vix.ing · top · new · best · stats · spec

Cosmological constant, renormalization group and Planck scale physics

2003/05/25 by Ilya L. Shapiro, Joan Solà, Joan Sola · 2 citations
Physics and Astronomy · #Advanced Mathematical Theories and Applications #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #astro-ph #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1016/s0920-5632(03)02402-2

LaTeX, 6 pages, no figures. Talk presented at IRGA 2003: Renormalization Group and Anomalies in Gravitation and Cosmology, Ouro Preto, Brazil, 16-23 March, 2003

arxiv created 2003/05/25 · openalex publication_date 2004/02/01 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Starting from generic quantum effects at the Planck scale MP, we find that the renormalization group running of the cosmological constant (CC) at low energies is possible if there is a smooth decoupling of all massive particles from MP to the mass of the lightest neutrino. We discuss the theoretical implications of this running for the ``old'' and ``new'' cosmological constant problems. Interestingly enough, the CC running implies a strong relationship between quantum field theory and cosmology, which should be observable in the near future in experiments such as SNAP through the measurement of a cubic redshift dependence of the CC.

Cited by