Stringy Model of Cosmological Dark Energy
arXiv:0710.3017 · doi:10.1063/1.2823785
Abstract
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.
Talk at PASCOS 2007, to appear in the proceedings, 5 pages, latex
References in corpus (3)
Cited by in corpus (15)
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- Pure Gauge Configurations and Tachyon Solutions to String Field Theories Equations of Motion
- Exact Solutions for Nonlocal Nonlinear Field Equations in Cosmology
- Perturbative stability of SFT-based cosmological models
- Multi-scalar field cosmology from SFT: an exactly solvable approximation
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- Convexity of effective Lagrangian in nonlinear electrodynamics as derived from causality
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- Exact Solutions in Nonlocal Linear Models