plus those obtained by symmetries of the Riemann Tensor. Confirm that
[ as required ].
and deduce that the orbital equation is
where .
[ Notation as in the lecture notes; this exercise fills in the algebra.]
Derive the orbital equation in Newtonian theory and show that it has the solution
Use the arguement in the lecture notes to show that the GR solution is
Show that the solution for a Photon orbit () is
where b is the impact parameter.
If you have any problems please come and see me or contact me by
email.
Peter Dunsby