Pre-Big-Bang in String Cosmology
Monica Borunda, M. Ruiz-Altaba
Abstract
We compute the amount of inflation required to solve the horizon problem of cosmology in the pre-big-bang scenario. First we give a quick overview of string cosmology as developed by Veneziano and collaborators. Then we show that the amount of inflation in this background solves the horizon problem. We discuss fine-tuning.
Create a lesson
Related papers
Heavy-Heavy-Light-Light correlators from holography on the worldsheet
Matías Colaneri, Diego H. Correa, Víctor I. Giraldo-Rivera et al.
Post-Newtonian theory in de Sitter and anti-de Sitter spacetimes
R. Loganayagam, Avi Wadhwa
Thermal AdS two-point functions and loop induced effective one-point vertices
Astha Kakkar
Giant Wilson loops from Fredholm determinants
Ludvig Chen, Victor Mishnyakov, Konstantin Zarembo
Degeneracy graph determinants and higher-dimensional Young diagrams
Sanjaye Ramgoolam, Michał Studziński
Black hole cohomologies in N=4 SYM
Seunggyu Kim, Jehyun Lee, Siyul Lee et al.