(i) Consider a thin lens placed between a source (S) and an observer (O) (Figure). Let the thickness of the lens vary as w(b)=w0-b2α, where b is the verticle distance from the pole, w0 is a constant. Using Fermat's principle i.e., the time of transit for a ray between the source and observer is an extremum, find the condition that all paraxial rays starting from the source will converge at a point O on the axis. Find the focal length.
              
(ii) A gravitational lens may be assumed to have a varying width of the form
                         w(b)=k1lnk2bbmin<b<bmax
                             =k1lnk2bminb<bmin
Show that an observer will see an image of a point object as a ring about the centre of the lens with an angular radius
                             β=(n-1)k1uvu+v