Linked from

The 28 pages that link to Large-scale structure of the universe, each with the reason it gives.

• Dark matterNarrower topic: Dark matter’s gravity helps explain how small early fluctuations grew into this structure.

• Cosmological principleRelated: Its changing appearance across scales tests where homogeneity becomes a useful approximation.

• Lambda-CDM modelRelated: Cold dark matter predicts how small early fluctuations develop into this cosmic web.

• Cosmic webNarrower topic: The cosmic web is the characteristic network pattern within this broader structure.

• Cosmic varianceNarrower topic: Its observed portion is one realization, limiting comparisons with statistical predictions.

• Gravitational instabilityNarrower topic: It is the largest-scale outcome of gravitational amplification of small initial variations.

• Galaxy redshift surveyNarrower topic: Redshift surveys provide three-dimensional maps of this cosmic network.

• Sloan Digital Sky SurveyRelated: SDSS redshift maps exposed the cosmic web over enormous volumes.

• Galaxy groupNarrower topic: Groups form as dense nodes within this larger distribution.

• Shapley SuperclusterNarrower topic: Shapley is a prominent case for studying how matter gathers into enormous cosmic structures.

• Sloan Great WallNarrower topic: The discovery placed the wall within the emerging map of cosmic structure.

• Euclid (space telescope)Related: Euclid's maps trace this structure and its growth over time.

• Dark Energy SurveyNarrower topic: DES mapped this structure to test how matter clumped over time.

• Cosmic neutrino backgroundRelated: Free-streaming relic neutrinos suppress the growth of structure on small scales.

• Subaru TelescopeNarrower topic: Subaru’s wide surveys chart this structure across extensive areas of sky.

• George SmootRelated: The background’s primordial variations trace density differences that later developed into this structure.

• Zone of AvoidanceNarrower topic: The obscured band once left a major gap in maps of cosmic structure.

• BOSS Great WallNarrower topic: The BOSS Great Wall is one mapped feature within this cosmic pattern.

• Physical cosmologyRelated: Its growth traces how gravity amplified early density differences.

• Structure formationNarrower topic: It is the broadest observable outcome of structure formation.

• Boötes VoidNarrower topic: The void is one low-density feature within this cosmic web of filaments, sheets, and voids.

• Large quasar groupNarrower topic: Large quasar groups are one proposed feature of this broader distribution.

• Primordial fluctuationsRelated: Its clustering provides evidence of how primordial fluctuations grew under gravity.

• IC 342/Maffei GroupNarrower topic: Locating this obscured group helps fill a gap in maps of nearby cosmic structure.

• Jim PeeblesRelated: His work explained how tiny early density variations grew into this structure.

• Pisces–Cetus Supercluster ComplexNarrower topic: The complex is a prominent regional pattern in this broader structure.

• South Pole WallNarrower topic: The wall is one feature in this larger cosmic web.

• Yakov ZeldovichNarrower topic: Zeldovich's gravitational-collapse model became a key framework for explaining this cosmic network.