2007/01/01 by I. Ya. Aref’eva, Irina Ya. Aref'eva, Arttu Rajantie +3 · 2 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Particle physics theoretical and experimental studies #hep-th
paper · pdf · doi:10.1063/1.2823785
published as AIPConf.Proc.957:297-300,2007 · Talk at PASCOS 2007, to appear in the proceedings, 5 pages, latex
openalex publication_date 2007/01/01 · arxiv created 2007/10/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29
A string field theory (SFT) nonlocal model of the cosmological dark energy providing w<−1 is briefly surveyed. We summarize recent developments and open problems, as well as point out some theoretical issues related with others applications of the SFT nonlocal models in cosmology, in particular, in inflation and cosmological singularity.