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Cosmological simulations: from galaxies to large scales
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LOCATION: Sexten Primary School - Via Panorama 6, Sexten
DETAILS
The field of cosmological hydrodynamical simulations that include a variety of physical processes (e.g. cooling, star formation, energy feedback from various sources, etc.) has seen important advancements in the last years, bringing to a number of important results: realistic simulated disk galaxies, realistic mix of galaxy morphological types, realistic description of multi-wavelength properties of galaxy clusters and of the IGM.
The meeting aims tat bringing together experts working on simulations of cosmic structures – galaxies, clusters and large scale cosmic web – to discuss the state-of-the-art in the field, with particular emphasis on ub-resolution description of relevant astrophysical processes. This will be a small, dedicated workshop of 30-35 participants with half of the working time dedicated to informal discussion and work sessions and half to presentations.
The workshop will focus on the following topics:
– state of the art in simulations of galaxies and galaxy clusters:
– discussion on the different sub-resolution description of star
formation and feedback
– the role of such schemes in predicting observable properties of intergalactic
and circumgalactic medium
RELATED FILES
Scientific Programme with contributions
FEE
To be defined
WORKSHOP CODE FOR PAYMENT
ORGANIZERS
Organizing commettee:
Stefano Borgani
Pierluigi Monaco
Giuseppe Murante