Abstract
One of the greatest problems of primordial inflation is that the inflationary space-time is past-incomplete. This is mainly because Einstein's GR suffers from a space-like Big Bang singularity. It has recently been shown that ghost-free, non-local higher-derivative ultra-violet modifications of Einstein's gravity may be able to resolve the cosmological Big Bang singularity via a non-singular bounce. Within the framework of such non-local cosmological models, we are going to study both sub- and super-Hubble perturbations around an inflationary trajectory which is preceded by the Big Bounce in the past, and demonstrate that the inflationary trajectory has an ultra-violet completion and that perturbations do not suffer from any pathologies.
Original language | English |
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Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2012 |
Issue number | 8 |
Pages (from-to) | 024 |
ISSN | 1475-7516 |
DOIs | |
Publication status | Published - 1 Aug 2012 |