The most common measure of the fluctuations of a set of numbers away from the average is the standard deviation, defined as follows.

(a) For each atom in the five-atom toy model of Figure 6.5, compute the deviation of the energy from the average energy, that is, Ei-E¯,fori=1to5. Call these deviations ΔEi.

(b) Compute the average of the squares of the five deviations, that is, ΔEi2¯. Then compute the square root of this quantity, which is the root-mean- square (rms) deviation, or standard deviation. Call this number σE. Does σEgive a reasonable measure of how far the individual values tend to stray from the average?

(c) Prove in general that

σE2=E2¯-(E¯)2

that is, the standard deviation squared is the average of the squares minus the square of the average. This formula usually gives the easier way of computing a standard deviation.

(d) Check the preceding formula for the five-atom toy model of Figure 6.5.

Short Answer

Expert verified

Therefore,

Deviation of energy is E1-E¯=-3eVE2-E¯=1eVE3-E¯=4eV

Average of the squares of five deviations is σE=2.683

Step by step solution

01

Given information

The most common measure of the fluctuations of a set of numbers away from the average is the standard deviation.

02

Explanation

(a) Consider the following toy energy model: there are two particles with E1 = 0 eV, two particles with E2 = 4 eV, and one particle with E3 = 7 eV, and their average energy is provided by:

E¯=2(0eV)+2(4eV)+1(7eV)5

Where 5 is the total number of particles, so:

E¯=3eV

The deviation is given by Ei-E¯, so:

E1-E¯=-3eVE2-E¯=1eVE3-E¯=4eV

We have two particles with the first deviation and two particles with the second deviation.

03

Explanation

(b)The square of these deviations is

9eV29eV21eV21eV216eV2

Average of these are:

σE2=9eV2+9eV2+1eV2+1eV2+16eV25=7.2eV2

The standard deviation is the square root of this value:

σE=7.2eV2=2.683eVσE=2.683eV

(c) Standard deviation is:

σE2=ΔEi2¯

The average equals the sum over the number of the values, so:

σE2=1NiΔEi2(1)

The deviation is:

ΔEi=Ei-E¯

Substitute into (1)

σE2=1NiEi-E¯2σE2=1NEi2+E¯2-2EiE¯σE2=1NiEi2+E¯2-2E¯iEiσE2=E2¯+E¯2-2E¯2σE2=E2¯-E¯2

04

Explanation

(d) We have 5 particles with energies of 0 eV, 0 eV, 4 eV, 4 eV, and 7 eV; their squares are 0 eV2, 0 eV2, 16 eV2, 16 eV,2 and 49 eV2; the average of these values is:

E2¯=(0+0+16+16+49)eV25=16.2eV2

The average of the energies is:

E¯=(0+0+4+4+7)eV5=3eV

The standard deviation is:

σE=16.2eV2-(3eV)2

σE=2.683eV

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Most popular questions from this chapter

This problem concerns a collection of N identical harmonic oscillators (perhaps an Einstein solid or the internal vibrations of gas molecules) at temperature T. As in Section 2.2, the allowed energies of each oscillator are 0, hf, 2hf, and so on. (

a) Prove by long division that

11-x=1+x+x2+x3+

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

(b) Evaluate the partition function for a single harmonic oscillator. Use the result of part (a) to simplify your answer as much as possible.

(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 T0 and T.

In the low-temperature limit (kT<<), each term in the rotational partition function is much smaller than the one before. Since the first term is independent of T, cut off the sum after the second term and compute the average energy and the heat capacity in this approximation. Keep only the largest T-dependent term at each stage of the calculation. Is your result consistent with the third law of thermodynamics? Sketch the behavior of the heat capacity at all temperature, interpolating between the high-temperature and low- temperature expressions.

Estimate the probability that a hydrogen atom at room temperature is in one of its first excited states (relative to the probability of being in the ground state). Don't forget to take degeneracy into account. Then repeat the calculation for a hydrogen atom in the atmosphere of the starγ UMa, whose surface temperature is approximately 9500 K.

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 mole nitrogen (N2)gas at room temperature and atmospheric pressure, compute the following U,H,F,G,Sand μ. (The electronic ground state of nitrogen is not degenerate.)

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