Universal approach to gravitational thermal effects
Michael B. Mensky

TL;DR
This paper introduces a universal framework for understanding gravitational thermal effects by generalizing the Unruh effect through the construction of Quasi-Rindler coordinates in curved spacetime, with applications to de Sitter space.
Contribution
It develops a universal scheme for gravitational thermal effects using Quasi-Rindler coordinates, extending the Unruh effect to arbitrary curved spacetimes.
Findings
Constructed Quasi-Rindler coordinates in curved spacetime.
Established the periodicity of imaginary QR time.
Applied the scheme to de Sitter spacetime.
Abstract
A universal scheme for describing gravitational thermal effects is developed as a generalization of Unruh effect. Quasi-Rindler (QR) coordinates are constructed in an arbitrary curved space-time in such a way that the imaginary QR time be periodical. The observer at rest in QR coordinates should experience a thermal effect. Application to de Sitter space-time is considered.
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