Recent Progress in the Pre-Big Bang Scenario

The pre-big bang scenario describes a dilaton-driven phase emerging from the perturbative string vacuum and preceding the standard hot big bang. Its lowest-order realization is, however, singular and drives the dilaton toward strong coupling. This review summarizes recent progress on two complementary aspects of the scenario. On the phenomenological side, string-phase modifications of scalar and tensor perturbations can generate primordial black holes and a stochastic gravitational-wave background, allowing to probe the structure of the high-curvature epoch. On the theoretical side, the all-order O(d, d) formulation organizes homogeneous α′ corrections and, through a Routhian description, provides simple conditions for regular bouncing solutions. Adding a non-perturbative dilaton potential can then stabilize the string coupling and lead to FLRW or de Sitter attractors, including from anisotropic initial conditions. Together, these results connect the graceful-exit problem with potentially observable relics of the string phase.

Authors

Publication Details

Journal
International Journal of Geometric Methods in Modern Physics
Published
2026-11-06
DOI
https://doi.org/10.1142/s0219887826400189
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
NOV
article

Recent Progress in the Pre-Big Bang Scenario

Pietro Conzinu
International Journal of Geometric Methods in Modern Physics
Cosmology and Gravitation Theories
article

Recent Progress in the Pre-Big Bang Scenario

Pietro Conzinu
article en

Abstract

The pre-big bang scenario describes a dilaton-driven phase emerging from the perturbative string vacuum and preceding the standard hot big bang. Its lowest-order realization is, however, singular and drives the dilaton toward strong coupling. This review summarizes recent progress on two complementary aspects of the scenario. On the phenomenological side, string-phase modifications of scalar and tensor perturbations can generate primordial black holes and a stochastic gravitational-wave background, allowing to probe the structure of the high-curvature epoch. On the theoretical side, the all-order O(d, d) formulation organizes homogeneous α′ corrections and, through a Routhian description, provides simple conditions for regular bouncing solutions. Adding a non-perturbative dilaton potential can then stabilize the string coupling and lead to FLRW or de Sitter attractors, including from anisotropic initial conditions. Together, these results connect the graceful-exit problem with potentially observable relics of the string phase.

International Journal of Geometric Methods in Modern Physics
Openalex Percentile: Top 26%
Cosmology and Gravitation Theories
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon