Description:Inizial conditions for cosmological n-body simulations
Abstract:<b>Experiment:</b>LSSU of Universe Simulations<br><br>
Method of generating initial conditions for N-body simulations that accurately models the real-space statistical properties, such as the mass variance in spheres and the correlation function.
<br>The method requires running ensembles of simulations because the power in the DC mode is no longer assumed to be zero.
Parallelized with MPI2 to obtain huge initial conditions
<BR><BR><B>Software requirements</B>: MPI2<br>fftw-3.2alpha3 library