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Pre-Big Bang (Gasperini-Veneziano) vs Loop Quantum Big Bounce

← Back to Pre-Big Bang (Gasperini-Veneziano)
Cyclic & Bouncing Cosmologies· within family
Pre-Big Bang (Gasperini-Veneziano)
1993 · Speculative
Loop Quantum Big Bounce
2001 · Speculative
Proposed
1993
2001
Key figures
Maurizio Gasperini, Gabriele Veneziano
Abhay Ashtekar, Martin Bojowald, Parampreet Singh
In one sentence
In string cosmology, a weakly-coupled contracting phase preceded the Big Bang, driven by the dilaton field.
A previous contracting universe bounced, quantum geometry prevented the collapse from becoming a singularity.
Predictions
  • Specific tilted spectrum of gravitational waves (blue tilt)
  • Before the Bang, a quiet low-energy state described by string theory, where all the forces were very weak (a weakly-coupled string vacuum)
  • Universe is asymmetric across the Bang
  • Quantum bounce at Planck density
  • Modified CMB power spectrum at large angular scales
  • Pre-Bang contracting universe phase
Where it breaks
  • Pre-Bang gravity-wave spectrum not yet detected
  • Mechanism of the bounce remains incompletely understood
  • Less developed than LQC bounce
  • Effects only at Planck scale, not currently testable
  • LQG itself is incomplete
  • CMB corrections sub-dominant to cosmic variance
Key unresolved problem
The breakdown at the bounce: at the moment of greatest curvature the low-energy string equations stop working, and no one has an accepted replacement, so the switch from shrinking to expanding is not fully described.
The out-of-reach test: the bounce in loop quantum cosmology only shows up at Planck-scale densities, energies far beyond any experiment we can imagine building, so the prediction stays untestable for now.
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