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We discuss a possible extension of calculations of the bending angle of light in a static, spherically symmetric and asymptotically flat spacetime to a non-asymptotically flat case.
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K = R r ϕ r ϕ / det ( γ I J ) K=R_{r\phi r\phi}/\det(\gamma_{IJ}) in our notation. See e.g. Eq. (16) in Werner(2012) [ 36 ] . K K can diverge at r = 0 r=0 for black hole cases. For such cases, it is likely that Eq. ( 22
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