1 Kinetics

1.4 The velocity and speed distributions

(September 1, 2023)

Consider an ideal gas. Each atom is a subsystem with velocity between vx and vx+d⁢vx, vy and vy+d⁢vy, and vz and vz+d⁢vz.

d⁢𝒫v→=C⁢e-m⁢v2/2⁢kB⁢T⁢d⁢vx⁢d⁢vy⁢d⁢vz=P⁢(vx,vy,vz)⁢d3⁢v (1.46)

where C is a normalizing constant and v→2=vx2+vy2+vz2. We can determine C from the normalization condition:

1=∫all v→d𝒫v→= ∫all v→C⁢e-m⁢(vx2+vy2+vz2)/2⁢kB⁢T⁢dvx⁢dvy⁢dvz (1.47)

Doing this integral (which factorizes into and integrals over vx, vy and vz) leads to the distribution of velocities

d⁢𝒫v→=(m2⁢π⁢k⁢T)3/2⁢e-m⁢v→2/2⁢kB⁢T⁢d⁢vx⁢d⁢vy⁢d⁢vz (1.48)

We note that the probability for the vector v→ factorizes into a probability of vx, times a probability of vy, times a probability of vz

d⁢𝒫v→=P⁢(vx)⁢d⁢vx⁢P⁢(vy)⁢d⁢vy⁢P⁢(vz)⁢d⁢vz (1.49)

So, the probability of finding a particle with x-component of velocity in [vx,vx+d⁢vx] is after integrating over vy and vz is

d⁢𝒫vx=P⁢(vx)⁢d⁢vx=(m2⁢π⁢k⁢T)1/2⁢e-m⁢vx2/2⁢kB⁢T⁢d⁢vx (1.50)

The book calls P⁢(vx), the uninformative name g⁢(vx).

To find the speed distribution we have to add up the probabilities d⁢𝒫v→ for all velocities with speed between v and v+d⁢v. This is a spherical shell of width d⁢v (see lecture)

d⁢𝒫v= ∫v→ in shelld𝒫v→ (1.51)
= (m2⁢π⁢k⁢T)3/2⁢e-m⁢v2/2⁢kB⁢T⁢ 4⁢π⁢v2⁢d⁢v≡P⁢(v)⁢d⁢v (1.52)

Explicitly the probability density for speed v is

P⁢(v)=(m2⁢π⁢k⁢T)3/2⁢e-m⁢v2/2⁢kB⁢T⁢ 4⁢π⁢v2 (1.53)

The book calls P⁢(v), the uninformative name f⁢(v).