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Chapter 03Kinetic Theory of Gases
P. J. Grandinetti
Chem. 4300
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
History of ideal gas law1662: Robert Boyle discovered with changing pressure at constant temperature thatproduct of pressure and volume of a gas at equilibrium is constant,
pV = constant at constant T
1780s: Jacques Charles found that ratio of volume to temperature was also invariantwhen temperature was changed with pressure kept constant,
V∕T = constant at constant p
1811: Amedeo Avogadro found ratio of volume to amount remained constant withchanging amount at fixed pressure and temperature,
V∕n = constant at constant p and T
1834: Emile Clapeyron combined gas laws of Boyle, Charles, and Avogadro into idealgas equation of state,
pV = nRTwhere R is gas constant.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Bernoulli’s derivation of Boyle’s law, pV = constant.As early as 1738 Daniel Bernoulli proposed a microscopic kinetic explanation of Boyle’s law,but only after Clapeyron’s work did Bernoulli’s kinetic theory gain widespread acceptance.Bernoulli’s derivation
m
z
xy
Remember pressure is defined as force per unit area.What is the force of one gas molecule hitting a wall?
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Force on wall is momentum change when a molecule hits it.
Force along y is given by ratio of change in momentum to time betweencollisions.
Fy =Δpy
Δt
vy
-vy
Linear momentum is conserved in collision with wall
Δpy = py,final − py,initial = (−mvy) − (mvy) = −2mvy
Time to travel length of box, hit wall, and travel back is Δt = 2𝓁∕vy
Average force of 1 molecule hitting 1 wall of box is Fy =Δpy
Δt=
−2mvy
2𝓁∕vy= −
mv2y
𝓁P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Force of N molecules hitting all walls of the box.Sum over N molecules hitting one wall is
FyN= −m
𝓁
N∑𝛼=1
v2y𝛼
Add magnitude (i.e., ignore signs) of all forces on all 6 walls (top, bottom, left, right, front, back)
Ftotal = 2m𝓁
N∑𝛼=1
v2x𝛼+ 2m
𝓁
N∑𝛼=1
v2y𝛼+ 2m
𝓁
N∑𝛼=1
v2z𝛼
= 2m𝓁
N∑𝛼=1
(v2
x𝛼+ v2
y𝛼+ v2
z𝛼
)⏟⏞⏞⏞⏞⏞⏞⏞⏞⏞⏟⏞⏞⏞⏞⏞⏞⏞⏞⏞⏟
v2𝛼
= 2m𝓁
N∑𝛼=1
v2𝛼
Define mean square velocity as
v2 = 1N
N∑𝛼=1
v2𝛼 or Nv2 =
N∑𝛼=1
v2𝛼
and write total force on all 6 walls of box asFtotal = 2m
𝓁Nv2
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Pressure from N molecules inside the box.Pressure is force per unit area. Total area of box walls is 6 times area of 1 wall: Atotal = 6Awall.
p = Ftotal∕Atotal = Ftotal∕(6Awall) Substituting previous result: Ftotal = 2m𝓁
Nv2
gives
p = 2m𝓁
Nv2∕(6Awall) =Nmv2
3Awall𝓁= Nmv2
3Vwhere V = Awall𝓁 is volume of box
Rearranging gives Boyle’s law (pV = constant)
pV = Nmv2
3= 2
3N(1
2mv2
)= 2
3N𝜖k, where 𝜖k is mean kinetic energy of molecule
Rewriting in terms of moles, i.e., N = nNA where NA is Avogradro constant,
pV = 23
nNA𝜖k = 23
nEk where Ek is kinetic energy of 1 mole of gas
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Temperature is a quantity derived from energyFinally connect to Ideal gas law:
pV = nRT = 23
nEk
and we discoverEk =
32
RT kinetic energy of 1 mole of ideal gas
Equation reveals true nature of temperature—reflects kinetic energy of atoms andmolecules.Can’t have negative temperatures because can’t have negative kinetic energy.Raising gas temperature increases kinetic energy of gas molecules and vice versa.Dividing by NA we obtain relationship on per molecule basis
𝜖k =EkNA
= 32
RNA
T = 32
kBT
kB = R∕NA = 1.38064852 × 10−23 J/K is defined as Boltzmann constant.P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Average molecular speed
Given12
mv2 = 32
kBT
define root mean square speed, crms =√
v2, and obtain
crms =√
3kBTm
=√
3RTM
crms is related to temperature and molecular mass, m, or molar mass, M
Molecular speeds increase with increasing temperature.Molecular speeds decrease with increasing molecular mass.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Average molecular speed
ExampleCalculate the rms speed for a mole of vanillin molecules at room temperature.
