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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.)

Short Answer

Expert verified

Therefore, the exponential formula for the density of an isothermal atmosphere is:ÒÏ(z)=ÒÏ(0)e-mgz/kT

Step by step solution

01

Given information

Let the system be a single air molecule, let S1be a state with the molecule at sea level, and let S2 be a state with the molecule at height z.

02

Explanation

Consider a system with a single air molecule, where S1 is the state when the molecule is at sea level and S2is the state when the molecule is at a height of 2. Assume that the energy is only potential energy, so the difference in energy between the states S1and S2is the potential energy, which is ΔE=mgz and the ratio of S2state probability to state s1 probability is:

role="math" localid="1647369610229" Ps2Ps1=e-E2/kTe-E1/kT=e-ΔE/kTPs2Ps1=e-mgz/kT

This means that the air molecule is less likely to be at height of z than at the see level by a factor of e-mgz/kT, and that the number of molecules per unit volume at height of z is also smaller than the see level by the same ratio in the isothermal atmosphere, so:

ÒÏ(z)=ÒÏ(0)e-mgz/kT

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