Analyticity properties and thermal effects for general quantum field theory on de Sitter space-time
Jacques Bros, Henri Epstein, Ugo Moschella

TL;DR
This paper develops a general framework for quantum field theory on de Sitter space-time, demonstrating that observers detect thermal radiation and establishing key theorems in this setting.
Contribution
It introduces a weak spectral condition based on analytic continuation, extending quantum field theory to more general local fields on de Sitter space.
Findings
Observers detect blackbody radiation at temperature T=1/(2πR)
Proves analogues of PCT, Reeh-Schlieder, and Bisognano-Wichmann theorems in this framework
Framework accommodates non-vanishing truncated Wightman functions
Abstract
We propose a general framework for quantum field theory on the de Sitter space-time (i.e. for local field theories whose truncated Wightman functions are not required to vanish). By requiring that the fields satisfy a weak spectral condition, formulated in terms of the analytic continuation properties of their Wightman functions, we show that a geodesical observer will detect in the corresponding ``vacuum'' a blackbody radiation at temperature T=1/(2 \pi R). We also prove the analogues of the PCT, Reeh-Schlieder and Bisognano-Wichmann theorems.
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