The Maxwell-Boltzmann probability distribution function for the energies of the particles in an ideal gas is given by:
f(E) = dN/N = (2/(k*T)^(3/2))*sqrt(E/π)*exp(-E/(k*T)) dE
As is commonly done, let β = 1/(k*T)
f(E) = dN/N = (2/sqrt(π)) * β^(3/2) *sqrt(E)*exp(-β*E) dE
The mean squared energy is given by:
<E^2> = INTEGRAL from 0 to ∞ of {E^2 * f(E) dE}
<E^2> = (2/sqrt(π)) * β^(3/2)*INTEGRAL from 0 to ∞ of
{E^(5/2) * exp(-β*E) dE}
Note that the definition of the Gamma function is:
Γ(x) = INTEGRAL from 0 to ∞ of {t^(x-1) * exp(-t) dt}
Letting t = β*E, (so E = t/β and dE = dt/β), we can write the
integral above as:
<E^2> = (2/sqrt(π)) * β^(3/2)*β^(-7/2)*INTEGRAL from 0 to ∞
of {t^(5/2) * exp(-t) dt}
<E^2> = (2/sqrt(π)) * β^(-2) * Γ(7/2)
Γ(7/2) = 15π/8, so:
<E^2> = (2/sqrt(π)) * β^(-2) * 15π/8
<E^2> = 15*sqrt(π)*(k*T)^2/4
Erms = sqrt(15)*k*T/2
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