I wrote:

It seems like the cross section would drop off with the square of the
> distance from the spectator nucleus.  Perhaps something like this:
>
>     σ(r) = 1/(1 + A*r^2),
>
> where A is a constant that is empirically determined; e.g.,
>
>     http://i.imgur.com/eWu4K1i.jpg
>

Another important parameter would be the energy.  Perhaps if you multiplied
the normal d+d cross sections by the curve above you would get a suitable
function for σ(E,r).  Also, I seem to be treating σ as a 0-1 number
probability, but I don't think that's how it generally is treated.

Eric

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