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The 64 pages that link to Dark energy, each with the reason it gives.

• General relativityRelated: In relativistic cosmology, its effects are often represented by a cosmological constant.

• Type Ia supernovaRelated: Supernova distance measurements constrain how dark energy affects cosmic expansion.

• Baryon acoustic oscillationsRelated: Comparing the acoustic ruler across cosmic times constrains dark energy’s influence.

• SupernovaRelated: Distant Type Ia supernovae supplied key evidence for cosmic acceleration.

• Big BangRelated: Its nature determines how the universe’s expansion may develop in the far future.

• GravityRelated: Its gravitational behavior challenges explanations of cosmic expansion.

• CosmologyRelated: Its physical nature remains unknown despite its central role in cosmic fate.

• Hubble tensionRelated: A changed expansion history could reshape constraints on its properties.

• Particle physicsRelated: The Standard Model does not explain the dominant component driving cosmic acceleration.

• Gravitational fieldRelated: Its relation to gravity and the cosmological constant remains a central theoretical problem.

• Hubble's lawRelated: It influences the expansion history behind the measured velocity–distance relation.

• Large-scale structure of the universeRelated: Its influence on expansion changes the late growth of structure.

• Zero-point energyRelated: Its nearly uniform density resembles vacuum energy, but their measured scale is unexpectedly small.

• Galaxy redshift surveyRelated: Distance and clustering measurements from surveys constrain models of cosmic acceleration.

• Luminosity distanceRelated: Distant supernova luminosity distances provided evidence for accelerated expansion.

• Age of the universeRelated: Its nature affects the expansion history used to infer cosmic age.

• Accelerating expansion of the universeRelated: It is the name given to the component linked to the observed acceleration.

• GravitationRelated: Its relation to gravitation and the cosmological constant remains unsettled.

• Hubble flowRelated: Its effects alter the expansion history beyond the simple present-day Hubble flow.

• Wilkinson Microwave Anisotropy ProbeRelated: WMAP’s geometry and matter-density results helped establish the need for a dominant dark-energy component.

• Cosmological parametersRelated: Its density is a central parameter in the standard model’s late-time expansion.

• Heat death of the universeRelated: If its effects persist, accelerated expansion shapes the route toward a cold, dilute future.

• Big CrunchRelated: Its continued influence makes a future turnaround harder in standard models.

• Brian SchmidtRelated: The discovery made dark energy a central problem in cosmology.

• Dark Energy SurveyRelated: DES tested its influence through expansion history and structure growth.

• High-Z Supernova Search TeamRelated: The team’s discovery prompted renewed efforts to explain what drives cosmic acceleration.

• Saul PerlmutterRelated: The supernova result prompted the modern dark-energy problem, though it did not identify the cause.

• Supernova Cosmology ProjectRelated: The project’s distance measurements helped establish the phenomenon later attributed to dark energy.

• Adam RiessRelated: The supernova discovery prompted dark energy to become a central cosmological problem.

• Cyclic modelRelated: Its long-term behavior affects whether expansion can ever reverse into contraction.

• South Pole TelescopeRelated: Cluster counts from the telescope help constrain how cosmic expansion changes over time.

• Theory of everythingRelated: Its physical origin remains unexplained by the Standard Model and general relativity together.

• Universe (cosmology)Related: Its nature remains unknown, yet its effects shape the universe’s expansion history.

• Extragalactic astronomyRelated: Distant galaxies and supernovae help constrain the expansion history it affects.

• Modern physicsRelated: Its physical origin remains unknown despite its importance in cosmology.

• Physical cosmologyRelated: It summarizes a central unresolved component in the standard cosmological model.

• Space scienceRelated: Its cause is uncertain, limiting understanding of the universe's future and large-scale dynamics.

• Chronology of the universeRelated: It dominates the late-time expansion and shapes predictions for cosmic history’s future.

• Expansion of the UniverseRelated: It accounts for the late-time acceleration rather than merely ongoing expansion.

• Observational cosmologyRelated: Its physical nature remains unknown despite measurements of expansion and structure.

• Giant VoidRelated: Accelerated expansion affects how quickly large-scale structure, including voids, evolves.

• Jim PeeblesRelated: Its physical nature remains outside the early-universe mechanisms Peebles’s work established.

• List of unsolved problems in physicsRelated: Its physical nature is not established, though its effects shape cosmic expansion.

• Outline of physical scienceRelated: Its physical nature is unresolved in modern cosmology.

• Outline of physicsRelated: Its physical explanation is absent from the standard inventory of established theories.

• Physics beyond the Standard ModelRelated: Cosmic acceleration is not explained by the Standard Model's particle content.

• Timeline of the far futureRelated: Its unknown nature limits confidence in forecasts of the universe’s ultimate fate.

• Ultimate fate of the universeRelated: Its density and evolution largely decide which long-term expansion scenario is possible.