A class of renormalization group invariant scalar field cosmologies

DOI10.1023/A:1026234623492zbMath1036.83031arXivhep-th/0303154OpenAlexW3103198913WikidataQ57514611 ScholiaQ57514611MaRDI QIDQ1420810

Giampiero Esposito, Alfio Bonanno, Claudio Rubano

Publication date: 23 January 2004

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0303154

zbMATH Keywords

renormalizationscalar fieldCosmologyNewton parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Gravitational interaction in quantum theory (81V17)

Related Items (7)

Running gauge coupling in asymptotically safe quantum gravity ⋮ Dynamical system analysis of cosmologies with running cosmological constant from quantum Einstein gravity ⋮ Entropy production during asymptotically safe inflation ⋮ Variable \(G\) and \(\Lambda\): scalar-tensor versus RG-improved cosmology ⋮ Variable \(G\) and \(\Lambda \) gravity theory and analytical cosmological solutions using Noether symmetry approach ⋮ The role of background independence for asymptotic safety in quantum Einstein gravity ⋮ ON THE POSSIBILITY OF QUANTUM GRAVITY EFFECTS AT ASTROPHYSICAL SCALES

Cites Work

• Unnamed Item
• Recovering the cosmological constant in scalar-tensor cosmologies
• Recovering the effective cosmological constant in extended gravity theories
• Is quantum Einstein gravity nonperturbatively renormalizable?
• The running gravitational couplings
• Cosmologies with variable \(G\) and \(\Lambda\) from action principle
• Scheme independence of the reduction principle and asymptotic freedom in several couplings
• Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point

This page was built for publication: A class of renormalization group invariant scalar field cosmologies