SolutionSince Vanillin has chemical formula C8H8O3 with a molecular weight of 152.1 g/mol we obtain
crms =√
3RTM
=
√3R(300 K)
152.1 g/mol≈ 221 m/s ≈ 500 mph
If vanillin has such a high speed why does it take so long for the scent to travel across a room?
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell Distribution Laws
James Clerk Maxwell1831-1879
What is parent probability distribution function formolecular velocities, p(v⃗)molecular speeds, p(c)molecular energies, p(E)?
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell Distribution LawsIn 1859 James Clerk Maxwell worked out the probability distribution of molecular velocities,f (v⃗), for gas molecules as perfectly elastic spheres.
Maxwell assumed that distribution of velocities in each direction were uncorrelated, that is,f (v⃗) can be written as product of 3 independent distributions
f (v⃗) = f (vx) f (vy) f (vz)
He also reasoned that distribution of velocities is independent of direction, implying that f (v⃗)should only depend on magnitude of velocities,
f (vx) f (vy) f (vz) = 𝜙(v2x + v2
y + v2z )
This is an example of a functional equation: an equation in which the unknowns are functions.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
How do we solve this functional equation?
f (vx) f (vy) f (vz) = 𝜙(v2x + v2
y + v2z )
Product of functions on left must give sum of their variables as function argument on right.
A function, f (vi), that satisfies this functional equation is
f (vi) = ae−bv2i
Putting this function into functional equation gives
𝜙(v2x + v2
y + v2z ) = a3e−b(v2
x+v2y+v2
z )
Need to determine a and b.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Normalizing Maxwell’s distribution for molecular velocitiesAs the f (vi) are probability distributions we require them to be normalized,
∫∞
−∞f (vi)dvi = 1 so ∫
∞
−∞ae−bv2
i dvi = 1
requires that a =√
b∕𝜋 and
f (vi) =√
b𝜋
e−bv2i
Taken together Maxwell’s probability distribution then becomes
f (v⃗) = f (vx) f (vy) f (vz) =( b𝜋
)3∕2e−b(v2
x+v2y+v2
z )
Still need to determine b.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular velocitiesFrom Bernoulli’s kinetic theory we learned that v2 = 3kBT∕m.This mean square speed should also be obtained from probability distribution
v2 = ∫ (v2x + v2
y + v2z ) f (v⃗) dv⃗ = 3kBT∕m
Substituting our normalized solution for f (v⃗) we obtain
v2 = ∫∞
−∞ ∫∞
−∞ ∫∞
−∞(v2
x + v2y + v2
z )( b𝜋
)3∕2e−b(v2
x+v2y+v2
z )dvx dvy dvz = 3kBT∕m
Solving this 3D integral equation requires b = m∕(2kBT), and finally obtain
f (v⃗) = 1√(2𝜋)3
(m
kBT
)3∕2e−
12 (v
2x+v2
y+v2z )∕(kBT∕m)
This is Maxwell’s distribution law for molecular velocities: A 3D Gaussian probabilitydistribution with a standard deviation of
√kBT∕m.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular velocitiesMaxwell’s distribution law is a 3D Gaussian distribution centered on v⃗ = 0.
Distribution for one component of velocity vector for N2 gas at 3 different temperatures.
