The Feynman Green Function Inside a Schwarzschild Black Hole
Nov, 198516 pages
Published in:
- Phys.Rev.D 33 (1986) 1596
Report number:
- Print-85-0911 (TEXAS)
Citations per year
Abstract: (APS)
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 〈cphi2〉reg for the region interior to the horizon. This expression is evaluated numerically for the range 0.5M- FIELD THEORY: SPACE-TIME
- FIELD THEORY: SCALAR
- TWO-POINT FUNCTION
- black hole
- NUMERICAL CALCULATIONS
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