For a bi-allelic locus, the model for haploid Natural Selection is:
$$\frac{dp}{dt} = \frac{pW_A}{pW_A + (1-p)W_B}$$
, where $p$ is the frequency of the allele $A$, which relative fitness is $W_A$. $W_B$ is the fitness of the allele $B$, which frequency is $1-p$. $\frac{dp}{dt}$ is the change in allele frequency through time.
The same model for diploid selection is:
$$\frac{dp}{dt} = \frac{p^2W_{AA} + p(1-p)W_{AB}}{p^2W_{AA} + 2p(1-p)W_{AB} + (1-p)^2W_{BB}}$$
, where $W_{AB}$ is the fitness of the diploid genotype carrying the allele $X$ on one chromosome and the allele $Y$ on the other chromosome. We define $W_{AB} = W_{BA}$ and therefore we use only the symbol $W_{AB}$ in the above calculations. Note: This equation assumes Hardy-Weinberg equilibrium.
Those equations can be found in any introductory courses in population genetics. For example, here is a source where you can find this same equation for diploid selection. They just express $q$ instead of $1-p$.
My questions are:
- Do these models assume constant population size? Why?
- Do these models assume threshold selection? Why?
Thank you!