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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=1N∑iΔEi2(1)

The deviation is:

ΔEi=Ei-E¯

Substitute into (1)

σE2=1N∑iEi-E¯2σE2=1N∑Ei2+E¯2-2EiE¯σE2=1N∑iEi2+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

For a CO molecule, the constant ϵis approximately 0.00024eV. (This number is measured using microwave spectroscopy, that is, by measuring the microwave frequencies needed to excite the molecules into higher rotational states.) Calculate the rotational partition function for a COmolecule at room temperature (300K), first using the exact formula 6.30 and then using the approximate formula 6.31.

Although an ordinary H2 molecule consists of two identical atoms, this is not the case for the molecule HD, with one atom of deuterium (i.e., heavy hydrogen, 2H). Because of its small moment of inertia, the HD molecule has a relatively large value of ϵ:0.0057eV At approximately what temperature would you expect the rotational heat capacity of a gas of HD molecules to "freeze out," that is, to fall significantly below the constant value predicted by the equipartition theorem?

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.

A particle near earth's surface traveling faster than about 11km/shas enough kinetic energy to completely escape from the earth, despite earth's gravitational pull. Molecules in the upper atmosphere that are moving faster than this will therefore escape if they do not suffer any collisions on the way out.

(a) The temperature of earth's upper atmosphere is actually quite high, around 1000K.Calculate the probability of a nitrogen molecule at this temperature moving faster than 11km/s, and comment on the result.

(b) Repeat the calculation for a hydrogen molecule (H2)and for a helium atom, and discuss the implications.

(c) Escape speed from the moon's surface is only about 2.4km/s. Explain why the moon has no atmosphere.

Carefully plot the Maxwell speed distribution for nitrogen molecules at T=300K and atT=600K. Plot both graphs on the same axes, and label the axes with numbers.

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