What Happens to a Photon Near the Sun in Quantum Gravity?

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SUMMARY

The discussion focuses on the behavior of photons near the Sun when considering quantum gravity (QG). It establishes that in classical general relativity, the angle of deflection of a photon is inversely proportional to the radius from the Sun's center. However, the conversation explores how quantum gravity, despite being an unfinished theory, may introduce complexities such as a minimum length scale and the consequent minimum angle of deflection. The blurring of a photon's location due to its momentum is also highlighted as a significant factor in understanding its trajectory in the context of QG.

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exponent137
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In classical general relativity it is known that angle of deflection is proportional to radius-1 from the center of the sun. If radius is large, this angle is very small, what happens already at the radius of the sun.
But what happens to this photon, when we include quantum gravity (QG)? I know that quantum gravity is unfinished theory. But what are the main the most simple QG approaches to the above example and where the problems arise?
regards
 
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I suspect, if if the smallest length exists, also the smallest angle of deflection of light exists.
If a photon gives small momentum, its location is additionaly blurred.
Because of its own momentum, its locations is primary blurred.
 

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