Hydrosim meeting

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Sessions*

Discussion session: Code status and development

Discussion Session: Sub-resolution physical modules

Galaxy Clusters

Code development

AGN

Break

General discussion

Non-standard models

Galaxies

Cosmological simulations

Discussion session: Implementations of non-standard cosmological models and/or non-standard Dark Matter physics

Discussion session: New HPC opportunities

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Contributions*

About the impact of baryons on the cluster mass function: Fitting formula and cosmological implications (in session "Galaxy Clusters")

An improved hydrodynamical scheme as the core of a new production code (in session "Code development")

Angular momentum in galactic halos (in session "Galaxies")

Anisotropic thermal conduction in galaxy clusters (in session "Galaxy Clusters")

Chaotic cold accretion onto SMBHs: the role of rotation (in session "AGN")

CLUES toward the formation of the Local Universe (in session "Cosmological simulations")

Comparison of old and new AGN and hydro schemes in the Dianoga cluster set: flash update (in session "Discussion Session: Sub-resolution physical modules")

Connection between AGN and their host galaxies (in session "AGN")

Formation of disk galaxies with MUPPI (in session "Galaxies")

Gadget3 Data Structures and Tree Walk: standard version vs. modifications (in session "Code development")

Gas angular momentum and BH accretion: flash update (in session "Discussion Session: Sub-resolution physical modules")

Magneticum: To big to fail (in session "Cosmological simulations")

MUPPI: current development: flash update (in session "Discussion Session: Sub-resolution physical modules")

MUPPI: new hydro scheme and AGN (in session "Discussion Session: Sub-resolution physical modules")

Music and Music-AGN clusters (in session "Galaxy Clusters")

New degrees of freedom in the Dark Sector: fifth forces, momentum exchange and dark energy clustering (in session "Non-standard models")

Pressure of the hot gas in simulations of galaxy clusters (in session "Galaxy Clusters")

Pseudo phase space density with Dianoga (in session "Galaxy Clusters")

Radio-mode AGN activity via kinetic feedback in galaxy clusters (in session "AGN")

Realistic distributions of HI without running expensive radiative transfer post-processing codes (in session "Cosmological simulations")

Simulating primordial structures (in session "Cosmological simulations")

SZ scaling relations in Dianoga simulations (in session "Galaxy Clusters")

Temperature Structure and high-z clusters (in session "Galaxy Clusters")

The importance of HPC for high precision, direct N-Body simulations (in session "Discussion session: New HPC opportunities")

The mass accretion rate of galaxy clusters: a measurable quantity (in session "Galaxy Clusters")

The nIFTy comparison project (in session "Galaxy Clusters")

Towards next generations of HPC systems (in session "Discussion session: New HPC opportunities")

Towards porting the GADGET code to the MIC architecture (in session "Discussion session: New HPC opportunities")

Welcome and scope of the meeting

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Events scheduled on*

02/02/2015

03/02/2015

04/02/2015

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