Skip to content
CosmosExplorer
Chapter 01 · Before the Universe/Cyclic & Bouncing Cosmologies

Pre-Big Bang (Gasperini-Veneziano)

1993 · Maurizio Gasperini, Gabriele Veneziano
Speculative

String theory predicts a dilaton-driven contracting phase before the Bang.

Skip 3D content

In one sentence

In string cosmology, a weakly-coupled contracting phase preceded the Big Bang, driven by the dilaton field.

The claim

The Pre-Big Bang scenario emerges from low-energy string theory. The string action contains a scalar field called the dilaton, which controls the strength of all forces. In the Pre-Big Bang model, the universe began in an empty, cold, weakly-coupled state with the dilaton at very negative values. The dilaton-driven dynamics led to accelerating expansion ("dilaton-driven inflation") that ended at a high-curvature bounce.

After the bounce, the universe entered the standard hot Big Bang phase. The asymmetry between the pre-Bang and post-Bang phases is a defining feature: cold and contracting before, hot and expanding after.

The family stance

A previous cycle, aeon, contracting phase, or alternate-brane state existed before our universe. The "before" is a physically connected predecessor, not nothing or another arena.

Predictions

  • Specific tilted spectrum of gravitational waves (blue tilt)
  • Pre-Bang phase has weakly-coupled string vacuum
  • Universe is asymmetric across the Bang

Evidence

  • Naturally derived from string theory low-energy action
  • Avoids singularity via high-curvature regime

Counterpoints

  • Pre-Bang gravity-wave spectrum not yet detected
  • Mechanism of the bounce remains incompletely understood
  • Less developed than LQC bounce
0votes
Go deeperTechnical detail with proper terminology

The Gasperini-Veneziano scenario uses the duality symmetries of string theory. The pre-Bang and post-Bang phases are related by scale-factor duality: a(t) ↔ 1/a(-t). The dilaton φ runs from -∞ to a finite value across the bounce.

The high-curvature bounce regime is where string-scale physics dominates and the low-energy effective action breaks down. Various proposed completions (loop corrections, string-theoretic completions) attempt to describe this transition, but none is universally accepted.

References

  1. Established
    Gasperini & Veneziano (1993). Astropart. Phys. 1, 317
  2. Established
    Gasperini & Veneziano (2003). Phys. Rep. 373, 1 (review)

Spotted an error? Have a source to add?

Prefer email?

You can also send a prefilled email with the variant URL already filled in.

Related theories