Linked from

The 45 pages that link to Expansion of the Universe, each with the reason it gives.

• Dark energyNarrower topic: Dark energy is inferred from the changing rate of this expansion.

• Lambda-CDM modelNarrower topic: Expansion is the evolving quantity described by the model’s background solution.

• Cosmic webNarrower topic: Expansion competes with gravitational collapse as large-scale structure evolves.

• Cosmological redshiftNarrower topic: Cosmological redshift is the wavelength-level effect of this broader expansion.

• Steady-state theoryNarrower topic: It is the process the theory balances with continuous matter creation.

• Recombination (cosmology)Narrower topic: Expansion diluted and cooled the plasma, driving it toward neutral atoms.

• Alexander FriedmannNarrower topic: Friedmann’s solutions showed that expansion could follow from Einstein’s equations.

• Virgo SuperclusterNarrower topic: Expansion limits the Virgo Supercluster’s cohesion and carries its most distant galaxies apart.

• Big RipNarrower topic: The Big Rip is an extreme future outcome of expansion accelerating ever faster.

• Big CrunchNarrower topic: The Big Crunch requires this expansion to halt before collapse begins.

• Cosmic neutrino backgroundNarrower topic: Expansion redshifted relic neutrino momenta and cooled the background.

• Static universeNarrower topic: The discovery of expansion overturned the premise that cosmic scale remains fixed.

• Photon epochNarrower topic: Expansion drives the changing energy densities that define the epoch's boundary.

• Hubble volumeNarrower topic: Expansion determines the time-dependent scale from which the Hubble volume is constructed.

• Timeline of the far futureNarrower topic: Expansion determines whether distant galaxies remain accessible and shapes the universe’s long-term evolution.

• Ultimate fate of the universeNarrower topic: Its rate and acceleration determine whether cosmic distances keep growing or eventually shrink.