N-body Simulations on a Massively Parallel Computer

N-body simulations on the numerical determination of the dissolution times of open star clusters in the Galactic tidal field.

N-body simulations using customised potential-density pair basis sets

N-body simulations using customized potential-density pair basis sets

N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function

N-body simulations with generic non-Gaussian initial conditions II: Halo bias

N-body Simulations with Live Stellar Evolution

N-Body Simulations with Multiple Co-moving Spherical Polar Grids

N-body simulations with perturbation particles - II. Dynamical friction at a distance

N-body simulations with two-orders-of-magnitude higher performance using wavelets

N-Body Studies of the Clustering of Galaxies

N-body/SPH study of the evolution of dwarf galaxies in a cluster environment

N-bursty emission from Uranus: A cyclotron maser source?

n-Capture Elemental Abundances in Active and Non-Active Stars

n-DBI gravity

N-dimensional Bianchi type-I universe in creation-field cosmology

n-Dimensional FLRW Quantum Cosmology

N-dimensional geometries and Einstein equations from systems of PDE's

N-dimensional gravitational collapse of Type I matter fields with non-zero radial pressure

n-Dimensional Gravity: Little Black Holes, Dark Matter, and Ball Lightning