Authors: Rajiv Thapa
A novel technique was introduced to re-investigate the “No Drama” conclusion of the Equivalence principle at the event horizon of the Schwarzschild Black Hole. It was found that the Equivalence principle has a different solution at the event horizon, on contrary to the popular belief that the gravitational effect on the observer at the horizon holds the similar properties as that to the observer travelling in the weaker gravitational field.
Comments: 6 Pages.
[v1] 2017-03-15 16:18:32
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