Feynman Green function inside a Schwarzschild black hole

Physics

Scientific paper

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Theory Of Quantized Fields

Scientific paper

A representation is given for the Feynman Green function corresponding to a scalar field that propagates in Schwarzschild spacetime and which is subject to the Hartle-Hawking boundary conditions. This representation is valid for all values of the Schwarzschild radial coordinate r and is used to obtain an expression for reg for the region interior to the horizon. This expression is evaluated numerically for the range 0.5M

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