Using a regulated point-source stress-energy tensor and integrating the Einstein equations near the origin, the paper obtains the identification r_s = 2GM directly within general relativity, without Newtonian asymptotics.
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A Purely Relativistic Point-Source Boundary Condition for the Schwarzschild Solution
Using a regulated point-source stress-energy tensor and integrating the Einstein equations near the origin, the paper obtains the identification r_s = 2GM directly within general relativity, without Newtonian asymptotics.