arXiv · 0903.5176
Cosmological perturbations in SFT inspired non-local scalar field models
Abstract
We study cosmological perturbations in models with a single non-local scalar field originating from the string field theory description of the rolling tachyon dynamics. We construct the equation for the energy density perturbations of the non-local scalar field and explicitly prove that for the free field it is identical to a system of local cosmological perturbation equations in a particular model with multiple (maybe infinitely many) local free scalar fields.
Explore related subjects
Keep this discovery
Alexey S. Koshelev, Sergey Yu. Vernov. 2012-07-16. Cosmological perturbations in SFT inspired non-local scalar field models. https://doi.org/10.1140/epjc%2Fs10052-012-2198-4
Cite the original work for its findings. Save a collection to share your selection of sources.