Skip to content
CosmosExplorer
Ch.01 Before the UniverseCyclic & Bouncing Cosmologies

The universe didn't begin. It contracted, hit a minimum, and bounced into ours.

Simple Big Bounce

variousVarious authorsSpeculative2 primary sources, 2 established Reviewed May 14, 2026

The universe contracted to a minimum size and then bounced into expansion. The Big Bang was not a beginning but a transition.

Skip 3D content

§1 · The claim, in one sentence

The Simple Big Bounce treats our universe as the rebound of a previously contracting universe, with the Big Bang as the minimum-size moment of that transition.

§2 · Why it might be true

The Simple Big Bounce is a more general version of the bouncing-universe concept than specific mechanism-based variants like the LQC Big Bounce. The basic idea: a previously contracting universe reached some minimum size or maximum density and then began expanding again. The 'Big Bang' that we infer from extrapolation backward is actually the bounce point.

Different versions of the Simple Big Bounce propose different mechanisms for the bounce. Quantum gravitational effects, modified gravity theories (like f(R) gravity), and specific scenarios have all been proposed. What unites them is the basic picture of a contracting universe transitioning to an expanding universe without going through a true .

This family of models is broader than any specific implementation. Some are more developed (LQC) and some are more speculative. The Simple Big Bounce, as a category, is older and more general than the more specific mathematical models that fall within it.

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.

§2.5 · Evidence

  • Avoids the initial singularity problem of standard cosmology
  • Provides a physical answer to "what existed before"
  • Multiple specific mechanisms (LQC, , modified gravity) have been developed

§3 · What you'd need to test it

  • The universe did not begin at a singularity but at a finite bounce point
  • Some matter or radiation from the previous contracting phase may be detectable
  • Specific signatures in the CMB depend on the bounce mechanism

§4 · Where it breaks

  • No direct observational evidence of a contracting pre-Big Bang phase
  • Different bounce mechanisms make different predictions, making the framework difficult to test as a single theory
  • Some bounce mechanisms require fine-tuning to avoid sending the universe into a singularity anyway
Go deeper

The Simple Big Bounce concept goes back to at least the 1930s, when several physicists proposed that a contracting universe might bounce rather than collapse into a singularity. The development of and the singularity theorems of Hawking and Penrose initially seemed to rule this out, but specific mechanisms (notably modifications to gravity at high curvature) have since revived the idea.

The Loop Quantum Big Bounce (Bojowald, Ashtekar, Pawlowski, Singh, 2001-2006) is the most developed specific implementation. Other mechanisms include the Ekpyrotic bounce, the dilaton-driven bounce of Pre-Big Bang cosmology, and various proposals from modified gravity.

The category remains useful because not every observation that points to a bounce will specify the bounce mechanism. CMB predictions that are robust across many bounce mechanisms could provide circumstantial evidence for the category as a whole.

§5 · Who built it, and when(2 sources, 2 established)
  1. Established
    Brandenberger & Peter (2017). 'Bouncing cosmologies: progress and problems.' Found. Phys. 47, 797570 citations
  2. Established
    Tolman (1934). 'Relativity, Thermodynamics, and Cosmology.' Oxford University Press
Simple Big Bounce, Various authors20052001200119931989

Variants in this family

Compare variants
0votes
Currently #2 in this family · #6 in Ch.1

Up next

Spotted an error? Have a source to add?

Prefer email?

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