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Euclidean scalar and spinor Green's functions in Rindler space
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abstract
In Rindler space, we consider the Feynman Green's functions associated with either the Fulling-Rindler vacuum or the Minkowski vacuum. In Euclidean field theory, they becomes respectively the Euclidean Green's functions $G_{\infty}$ and $G_{\2\pi}$, whose we give different suitable forms. In the case of the massive spin-$\frac{1}{2}$ field, we determine also the Euclidean spinor Green's function $S_{\infty}$ and $S_{\2\pi}$ in different suitable forms. In both cases for massless fields in four dimensions, we compute the vacuum expectation value of the energy-momentum tensor relative to the Rindler observer.
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Cited by 1 Pith paper
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A Measure for Quantum Paths, Gravity and Spacetime Microstructure
The Einstein-Hilbert action is expressed as the zero-length limit of the total proper length of closed quantum loops, with the loop measure defined through a Fourier transform of the Feynman propagator.
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