Big Crunch scenario

E737174

The Big Crunch scenario is a cosmological hypothesis in which the expansion of the universe eventually reverses, causing all matter and space to collapse back into an extremely dense, hot state.

All labels observed (2)

Label Occurrences
Big Crunch 3
Big Crunch scenario canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf cosmological hypothesis ⓘ
end-of-universe scenario ⓘ
theoretical cosmological model ⓘ
alsoKnownAs Big Crunch ⓘ
linked to: Big Crunch scenario
analyzedUsing Friedmann equations ⓘ
basedOn general relativity ⓘ
canLeadTo Big Bounce in cyclic cosmologies ⓘ
category cosmological end-of-time hypotheses ⓘ
theoretical physics concepts ⓘ
contrastsWith Big Freeze scenario ⓘ
Big Rip scenario ⓘ
Heat Death of the universe ⓘ
dependsOn cosmological parameters ⓘ
dark energy density ⓘ
dark matter density ⓘ
mean matter density ⓘ
total energy density of the universe ⓘ
describes possible fate of the universe ⓘ
discussedIn cosmology textbooks ⓘ
disfavoredBy current measurements of dark energy equation of state ⓘ
evidence for accelerated cosmic expansion ⓘ
observations of distant Type Ia supernovae ⓘ
hasKeyConcept closed universe geometry ⓘ
critical density of the universe ⓘ
gravitational deceleration of expansion ⓘ
historicallyProposedBy early 20th-century cosmologists ⓘ
implies cosmic microwave background temperature would increase in final phase ⓘ
cosmic scale factor reaches a maximum then contracts ⓘ
eventual destruction of large-scale cosmic structures ⓘ
extreme curvature of spacetime at final stage ⓘ
galaxies would move closer together over time in contraction phase ⓘ
scale factor of the universe eventually decreases to zero ⓘ
involves end of spacetime as currently known ⓘ
gravitational collapse of the universe ⓘ
reversal of cosmic expansion ⓘ
universe contracting to high density ⓘ
universe contracting to high temperature ⓘ
relatedTo Big Bounce hypothesis ⓘ
Friedmann–Lemaître–Robertson–Walker cosmologies ⓘ
cyclic universe models ⓘ
requires gravitational attraction to overcome expansion ⓘ
universe to be closed or sufficiently dense ⓘ
status disfavored by current observations ⓘ
speculative ⓘ
studiedIn physical cosmology ⓘ
timeScale would occur in the far future if realized ⓘ
timeSymmetryWith Big Bang in some models ⓘ

How these facts were elicited

Referenced by (4)

Full triples — surface form annotated when it differs from this entity's canonical label.

The Collapsing Universe → discusses → Big Crunch scenario ⓘ
The Origin and Fate of the Universe → mainTopic → Big Crunch ⓘ
linked to: Big Crunch scenario
Big Crunch scenario → alsoKnownAs → Big Crunch ⓘ
linked to: Big Crunch scenario
Tau Zero → featuresConcept → Big Crunch ⓘ
linked to: Big Crunch scenario