SOURCE-LINKED INTELLIGENCE

The key to precise and accurate cosmology: Simulating the physics that shapes gaseous haloes

CORDIS · observation · Publication date unknown

nt for the effects of the multi-phase structure of the gas, of radiation, and of more sophisticated SMBH physics by using new simulation techniques and by complementing the AREPO code with on-the-fly machine learning-based methods. These will enable groundbreaking large-scale simulations, new types of comparisons to observations of both the hot and cold halo gas, and, ultimately, novel and independent analyses of available cosmological data. Cosmological magneto-hydrodynamical simulations; galaxy formation and evolution; groups and clusters of galaxies; feedback from supermassive black holes; gaseous haloes; circumgalactic medium, intra-group and intra-cluster medium; cosmology with groups and clusters; eROSITA.

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recordType

award

status

SIGNED

region

EU

value

1997500

unit

EUR