%0 Generic %1 Vogelsberger2011 %A Vogelsberger, Mark %A Sijacki, Debora %A Keres, Dusan %A Springel, Volker %A Hernquist, Lars %D 2011 %K arepo sph %T Moving mesh cosmology: numerical techniques and global statistics %U http://arxiv.org/abs/1109.1281 %X We present the first hydrodynamical simulations of galaxy formation using the new moving mesh code AREPO and compare the results with equivalent GADGET simulations based on the SPH technique. Both codes use an identical Tree-PM gravity solver and include the same sub-resolution physics for the treatment of star formation, but employ a completely different method to solve the inviscid Euler equations. This allows us to cleanly assess the impact of hydro-solver uncertainties on the results of cosmological studies of galaxy formation. In this paper, we focus on predictions for global baryon statistics, such as the cosmic star formation rate density, after we introduce our simulation suite and numerical methods. Properties of individual galaxies and haloes are examined by Keres et al. (2011), while Sijacki et al. (2011) uses idealised simulations to analyse differences between the hydrodynamical schemes. Global baryon statistics differ significantly between the two simulation approaches. AREPO shows systematically higher star formation rates at late times, lower mean temperatures averaged over the simulation volume, and different gas mass fractions in characteristic phases of the intergalactic medium, in particular a reduced amount of hot gas. These striking differences originate through a higher heating rate with SPH in the outer parts of haloes, caused by viscous dissipation of SPH's inherent sonic velocity noise and SPH's efficient damping of subsonic turbulence injected in the halo infall region, and because of a higher efficiency of gas stripping in AREPO. These differences also produce more disk-like galaxy morphologies in the moving mesh calculations compared to SPH. Our results hence demonstrate that inaccuracies in hydrodynamic solvers can lead to comparatively large systematic differences even at the level of predictions for the global state of baryons. Abridged

@misc{Vogelsberger2011, abstract = { We present the first hydrodynamical simulations of galaxy formation using the new moving mesh code AREPO and compare the results with equivalent GADGET simulations based on the SPH technique. Both codes use an identical Tree-PM gravity solver and include the same sub-resolution physics for the treatment of star formation, but employ a completely different method to solve the inviscid Euler equations. This allows us to cleanly assess the impact of hydro-solver uncertainties on the results of cosmological studies of galaxy formation. In this paper, we focus on predictions for global baryon statistics, such as the cosmic star formation rate density, after we introduce our simulation suite and numerical methods. Properties of individual galaxies and haloes are examined by Keres et al. (2011), while Sijacki et al. (2011) uses idealised simulations to analyse differences between the hydrodynamical schemes. Global baryon statistics differ significantly between the two simulation approaches. AREPO shows systematically higher star formation rates at late times, lower mean temperatures averaged over the simulation volume, and different gas mass fractions in characteristic phases of the intergalactic medium, in particular a reduced amount of hot gas. These striking differences originate through a higher heating rate with SPH in the outer parts of haloes, caused by viscous dissipation of SPH's inherent sonic velocity noise and SPH's efficient damping of subsonic turbulence injected in the halo infall region, and because of a higher efficiency of gas stripping in AREPO. These differences also produce more disk-like galaxy morphologies in the moving mesh calculations compared to SPH. Our results hence demonstrate that inaccuracies in hydrodynamic solvers can lead to comparatively large systematic differences even at the level of predictions for the global state of baryons. [Abridged] }, added-at = {2011-09-08T18:47:13.000+0200}, author = {Vogelsberger, Mark and Sijacki, Debora and Keres, Dusan and Springel, Volker and Hernquist, Lars}, biburl = {https://www.bibsonomy.org/bibtex/298e879ae69c295ac33376f1dda70dc7e/miki}, description = {[1109.1281] Moving mesh cosmology: numerical techniques and global statistics}, interhash = {d1fd926f5dbc2da4364b0850d5a7ba55}, intrahash = {98e879ae69c295ac33376f1dda70dc7e}, keywords = {arepo sph}, note = {cite arxiv:1109.1281 Comment: 30 pages, 25 figures, submitted to MNRAS. Volume-rendering movies and high-resolution images can be found http://www.cfa.harvard.edu/itc/research/movingmeshcosmology}, timestamp = {2011-09-08T18:47:13.000+0200}, title = {Moving mesh cosmology: numerical techniques and global statistics}, url = {http://arxiv.org/abs/1109.1281}, year = 2011 }