-1500 -1000 -500 0 500 1000 1500
0.0005
0.0000
0.0010
0.0015
0.0020
0.0025
100 K
300 K
1000 K
velocity/ m/s
N2 gas/ s
/m
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular speeds
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular speedsSpeed is magnitude of velocity vector. To get speed distribution transform Maxwell’s velocitydistribution into spherical coordinates,
c =√
v2x + v2
y + v2z , cos 𝜃 =
vz
c, tan𝜙 =
vy
vx.
With this change of variables we find
f (v⃗) = f (c, 𝜃, 𝜙) = 1√(2𝜋)3
(m
kBT
)3∕2e−
12 c2∕(kBT∕m)
This is independent of 𝜃 and 𝜙 so if we put it into the normalization
∫∞
0 ∫𝜋
0 ∫2𝜋
0f (c, 𝜃, 𝜙)c2dc sin 𝜃 d𝜃 d𝜙 = 1
we can integrate away 𝜃 and 𝜙 and obtain
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m) Maxwell’s distribution law
for molecular speeds.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular speeds
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m)
5000 1000 1500 2000
0.0005
0.0000
0.0010
0.0015
0.0020
0.0025
0.0030
0.0035
speed/ m/s
100 K
300 K
1000 K
N2 gas/ s
/m
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Maxwell’s distribution law for molecular speeds
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m)
5000 1000 1500 2000 2500
0.0005
0.0000
0.0010
0.0015
0.0020
0.0025
speed/ m/s
Ar
Ne
He
300 K/ s
/m
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Mean speedWith Maxwell’s distribution law for molecular speeds
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m)
we can calculate the mean speed
c = ∫∞
0cf (c)dc =
√2𝜋
(m
kBT
)3∕2⋅
12
(2kBT
m
)2
which simplifies to
c =√
8kBT𝜋m
=√
8RT𝜋M
Note, mean speed, c, is smaller than root mean square speed, crms =√
3kBTm
.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Most probable speed
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m)
To calculate most probablespeed need to find c value wheref (c) is maximum.Set df (c)∕dc = 0, solve for c toobtain
cmode =√
2kBTm
=√
2RTM
10 2 3 4 5
0.1
0.0
0.2
0.3
0.4
0.5
0.6
speed /
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Fraction of molecules with speeds between c1 and c2.Fraction of molecules with speeds between c1 and c2 is obtained by integrating Maxwell speeddistributions between these two limits,
𝛿NN
= ∫c2
c1
f (c)dc
10 2 3 4 5
0.1
0.0
0.2
0.3
0.4
0.5
0.6
speed /P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Web Apps by Paul Falstad
Kinetic Theory of Gases Simulation
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
1955 - Miller and Kusch experimentally verify Maxwell’s molecular speed distribution.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Miller and Kusch experiments
In 1955 Miller and Kusch published firstconvincing measurements of speeddistribution for K and Tl atoms in gasphase.For each fixed rotation speed onlymolecules with a small range of speeds cantravel from the furnace to the detector.With dimensions given in instrumentdiagram the selected speed is v0 = 𝜔l∕𝜙.Measuring intensity as a function ofrotation speed gives the atomic speeddistribution.
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Miller and Kusch experiments
0.20
5
10
15
20
0.6 0.80.4 1.0 1.2 1.4 1.6 1.8 2.0speed / speed /
0.2 0.6 0.80.4 1.0 1.2 1.4 1.6 1.8 2.0
Inte
nsity
0
5
10
15
20
Inte
nsity
Run 31Run 60Run 57
Run 99Run 97
Potassium vapor Thallium vapor
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Miller and Kusch experiments
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases
Distribution of kinetic energies
Homework
Given
f (c) =√
2𝜋
(m
kBT
)3∕2c2e−
12 c2∕(kBT∕m)
derive distribution of kinetic energies,
f (𝜖k) =2√𝜋
(1
kBT
)3∕2𝜖k
1∕2e−𝜖k∕(kBT)
50 10 15 20 25 30
0.05
0.00
0.10
0.15
0.20
0.25
0.30
0.35
1000 K
300 K
100 K
Energy/ 10-21 J
10-2
1 J
P. J. Grandinetti Chapter 03: Kinetic Theory of Gases