On (dis)agreement between different methods of calculation of the imaginary part of the effective action in expanding space-times
arXiv:2411.02170 · doi:10.1016/j.physletb.2025.139256
Abstract
We consider two approaches to calculate imaginary parts of effective actions in expanding space-times. While the first approach uses Bogolyubov coefficients, the second one uses the functional integral or the Feynman propagator. In eternally expanding space-times these two approaches give different answers for the imaginary parts. The origin of the difference can be traced to the presence if the wave-functionals for the initial and final states in the functional integral. We show this explicitly on the example of the expanding Poincare patch of the de Sitter space-time.
References in corpus (6)
- De Sitter Space and Eternity
- Cosmological Particle Production: A Review
- Large-order Perturbation Theory and de Sitter/Anti de Sitter Effective Actions
- Quantum fields in the future Rindler wedge
- Complex effective actions and gravitational pair creation
- Is the Euclidean path integral always equal to the thermal partition function?