2008/10/09 by F. R. Klinkhamer, Klinkhamer, F. R. · 2 citations
Physics and Astronomy · #Astrophysics #Astrophysics (astro-ph) #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Dark energy #Energy (signal processing) #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Phenomenology (hep-ph) #High Energy Physics - Theory (hep-th) #Lorentz covariance #Lorentz factor #Lorentz transformation #Mathematical physics #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Relativity and Gravitational Theory #Theoretical physics #Vacuum energy #astro-ph #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.48550/arxiv.0810.1684
published in arXiv (Cornell University) (Cornell University) · Parallel talk at ICHEP08, Philadelphia, USA, July 2008. 6 pages, LaTeX, 2 eps figures. v4: minor polishing
openalex publication_date 2008/10/09 · arxiv created 2008/11/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
This contribution reviews recent work on a new approach to the cosmological constant problem, which starts from the macroscopic behavior of a conserved relativistic microscopic variable q. First, the statics of the vacuum energy density is discussed and, then, the dynamics in a cosmological context.