Exponential freeze-out sensitivity (source code)

= Exponential freeze-out sensitivity
{title2=$d\ln n_0/dP=3/(2P)-1$}

In a supplied equilibrium-cutoff model with $P=mc^2/(k_BT_f)$, present <number density> can contain $P^{3/2}e^{-P}$. The logarithmic derivative is $3/(2P)-1$, making small changes in a large <cosmological particle freeze-out> parameter important for the inferred abundance.