Kinetic Theory of Gases Flashcards
Assumptions
Gases are modelled as hard spheres with no potential and negligible volume.
Spheres are in ceaseless, random motion.
Collisions between gases are brief and elastic.
Energy contribution (kinetic) ΔEi =
(1/2)*mv_x^2
(Only in x direction)
Distribution of this (partition theorem)
We use integral as 1/2mv_x^2 is sufficiently large
f(v_x) = partition with integral and substitution = (m/2pikT)^(1/2)*e^((-mv_x^2)/2kT)
For 3 dimensions speed formula:
c = (v_x^2 +v_y^2+v_z^2)^(1/2)
Using c for partition theorem to get F(c)
=(4pic^2)(m/2pikT)^(3/2)(e^((-mc^2)/2kt))
It is ^3/2 as there are 3 dimensions.
Peak velocity, ĉ
dF(c)/dc = 0
ĉ = ((2kt)/m)1/2
Mean speed, <c></c>
=∫F(c)cdc = ((8kT)/pim)^(1/2)
Integral between 0 and infinty
Root mean squared speed
<c^2>^(1/2)
=[∫F(c)c^2]^(1/2) =((3kT)/m)^(1/2)
Ek for rms
Ek = 1/2mc^2=(m/2)((3kT)/m) =(3/2)kT
(In line with equipartition theorem)
Why are translational energy levels highly degenerate?
For every c there are many combinations of v_x, v_y and v_z’s