In Einstein's theory of gravity an electromagnetic wave passing near a massive object is bent from its rectilinear path. We may regard this bending equivalently as due to a medium of refractive index given by , where denotes the gravitational potential due to object of mass . If the angle of deflection of the light coming from the distant object is , where is the impact parameter (closest distance of approach), compute .
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Well , I did this problem by finding the deviation angle using :
α = c 2 2 ∫ − ∞ + ∞ ∇ ϕ d z
Where ϕ denotes Gravitational Potential ,i.e ; ϕ = r G M , where r = b 2 + z 2
I will be glad , if someone points out some other elegant way of doing this sum !