2006/06/30 by Mathias Garny · 29 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology #Cosmology and Gravitation Theories #Dark energy #Particle physics theoretical and experimental studies #Physics #Quantum #Quantum mechanics #Quintessence #Theoretical physics #astro-ph #hep-ph
paper · pdf · doi:10.1103/physrevd.74.043009
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 74(4) (American Physical Society) · 10 pages + appendix, added references
openalex publication_date 2006/08/31 · arxiv created 2006/09/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We investigate the impact of quantum fluctuations on a light rolling quintessence field from three different sources, namely, from a coupling to the standard model and dark matter, from its self-couplings, and from its coupling to gravity. We derive bounds for time-varying masses from the change of vacuum energy, finding \ensuremathΔme/me\ensuremath≪10^\ensuremath-11 for the electron and \ensuremathΔmp/mp\ensuremath≪10^\ensuremath-15 for the proton since redshift z\ensuremath∼2, whereas the neutrino masses could change of order one. Mass-varying dark matter is also constrained. Next, the self-interactions are investigated. For inverse power law potentials, the effective potential does not become infinitely large at small field values, but saturates at a finite maximal value. We discuss implications for cosmology. Finally, we show that one-loop corrections induce nonminimal gravitational couplings involving arbitrarily high powers of the curvature scalar R, indicating that quintessence entails modified gravity effects.