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Theoretical models and numerical simulations have been developed in order to capture the complexity of this interaction and to understand when, where, and how feedback takes place. At the same time the ICM is an important diagnostic of the dynamics of the cluster itself, and an exhaustive understanding of its properties is crucial for a full understanding of the growth of cosmic structures at large, and the measurement of cosmological parameters. This workshop will focus on the physics of the ICM and its relation with the different mass components of galaxy clusters. The aim is to provide an overview of the many exciting recent results at vastly different wavelengths (Radio, SZ, sub-mm, IR, optical, X-ray, gamma-ray) and use them to challenge theoretical models and advanced numerical simulations.
DFT 2017 is dedicated to the memory of Walter Kohn and will be the following in a series of biennial meetings, which took place in Paris (1995), Vienna (1997), Rome (1999), Madrid (2001), Brussels (2003), Geneva (2005), Amsterdam (2007), Lyon (2009), Athens (2011), Durham (2013), and Debrecen (2015).
The aim of these conferences is to bring together researchers from all around the world working on the development of theory, extensions to new fields and providing a broad range of fascinating applications. We organize sessions with oral lectures, invited and contributed, and poster sessions covering versatile topics. As usual the conference covers five subtopics: Time-independent excited state density-functional theory; Time-dependent density-functional theory; Density-functional theory of solids; Strongly correlated systems; Biomolecular modeling and bioreactions.
Last updated: 24 March 2017