Abstract
Recent progress on nonlinear sigma models on de Sitter background has permitted the resummation of large inflationary logarithms by combining a variant of Starobinsky's stochastic formalism with a variant of the renormalization group. We reconsider single graviton loop corrections to the photon wave function, and to the Coulomb potential, in light of these developments. Neither of the two 1-loop results have a stochastic explanation, however, the flow of a curvature-dependent field strength renormalization explains their factors of ln(a). We speculate that the factor of ln(Hr) in the Coulomb potential should not be considered as a leading logarithm effect.
| Original language | English |
|---|---|
| Article number | 195 |
| Number of pages | 18 |
| Journal | Journal of High Energy Physics |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 29 Aug 2023 |
Funding
DG was supported by the European Union and the Czech Ministry of Education, Youth and Sports (Project: MSCA Fellowship CZ FZU I - CZ.02.01.01/00/22_010/0002906). SPM was supported by Taiwan NSTC grants 111-2112-M-006-038 and 112-2112-M-006-017. TP was supported by the D-ITP consortium, a program of the Netherlands Organization for Scientific Research (NWO) that is funded by the Dutch Ministry of Education, Culture and Science (OCW). RPW was supported by NSF grant PHY-2207514 and by the Institute for Fundamental Theory at the University of Florida.
| Funders | Funder number |
|---|---|
| European Union | 111-2112-M-006-038 |
| Czech Ministry of Education, Youth and Sports (Project: MSCA Fellowship) | 112-2112-M-006-017, PHY-2207514 |
| Taiwan NSTC grants | |
| D-ITP consortium, a program of the Netherlands Organization for Scientific Research (NWO) - Dutch Ministry of Education, Culture and Science (OCW) | |
| NSF | |
| Institute for Fundamental Theory at the University of Florida | |
| ???publication-publication-funding-organisation-not-added??? | CZ FZU I CZ.02.01.01/00/22_010/0002906 |
Keywords
- Renormalization Group
- de Sitter space
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