Stringy Model of Cosmological Dark Energy

Journal Article · Tue Nov 20 00:00:00 EST 2007 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2823785· OSTI ID:21039332

Aref'eva, Irina Ya ^[1]

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1. Steklov Mathematical Institute of Russian Academy of Sciences, Gubkin st., 8, 119991, Moscow (Russian Federation)

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.

• OSTI ID: 21039332
• Journal Information: AIP Conference Proceedings, Vol. 957, Issue 1; Conference: PASCOS 2007: 13. international symposium on particles, strings and cosmology, London (United Kingdom), 2-7 Jul 2007; Other Information: DOI: 10.1063/1.2823785; (c) 2007 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COSMOLOGY
INFLATIONARY UNIVERSE
NONLUMINOUS MATTER
QUANTUM FIELD THEORY
SINGULARITY
STRING MODELS
STRING THEORY