Renormalization group inspired autonomous equations for secular effects in de Sitter space
arXiv:2005.02504 · doi:10.1103/PhysRevD.102.065010
Abstract
We develop a method for treating a series of secularly growing terms obtained from quantum perturbative calculations: autonomous first-order differential equations are constructed such that they reproduce this series to the given order. The exact solutions of these equations are free of secular terms and approach a finite limit at late times. This technique is illustrated for the well-known problem of secular growth of correlation functions of a massless scalar field with a quartic self-interaction in de Sitter space. For the expectation value of the product of two fields at coinciding space-time points we obtain a finite late-time result that is very close to the one following from Starobinsky's stochastic approach.
20 pages
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Cited by in corpus (9)
- Unitarity of quantum-gravitational corrections to primordial fluctuations in the Born-Oppenheimer approach
- Observations in Quantum Cosmology
- Massive scalar field in de Sitter spacetime: a two-loop calculation and a comparison with the stochastic approach
- IR finite correlation functions in de Sitter space, a smooth massless limit, and an autonomous equation
- Non-perturbative analysis for a massless minimal quantum scalar with in the inflationary de Sitter spacetime
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- When tadpoles matter: One-loop corrections for spectator Higgs in inflation
- Resummation of local and non-local scalar self energies via the Schwinger-Dyson equation in de Sitter spacetime
- From the Fokker-Planck equation to perturbative QFT's results in de Sitter space