Journey Through the Universe with Dr. Ata's ‘Time Machine': From Protoclusters to Superclusters episode artwork

EPISODE · Jun 20, 2022 · 2H 19M

Journey Through the Universe with Dr. Ata's ‘Time Machine': From Protoclusters to Superclusters

from Science Society

In this insightful episode, we venture into the universe's depths with Dr. Sedat Ata, exploring the complex structure and evolution of our cosmos. We discuss the vital role of cosmological simulations in studying the universe and how these simulations can align with real observed structures.Dr. Ata introduces us to a novel approach in cosmic exploration - constrained cosmological simulations. These are specifically designed to match the observed distribution of galaxies, enabling scientists to 'fast-forward' the simulation to our present day and study the evolution of cosmic structures in a self-consistent way.Based on spectroscopic surveys at a redshift of z ≈ 2.3, approximately 11 Gyr ago, these simulations predict that several protoclusters observed earlier would evolve into massive galaxy clusters today. One such prediction includes the 'Hyperion' structure, which will collapse into a filamentary supercluster spanning 100 Mpc.Moreover, the constrained simulations reveal previously unknown protoclusters with lower final masses, nearly doubling the number of known protoclusters within this volume. The approach Dr. Ata presents, when applied to future high-redshift datasets, offers a unique opportunity to study early structure formation and match galaxy properties between high and low redshifts.Tune in as we journey through time and space, understanding the universe's past, present, and future, and learn about the fascinating structures it houses.Keywords: Dr. Sedat Ata, Cosmological Simulations, Constrained Cosmological Simulations, Universe Structure, Protoclusters, Superclusters, Galaxy Clusters, High-redshift Datasets.Ata, M., Lee, KG., Vecchia, C.D. et al. Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations. Nat Astron (2022). https://doi.org/10.1038/s41550-022-01693-0

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