβc=-ββ1β=1β=kT

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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.

Prove that the probability of finding an atom in any particular energy level is P(E)=(1/Z)e-F/kT, whereF=E-TS and the "'entropy" of a level is k times the logarithm of the number of degenerate states for that level.

Consider a classical particle moving in a one-dimensional potential well ux, as shown. The particle is in thermal equilibrium with a reservoir at temperature T, so the probabilities of its various states are determined by Boltzmann statistics.

{a) Show that the average position of the particle is given by

x=xe-βuxdxe-βuxdx

where each integral is over the entire xaxis.

A one-dimensional potential well. The higher the temperature, the farther the particle will stray from the equilibrium point.

(b) If the temperature is reasonably low (but still high enough for classical mechanics to apply), the particle will spend most of its time near the bottom of the potential well. In that case we can expand u(z) in a Taylor series about the equilibrium point

ux=ux0+x-x0dudxx0+12x-x02d2udx2x0+13!x-x03d3udx3x0+........

Show that the linear term must be zero, and that truncating the series after the quadratic term results in the trivial prediction x=x0.

(c) If we keep the cubic term in the Taylor series as well, the integrals in the formula for xbecome difficult. To simplify them, assume that the cubic term is small, so its exponential can be expanded in a Taylor series (leaving the quadratic term in the exponent). Keeping only the smallest temperature-dependent term, show that in this limit x differs from by a term proportional to kT. Express the coefficient of this term in terms of the coefficients of the Taylor series ux

(d) The interaction of noble gas atoms can be modeled using the Lennard Jones potential,

ux=u0x0x12-2x0x6

Sketch this function, and show that the minimum of the potential well is at x=x0, with depth u0. For argon, x0=3.9Aand u0=0.010eV. Expand the Lennard-Jones potential in a Taylor series about the equilibrium point, and use the result of part ( c) to predict the linear thermal expansion coefficient of a noble gas crystal in terms of u0. Evaluate the result numerically for argon, and compare to the measured value α=0.0007K-1

For a diatomic gas near room temperature, the internal partition function is simply the rotational partition function computed in section 6.2, multiplied by the degeneracy Zeof the electronic ground state.

(a) Show that the entropy in this case is

S=NkInVZeZrotNvQ+72.

Calculate the entropy of a mole of oxygen at room temperature and atmospheric pressure, and compare to the measured value in the table at the back of this book.

(b) Calculate the chemical potential of oxygen in earth's atmosphere near sea level, at room temperature. Express the answer in electron-volts

Show explicitly from the results of this section thatG=Nμfor an ideal gas.

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