De Sitter space and perpetuum mobile
arXiv:0905.2742 · doi:10.1134/S1063778812040023
Abstract
We give general arguments that any interacting non--conformal {\it classical} field theory in de Sitter space leads to the possibility of constructing a perpetuum mobile. The arguments are based on the observation that massive free falling particles can radiate other massive particles on the classical level as seen by the free falling observer. The intensity of the radiation process is non-zero even for particles with any finite mass, i.e. with a wavelength which is within the causal domain. Hence, we conclude that either de Sitter space can not exist eternally or that one can build a perpetuum mobile.
11 pages revtex, no figures. Added discussion to strengthen conclusion
References in corpus (3)
Cited by in corpus (28)
- Lecture notes on interacting quantum fields in de Sitter space
- An effective field theory during inflation: reduced density matrix and its quantum master equation
- An effective field theory during inflation II: stochastic dynamics and power spectrum suppression
- Perturbative Quantum Gravity Comes of Age
- Infrared dynamics of the massive theory on de Sitter space
- Effective Field Theory out of Equilibrium: Brownian quantum fields
- Condensates and quasiparticles in inflationary cosmology: mass generation and decay widths
- Solution of the Dyson--Schwinger equation on de Sitter background in IR limit
- Secularly growing loop corrections in strong electric fields
- Physical meaning and consequences of the loop IR divergences in global dS
- Spontaneous symmetry breaking in inflationary cosmology: on the fate of Goldstone Bosons
- De Sitter Stability and Coarse Graining
- Massive scalar field evolution in de Sitter
- Pre-slow roll initial conditions: large scale power suppression and infrared aspects during inflation
- Imprint of entanglement entropy in the power spectrum of inflationary fluctuations
- IR Divergences in Inflation and Entropy Perturbations
- Particle production in a gravitational wave background
- Superhorizon entanglement entropy from particle decay in inflation
- Fermionic influence (action) on inflationary fluctuations
- New Geometric Transition as Origin of Particle Production in Time-Dependent Backgrounds
- On quantization in background scalar fields
- Electron as a Tiny Mirror: Radiation From a Worldline With Asymptotic Inertia
- Time evolution of cascade decay
- Horizon Feedback Inflation
- Cosmological Particle Creation Beyond de Sitter
- Out of equilibrium two-dimensional Yukawa theory in a strong scalar wave background
- On radiation due to homogeneously accelerating sources
- Late-time quantum radiation by a uniformly accelerated detector in de Sitter spacetime