PreprintCC BY 4.0arXiv
Massive scalar's self-mass from gravitons in de Sitter
Abstract
We compute the fully renormalized one-graviton-loop contribution to the self-mass of a massive scalar field in de Sitter space. The computation is performed using dimensional regularization and the divergences are absorbed by BPHZ counterterms. This self-mass can be used to study one-loop quantum-gravitational corrections to the dynamics of massive spectator scalars in inflation.
Related
- Universal Secular External Leg Corrections for Gauge Independent Scalar Self-Mass on de Sitter
- Dimensionally Regulated Graviton Self-Energy from Gravitons on de Sitter
- Devoured by a Hairy Gargantua: Probing Massive Scalar Charges with Non-minimal Curvature Coupling with Extreme-Mass-Ratio Inspirals
- Casimir effect for a massive scalar field confined between parallel plates with a spatially varying effective mass
- Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals
BibTeX
@misc{glavan2026massive,
title = {{Massive scalar's self-mass from gravitons in de Sitter}},
author = {Dražen Glavan and Shun-Pei Miao and Tomislav Prokopec and Richard P. Woodard},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.21750},
eprint = {2609.21750},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.21750},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Massive scalar's self-mass from gravitons in de Sitter
AU - Dražen Glavan
AU - Shun-Pei Miao
AU - Tomislav Prokopec
AU - Richard P. Woodard
PY - 2026
DA - 2026/09/18
PB - arXiv
DO - 10.48550/arxiv.2609.21750
UR - https://arxiv.org/abs/2609.21750
AB - We compute the fully renormalized one-graviton-loop contribution to the self-mass of a massive scalar field in de Sitter space. The computation is performed using dimensional regularization and the divergences are absorbed by BPHZ counterterms. This self-mass can be used to study one-loop quantum-gravitational corrections to the dynamics of massive spectator scalars in inflation.
ER -