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Subgrid-scale modeling of turbulence regulated star formation in simulations of galaxy evolution

Fachliche Zuordnung Astrophysik und Astronomie
Förderung Förderung von 2008 bis 2013
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 48923236
 
Taking advantage of the unique capabilities of the FEARLESS code currently developed in our group, we intend to implement a theory for turbulence regulated star formation recently proposed by Krumholz and McKee (2005) as a subgrid-scale (SGS) model in galaxy simulations. FEARLESS combines SGS modeling of unresolved turbulence with adaptive mesh refinement (AMR) in the cosmological hydrocode ENZO. It provides a local measure for the kinetic energy of unresolved turbulence which is required to calculate the local star formation rate if star formation occurs in virialized, supersonically turbulent gas clouds. We propose to recalibrate the Krumholz-McKee model using data from our own simulations of supersonic turbulence, followed by simulations of a disk galaxy using the calibrated algorithm as a star formation SGS model. These results will be compared with older simulations using phenomenological parameterizations of the star formation rate.
DFG-Verfahren Sachbeihilfen
 
 

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