A model for turbulent combustion simulation of large scale hydrogen explosions

Numerical simulations accounting for the gravitational evolution of billions of dark matter particles confirm that the cold dark matter model is consistent, at least on large

In the more widely used large scale shell model (LSSM) with a core, shell model with configuration mixing in large valence spaces (SM-CI) [1,2], a valence space consisting of one or

8 Future Work 111 8.1 Scheduling Task-Based Programs Using Execution Time Predictability 111 8.2 Sampled Simulation of Task-Based

In this thesis we have presented several modelling techniques that can improve the cur- rent state-of-art of statistical cosmology: an improved halo modelling, a more realistic

The ground-state band in 32 Mg, in particular the observed change in moment of inertia between the ground state and 6 + state, is well reproduced by large-scale shell-

One of the dominant uncertainties affecting recon- structed physics objects is the jet energy scale (JES) uncertainty, especially for large-radius jets [60,66], which has an effect

As a means to probe the possible fractal structure of the galaxy distribution we have studied the scaling of the num- ber density and angular correlation function of galaxies

The proposed model was applied to predict the transient evolution of lab-scale turbulent combustion sequences of mixtures of hydrogen, air and graphite particles under low