On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction
Abstract In this paper, we revisit the infrared (IR) divergences in de Sitter (dS) space using the wavefunction method, and explicitly explore how the resummation of higher-order loops leads to the stochastic formalism. In light of recent developments of the cosmological bootstrap, we track the beha...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
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SpringerOpen
2024-04-01
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| Series: | Journal of High Energy Physics |
| Subjects: | |
| Online Access: | https://doi.org/10.1007/JHEP04(2024)004 |
| _version_ | 1797220076030525440 |
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| author | Sebastián Céspedes Anne-Christine Davis Dong-Gang Wang |
| author_facet | Sebastián Céspedes Anne-Christine Davis Dong-Gang Wang |
| author_sort | Sebastián Céspedes |
| collection | DOAJ |
| description | Abstract In this paper, we revisit the infrared (IR) divergences in de Sitter (dS) space using the wavefunction method, and explicitly explore how the resummation of higher-order loops leads to the stochastic formalism. In light of recent developments of the cosmological bootstrap, we track the behaviour of these nontrivial IR effects from perturbation theory to the non-perturbative regime. Specifically, we first examine the perturbative computation of wavefunction coefficients, and show that there is a clear distinction between classical components from tree-level diagrams and quantum ones from loop processes. Cosmological correlators at loop level receive contributions from tree-level wavefunction coefficients, which we dub classical loops. This distinction significantly simplifies the analysis of loop-level IR divergences, as we find the leading contributions always come from these classical loops. Then we compare with correlators from the perturbative stochastic computation, and find the results there are essentially the ones from classical loops, while quantum loops are only present as subleading corrections. This demonstrates that the leading IR effects are contained in the semi-classical wavefunction which is a resummation of all the tree-level diagrams. With this insight, we go beyond perturbation theory and present a new derivation of the stochastic formalism using the saddle-point approximation. We show that the Fokker-Planck equation follows as a consequence of two effects: the drift from the Schrödinger equation that describes the bulk time evolution, and the diffusion from the Polchinski’s equation which corresponds to the exact renormalization group flow of the coarse-grained theory on the boundary. Our analysis highlights the precise and simple link between the stochastic formalism and the semi-classical wavefunction. |
| first_indexed | 2024-04-24T12:43:47Z |
| format | Article |
| id | doaj.art-8d45c632d37b42388b843608776a4150 |
| institution | Directory Open Access Journal |
| issn | 1029-8479 |
| language | English |
| last_indexed | 2024-04-24T12:43:47Z |
| publishDate | 2024-04-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | Journal of High Energy Physics |
| spelling | doaj.art-8d45c632d37b42388b843608776a41502024-04-07T11:06:16ZengSpringerOpenJournal of High Energy Physics1029-84792024-04-012024415810.1007/JHEP04(2024)004On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunctionSebastián Céspedes0Anne-Christine Davis1Dong-Gang Wang2Department of Physics, Imperial CollegeDepartment of Applied Mathematics and Theoretical Physics, University of CambridgeDepartment of Applied Mathematics and Theoretical Physics, University of CambridgeAbstract In this paper, we revisit the infrared (IR) divergences in de Sitter (dS) space using the wavefunction method, and explicitly explore how the resummation of higher-order loops leads to the stochastic formalism. In light of recent developments of the cosmological bootstrap, we track the behaviour of these nontrivial IR effects from perturbation theory to the non-perturbative regime. Specifically, we first examine the perturbative computation of wavefunction coefficients, and show that there is a clear distinction between classical components from tree-level diagrams and quantum ones from loop processes. Cosmological correlators at loop level receive contributions from tree-level wavefunction coefficients, which we dub classical loops. This distinction significantly simplifies the analysis of loop-level IR divergences, as we find the leading contributions always come from these classical loops. Then we compare with correlators from the perturbative stochastic computation, and find the results there are essentially the ones from classical loops, while quantum loops are only present as subleading corrections. This demonstrates that the leading IR effects are contained in the semi-classical wavefunction which is a resummation of all the tree-level diagrams. With this insight, we go beyond perturbation theory and present a new derivation of the stochastic formalism using the saddle-point approximation. We show that the Fokker-Planck equation follows as a consequence of two effects: the drift from the Schrödinger equation that describes the bulk time evolution, and the diffusion from the Polchinski’s equation which corresponds to the exact renormalization group flow of the coarse-grained theory on the boundary. Our analysis highlights the precise and simple link between the stochastic formalism and the semi-classical wavefunction.https://doi.org/10.1007/JHEP04(2024)004de Sitter spaceCosmology of Theories BSMNonperturbative EffectsRenormalization Group |
| spellingShingle | Sebastián Céspedes Anne-Christine Davis Dong-Gang Wang On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction Journal of High Energy Physics de Sitter space Cosmology of Theories BSM Nonperturbative Effects Renormalization Group |
| title | On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction |
| title_full | On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction |
| title_fullStr | On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction |
| title_full_unstemmed | On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction |
| title_short | On the IR divergences in de Sitter space: loops, resummation and the semi-classical wavefunction |
| title_sort | on the ir divergences in de sitter space loops resummation and the semi classical wavefunction |
| topic | de Sitter space Cosmology of Theories BSM Nonperturbative Effects Renormalization Group |
| url | https://doi.org/10.1007/JHEP04(2024)004 |
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