Retrieving "Large Scale Structure Of The Universe" from the archives
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Cold Dark Matter (cdm)
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CDM and Structure Formation Simulations
Numerical simulations, such as the Millennium Simulation, require CDM) to accurately reproduce the observed large-scale structure of the universe, including the cosmic web, voids, and the hierarchical clustering of galaxies. These simulations demonstrate that CDM) naturally leads to a bottom-up formation scenario, where small halos form first and merge hierar… -
Cosmic Microwave Background
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Anisotropies and Structure Formation
While the CMB is extremely uniform, precision measurements reveal minute temperature fluctuations, known as anisotropies, on the order of one part in $10^5$. These fluctuations represent the density variations in the early plasma that acted as seeds for all subsequent large-scale structure, including galaxies and clusters.
Major satellite missions have mapped these anisotropies: -
European Space Agency
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Astrophysics
The history of cosmology within ESA/) is largely defined by the multi-decade success of the Planck mission, which mapped the Cosmic Microwave Background (CMB)/) with unprecedented fidelity. More recently, the Euclid space telescope has been tasked with mapping the large-scale structure of the universe to constrain models of [dark energy](/entries/dark-energ…