In real-time hybrid model testing, complex ocean structures are emulated by fusing numerical modelling with traditional hydrodynamic testing. This is done partitioning the structure under consideration into a and physical substructure, coupled in real time via measurement control interface. The numerically computed load vector applied to substructure means of multiple actuated winches so that r...

High resolution dark matter only simulations provide a realistic and fully general means to study the theoretical predictions of cosmological structure formation models for gravitational lensing. Due to the finite number of particles, the density field only becomes smooth on scales beyond a few times the local mean interparticle separation. This introduces noise on the gravitational lensing pro...

The Cold Dark Matter (CDM) model for galaxy formation predicts that a significant fraction of mass in the dark matter haloes that surround L ∼ L∗ galaxies is bound in substructures of mass 104–107M⊙. The number of observable baryonic substructures (such as dwarf galaxies and globular clusters) falls short of these predictions by at least an order of magnitude. We present a method for searching ...

aims: the aim of the present work is (1) to evaluate dose calculation accuracy of two commonly used algorithms for 15 mv small photon fields in a medium encompassing heterogeneity and (2) compare these results with measured results obtained using gafchromic film ebt2. materials and methods: authors employed kailwood (pinus wallichiana) to mimic lung. briefly, seven kailwood plates, each measuri...

We perform three dimensional hydrodynamical simulations of a moving substructure in a cluster of galaxies. We investigate dynamical evolution of the intracluster medium (ICM) in and around the substructure moving radially in the larger cluster’s gravitational potential, and its observational consequences. After the substructure passes the larger cluster’s center, a bow shock and clear contact d...