Non-singular string cosmology via corrections
arXiv:1909.00830 · doi:10.1007/JHEP10(2019)263
Abstract
In string theory, an important challenge is to show if the big-bang singularity could be resolved by the higher derivative corrections. In this work, based on the Hohm-Zwiebach formula, we construct a series of non-singular non-perturbative cosmological solutions with the complete corrections, for the bosonic gravi-dilaton system. In the perturbative regime, these solutions exactly match the perturbative results given in literature. Our results show that the big-bang singularity indeed could be smoothed out by the higher derivative corrections.
V2: 12 pages, 6 figures, references added, V3: typos corrected in equations (3.21) and (3.22), references added, version to appear in JHEP
References in corpus (2)
Cited by in corpus (6)
- New non-perturbative de Sitter vacua in -complete cosmology
- Construct corrected or loop corrected solutions without curvature singularities
- Kalb-Ramond backgrounds in -complete cosmology
- Stability of the non-perturbative de-Sitter spacetime. The isotropic case
- Dilatonic Effect in Double Field Theory Cosmology
- Duality covariant field redefinitions