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Show that during the quasistatic isothermal expansion of a monatomic ideal gas, the change in entropy is related to the heat input Qby the simple formula

s=QT

In the following chapter I'll prove that this formula is valid for any quasistatic process. Show, however, that it is not valid for the free expansion process described above.

Short Answer

Expert verified

The Formula of monatomic ideal gas of during quasistatic isothermal expansion is proved as change in entropy,s=QTand the reason is valid where expanding gas is work,so the heat input provide energy for work.

Step by step solution

01

Step: 1 Sackur-Tetrode equation:

The entropy substance as

S=kln()

where is the number of microstates accessible substance.

For 3-dideal gas, the formula by

S=NklnVN4mU3Nh232+52

02

Step; 2 Equating amount of energy:

Where,Vrepresents volume, Urepresents energy, Nrepresents the number of molecules, mrepresents the mass of a single molecule, and hrepresents Planck's constant. Despite the fact that this formula appears to be a little difficult, we can see that raising either of V,U, or Nincreases entropy. The gas expands quasistatically in an isothermal expansion, keeping its temperature constant. This indicates that U=3/2NkTremains constant as well, leaving just the volume to vary. Because the gas is doing work Wby expanding, the energy for the work must come from a source of heat Qintroduced into the gas to keep the temperature constant. The first law of thermodynamics states:

Q=U+W

But U=0and W=ViVfPdVwe get

Q=ViVfPdV

From ideal-gas law,

role="math" localid="1650264837406" P=NkTV,ViVfdVVdVQ=NkTNkT[ln(V)]ViVfQ=NkTlnVfVi

03

Step: 3 Change in entropy:

Substituting the constant Uand Nwe get

S=NklnVN4mU3Nh232+52S=Nkln(V)+ln1N4mU3Nh232+52ln1N4mU3Nh232

The change in entropy process where volume only changes by

S=SfSi=NklnVflnViS=NklnVfViS=QT

The reason is valid where expanding gas is work,so the heat input provide energy for work.

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Most popular questions from this chapter

Suppose you flip four fair coins.

(a) Make a list of all the possible outcomes, as in Table 2.1.

(b) Make a list of all the different "macrostates" and their probabilities.

(c) Compute the multiplicity of each macrostate using the combinatorial formula 2.6, and check that these results agree with what you got by bruteforce counting.

For a single large two-state paramagnet, the multiplicity function is very sharply peaked about N=N/2.

(a) Use Stirling's approximation to estimate the height of the peak in the multiplicity function.

(b) Use the methods of this section to derive a formula for the multiplicity function in the vicinity of the peak, in terms of xN(N/2). Check that your formula agrees with your answer to part (a) when x=0.

(c) How wide is the peak in the multiplicity function?

(d) Suppose you flip 1,000,000coins. Would you be surprised to obtain heads and 499,000 tails? Would you be surprised to obtain 510,000 heads and 490,000 tails? Explain.

For an Einstein solid with each of the following values of N and q , list all of the possible microstates, count them, and verify formula (N,q)=q+N1q=(q+N1)!q!(N1)!

(a) N=3,q=4

(b)N=3,q=5

(c) N=3,q=6

(d) N=4,q=2

(e) N=4,q=3

(f) N=1,q=anything

(g) N= anything, q=1

According to the Sackur-Tetrode equation, the entropy of a monatomic ideal gas can become negative when its temperature (and hence its energy) is sufficiently low. Of course this is absurd, so the Sackur-Tetrode equation must be invalid at very low temperatures. Suppose you start with a sample of helium at room temperature and atmospheric pressure, then lower the temperature holding the density fixed. Pretend that the helium remains a gas and does not liquefy. Below what temperature would the Sackur-Tetrode equation predict that Sis negative? (The behavior of gases at very low temperatures is the main subject of Chapter 7.)

Consider a system of two Einstein solids, with N{A} = 300, N{B} = 200 and q{total} = 100 (as discussed in Section 2.3). Compute the entropy of the most likely macrostate and of the least likely macrostate. Also compute the entropy over long time scales, assuming that all microstates are accessible. (Neglect the factor of Boltzmann's constant in the definition of entropy; for systems this small it is best to think of entropy as a pure number.) 65

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