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Thermal loops in the accelerating frame
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abstract
We consider the conformal scalar field theory with $\lambda \phi^4$ self-interaction in Rindler and Minkowskian coordinates at finite temperature planckian distribution for the exact modes. The solution of the one-loop Dyson-Schwinger equation is found to the order in $\lambda^{3/2}$. Appearance of the thermal (Debye) mass is shown. Unlike the physical mass, the thermal one gives a gap in the energy spectrum in the quantization in the Rindler coordinates. The difference between such calculations in Minkowski and Rindler coordinates for the exact modes is discussed. It is also shown that states with a temperature lower than the Unruh one are unstable. It is proved that for the canonical Unruh temperature the thermal mass is equal to zero. The contribution to the quantum average of the stress-energy tensor is also calculated, it remains traceless even in the presence of the thermal mass.
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Cited by 1 Pith paper
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On the late time behavior of thermal two point function in curved space-time
For thermal Bose fields in static de Sitter or a planar BTZ black hole, the late-time correlation decay switches from temperature-limited to quasinormal-mode-limited at a critical temperature Tc.
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