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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

Short Answer

Expert verified

(a) The statement is proved below and the entropy of a mole of oxygen at room temperature and atmospheric pressure isS=205.1J/k.

(b) The chemical potential of oxygen in earth's atmosphere near sea level, at room temperature isμ=-0.547eV.

Step by step solution

01

Part (a) step 1: Given information

We have given that 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 Ze

We need to 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.

02

Part (a) step 2: Simplify

The entropy is given as:

S=NkInVNvQ+52-ϑFintϑT

where Fintis the internal Helmholtz free energy and it's given in terms of the internal partition as:

Fint=-NktIn(Zint)

for a diatomic gas, the internal partition function is simply the rotational partition function multiplied by the degeneracy of the electronic ground state Ze,the at is:

Zint=ZeZrot

substitute into (2)to get:

Fint=-NkTIn(ZeZrot)

the partial derivative with respect to the temperature is, So(note that Zrotis proportional to T):

ϑFintϑt=-NkIn(ZeZrot0-nk

substitute into (1)to get:

S=NkInVNvQ+52+nKIn(ZeZrot)+NkS=NkInVNvq+In(ZeZrot)+52S+NKInVZeZrotNvQ+72 (3)

Considering an oxygen molecule at the room temperature and atmospheric pressure where Ze=3. The rotation partition for a diatomic gas is given by:

Zrot=kT2∈

Here,∈is the energy constant, which equals 0.00018eVfor oxygen. So at the room temperature, the rotational partition function is:

The quantum volume will be given as:

vQ=h22Ï€³¾°ì°Õ

The mass of the oxygen molecule O2is 32u,hereu=1.66-27kg, substituting (not that h=6.626×10-34J.sand k=1.38×10-23J/K):

vQ=(6.626×10-34J.s)22π(32×1.66×10-27kg)(1.38×10-23J/K)(300K)=5.66×10-33m3

the volume per particle is written as (from the ideal gas law):

VN=kTP

at a pressure of 1atmand the room temperature we have:

vN=(1.38×10-23J/K)(300K)1.01×105Pa=4.1×10-26m3

plug all these numbers into the natural logarithm in the equation (3)to get:

InVZeZrotNvQ=In(4.1×10-26m3)(3)(71.8)5.66×10-33m3=21.17

now substitute into the equation (3)to get the entropy as:

S=Nk21.17+72

but Nk=nR,

S=n(8.314J/K.mol)21.17+72

for one mole n=1,

S=(8.314J/K)21.17+72=205.1J/KS=205.1J/K

03

Part (b) step 1: Given information

We have given that 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.

We need to calculate the chemical potential of oxygen in earth's atmosphere near sea level, at room temperature.

04

Part (b) step 2: Simplify

The chemical potential is given by:

μ=-kTInVZeZrotNvQ

substitute with the values to get:

μ=-(8.62×10-5eV/K)(300K)(21.17)=-0.547eVμ=-0.547eV

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Most popular questions from this chapter

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.

Use Boltzmann factors to derive the exponential formula for the density of an isothermal atmosphere, already derived in Problems 1.16 and 3.37. (Hint: Let the system be a single air molecule, let s1 be a state with the molecule at sea level, and let s2 be a state with the molecule at height z.)

Some advances textbooks define entropy by the formula

S=-k∑sPslnPs

where the sum runs over all microstates accessible to the system and Psis the probability of the system being in microstate s.

(a) For an isolated system, role="math" localid="1647056883940" Ps=1Ωfor all accessible states s. Show that in this case the preceding formula reduces to our familiar definition of entropy.

(b) For a system in thermal equilibrium with a reservoir at temperatureT,role="math" localid="1647057328146" Ps=e-EskTZ. Show that in this case as well, the preceding formula agrees with what we already know about entropy.

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.

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