text:   intracluster medium",6,"['New paper is out: <LINK>\n\nWe test particle methods (traditional SPH, pressure SPH), hybrid methods (meshless finite mass) and grid (AMR) in an idealised yet realistic cluster setup. <LINK>', 'We inject hot bubble and study how it buoyantly rises in the environment without and with turbulence. If Kelvin-Helmholtz instability is well captured, then it is disrupted as expected. Energy is then deposited as kinetic energy. SPH variants do it v. poorly https://t.co/qSNcsAWcGy', 'As soon as the paper is accepted we intend to make the initial conditions fully public and encourage others to try their favourite code in this setup, which we hope to become a standard, 3D, astrophysical test for hydro codes.', '@franco_vazza It is of order of what is feasible for these masses of clusters. Here RAMSES max res is about 1.5 kpc, Rhapsody-G had about 2 kpc.', '@franco_vazza For full cosmo boxes… I think only Illustris TNG comes close', '@CosmoCa3sar @franco_vazza Yup. I was thinking more of a spatial resolution (we compared mostly to Illustris TNG)']",18,02,1014