# IR finite correlation functions in de Sitter space, a smooth massless limit, and an autonomous equation

- Institution: CERN
- Department: TH institutes
- Speaker: Polina Petriakova
- Year: 2024
- Language: English
- Subjects: Astronomy and space
- Source: [CERN](https://videos.cern.ch/record/3020127)
- Licence: [CERN](http://copyright.web.cern.ch)
- Who can watch: Tweens profiles and older (sources give no ratings; placed by Invisible Network from the source's own words)

Currently, the study of cosmological correlation functions is extremely favored, and a large number of new techniques are being developed. I will discuss a less-fashioned but very efficient technique to calculate the loop corrections to the correlation function in the long-wavelength approximation. By employing the Yang-Feldman-type equation, we compute the two-point correlation function up to the three-loop level and the four-point correlation function up to the two-loop one. In contrast to the standard theory of a massive scalar field based on the de Sitter-invariant vacuum, we develop the vacuum-independent reasoning that may not possess de Sitter invariance but results in a smooth massless limit of the correlation function's infrared part. Our elaboration affords to calculate correlation functions of a free massive scalar field and to proceed with quantum corrections, relying only on the known two-point correlation function's infrared part of a free massless one. Remarkably, the two-point correlation function of a free massive scalar field coincides with the Ornstein-Uhlenbeck stochastic process's one and has a clear physical interpretation. We compared our results with those obtained with the Schwinger-Keldysh diagrammatic technique, Starobinsky's stochastic approach, and the Hartree-Fock approximation. At last, I will also discuss a way to generalize the obtained results to the non-perturbative case, as well as further prospects in this direction.

Based on arXiv: \[2410.16226\]..

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## Lectures

1. [IR finite correlation functions in de Sitter space, a smooth massless limit, and an autonomous equation](https://invisiblenetwork.ai/learn/cern/3020127/8d897ce74c43), 23 min (CERN's player)