Results 31 to 40 of about 1,809,603 (303)

Substructures in hydrodynamical cluster simulations

open access: yes, 2009
The abundance and structure of dark matter subhaloes have been analysed extensively in recent studies of dark-matter-only simulations, but comparatively little is known about the impact of baryonic physics on halo substructures.
MURANTE G.   +3 more
core   +1 more source

Full hydrodynamic simulation of GaAs MESFETs [PDF]

open access: yesInternational Journal of Numerical Modelling: Electronic Networks, Devices and Fields, 2004
AbstractA finite difference upwind discretization scheme in two dimensions is presented in detail for the transient simulation of the highly coupled non‐linear partial differential equations of the full hydrodynamic model, providing thereby a practical engineering tool for improved charge carrier transport simulations at high electric fields and ...
Aste, Andreas   +2 more
openaire   +3 more sources

MHD numerical simulations in a cosmological context [PDF]

open access: yes, 2011
Magnetic fields in the Universe are found in almost all studied environments. In particular, their presence in the inter-galactic medium and in the intra-cluster medium is confirmed by diffuse radio emission as well as by observations of Faraday ...
Stasyszyn, Federico Andrés   +1 more
core   +1 more source

Hydrodynamic Simulations of Convection [PDF]

open access: yesInternational Astronomical Union Colloquium, 2002
Convection is one of the most problematic components of almost every model of a pulsating star. RR Lyrae stars, in particular, have a narrow convection zone at the outer layers, and a model without convection cannot get the red edge of the instability strip (see for example Kollath et al., 2000).In recent years, the common approach is to use non-local ...
openaire   +1 more source

Hydrodynamical simulations of molecular dynamics in supersonic turbulent flow

open access: yes, 2004
Here we present results from simulations of turbulence in starforming environments obtained by coupling three-dimensional hydrodynamical models with appropriate chemical processes. We investigate regimes of decaying high-speed molecular turbulence.
Pavlovski, G.   +3 more
core   +1 more source

The VHL tumor suppressor at the crossroad of protein folding, aggregation, and cancer

open access: yesMolecular Oncology, EarlyView.
Mutations, environmental stress, and chaperone dysfunction can destabilize pVHL, promoting its conversion from the native folded state into amyloid‐like assemblies. This transition may contribute to protein storage, cell dormancy, survival, and drug resistance.
Lara Abad   +2 more
wiley   +1 more source

Hydrodynamic and magnetohydrodynamic simulations of wire turbulence [PDF]

open access: yesHigh Energy Density Physics, 2019
We report on simulations of laboratory experiments in which magnetized supersonic flows are driven through a wire mesh. The goal of the study was to investigate the ability of such a configuration to generate supersonic, MHD turbulence. We first report on the morphological structures that develop in both magnetized and non-magnetized cases.
Fogerty, E   +4 more
openaire   +3 more sources

Constructing stable 3D hydrodynamical models of giant stars

open access: yes, 2017
Hydrodynamical simulations of stellar interactions require stable models of stars as initial conditions. Such initial models, however, are difficult to construct for giant stars because of the wide range in spatial scales of the hydrostatic equilibrium ...
Friedrich K. Röpke   +3 more
core   +1 more source

Reprogramming tumor cells with LCOR mRNA nanotherapy to enhance immunotherapy

open access: yesMolecular Oncology, EarlyView.
LCOR (Ligand‐dependent corepressor) mRNA encapsulated in polymeric nanoparticles restores LCOR activity in tumor cells, constraining aggressive tumor cell states and increasing tumor immunogenicity. This reprogramming makes tumor cells more vulnerable to T‐cell attack and enhances their response to immune‐checkpoint immunotherapy.
Gabriel Serra‐Mir   +9 more
wiley   +1 more source

Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact

open access: yesThe Astrophysical Journal
The 98° obliquity of Uranus is widely attributed to a giant impact that ejected material and formed a debris disk, which subsequently coalesced into its regular satellites.
Keiya Murashima, Takanori Sasaki
doaj   +1 more source

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