# Classical scattering

1. Sep 13, 2011

### Amith2006

I have spent lot of time trying to understand scattering from Goldstein but in vain. The general equation of an orbit is,

1/r = K[1 + e*cos(θ - θ')] where e=eccentricity
I refer to a sentence in goldstein which says, if θ'=pi then θ = 0 corresponds to the periapsis. What is θ' in the case of hyperbolic orbit? As far as the general equation is concerned, θ' is one of the turning angles of the orbit but in scattering there is only one turning angle which corresponds to the periapsis.
Then the equation becomes,
1/r = K[1 - e*cos(θ)]