When Einstein meets Huygens

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 n n given by n = 1 2 V c 2 n=1-\frac {2V}{c^2} , where V V denotes the gravitational potential due to object of mass M M . If the angle of deflection θ \theta of the light coming from the distant object is θ = k G M b c 2 \theta=\frac {kGM}{bc^2} , where b b is the impact parameter (closest distance of approach), compute k 2 k^2 .


The answer is 16.

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1 solution

Richeek Das
Jan 14, 2019

Well , I did this problem by finding the deviation angle using :

α \alpha = 2 c 2 \frac{2}{c^{2}} + ϕ d z \int_{-\infty}^{+\infty} \nabla \phi dz

Where ϕ \phi denotes Gravitational Potential ,i.e ; ϕ \phi = G M r \frac{GM}{r} , where r r = b 2 + z 2 \sqrt{b^{2}+z^{2}}

I will be glad , if someone points out some other elegant way of doing this sum !

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