Results 111 to 120 of about 5,632,379 (394)

Using CFD simulations to investigate the shear stress in hydrodynamic cavitation reactors coupled with experimental validation using colony count measurements [PDF]

, 2022
Máté Polgár, Charu Agarwal, Parag R. Gogate, Gábor Németh, Levente Csóka   +4 more
openalex   +1 more source

Expanding Chemical Space of Nucleic Acid Nanoparticles for Tunable Antiviral‐Like Immunomodulatory Responses and Potent Adjuvant Activity

Advanced Functional Materials, EarlyView.
We introduce a nucleic acid nanoparticle (NANP) platform designed to be rrecognized by the human innate immune system in a regulated manner. By changing chemical composition while maintaining constant architectural parameters, we identify key determinants of immunorecognition enabling the rational design of NANPs with tunable immune activation profiles
Martin Panigaj, Hannah S. Newton, Jian Wang, Laxmi Pandey, Yelixza I. Avilla, Phong Nguyen, Morgan Chandler, Justin Halman, Yasmine Radwan, Stephanie Smith, Elijah Edmondson, Simone Difilippantonio, Chelsea Sanders, Bao Tran, Yongmei Zhao, Shaojun Xie, Edward Cedrone, Barry W. Neun, Meni Wanunu, Nikolay V. Dokholyan, Marina A. Dobrovolskaia, Kirill A. Afonin   +21 more
wiley   +1 more source

The new computer program for three dimensional relativistic hydrodynamical model [PDF]

, 2006
An effective computer program for three dimensional relativistic hydrodynamical model has been developed. It implements a new approach to the early hot phase of relativistic heavy-ion collisions.
Kikola, Daniel, Peryt, Wiktor, Sinyukov, Yuri M., Slodkowski, Marcin, Szuba, Marek   +4 more
core   +1 more source

3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis

, 2007
We investigate the impact of 3D hydrodynamical model atmospheres of red giant stars at different metallicities on the formation of spectral lines of a number of ions and molecules.
Allende Prieto, Allende Prieto, Allende Prieto, Asplund, Asplund, Asplund, Asplund, Asplund, Asplund, Asplund, Asplund, Barbuy, Barklem, Barklem, Beers, Beers, Bessell, Böhm-Vitense, Canuto, Carlsson, Carney, Cayrel, Christlieb, Christlieb, Collet, Conti, Dravins, Dravins, Dravins, Freytag, Fulbright, García Pérez, Gratton, Grevesse, Gustafsson, Gustafsson, Henyey, Hill, Irwin, Iwamoto, Kiselman, Kiselman, Kiselman, Kurucz, Ludwig, M. Asplund, McWilliam, Meynet, Mihalas, Nissen, Nordlund, Nordlund, R. Collet, R. Trampedach, Ruland, Ryan, Sauval, Schwarzschild, Smith, Spite, Spruit, Steffen, Stein, Storey, Uitenbroek, Vögler, Weiss, Yong   +67 more
core   +2 more sources

An Investigation of Intracluster Light Evolution Using Cosmological Hydrodynamical Simulations [PDF]

, 2018
Intracluster light (ICL) in observations is usually identified through the surface brightness limit (SBL) method. In this paper, for the first time we produce mock images of galaxy groups and clusters, using a cosmological hydrodynamical simulation to ...
L. Tang, Weipeng Lin, W. Cui, X. Kang, Yang Wang, E. Contini, Yu Yu   +6 more
semanticscholar   +1 more source

Tailoring the Properties of Functional Materials With N‐Oxides

Advanced Functional Materials, EarlyView.
The properties of materials bearing N‐oxide groups are often dominated by the polar N+─O− bond. It provides hydrophilicity, selective ion‐binding, electric conductivity, or antifouling properties. Many of the underlying mechanisms have only recently been discovered, and the interest in N‐oxide materials is rapidly growing.
Timo Friedrich, Michelle Kobus, Shirin Mesgarha, Erica Moretto, Laurens Grosche, Wolfgang Maison   +5 more
wiley   +1 more source

A new numerical code for hydrodynamical 3D simulations of supernova remnants [PDF]

Serbian Astronomical Journal, 2019
We develop a 3D hydrodynamical code written in C programming language to study the expansion of supernova remnants (SNRs) in the surrounding medium. It is based on the MUSCL-Hancock finite volume scheme with the HLLC Riemann solver.
Kostić P.
doaj   +1 more source

The baryon fraction in hydrodynamical simulations of galaxy clusters

, 2005
We study the baryon mass fraction in a set of hydrodynamical simulations of galaxy clusters performed using the Tree+SPH code GADGET-2. We investigate the dependence of the baryon fraction upon the radiative cooling, star formation, feedback through ...
Borgani, S., Dolag, K., Ettori, S., Murante, G.   +3 more
core   +1 more source

Evolution of N/O ratios in galaxies from cosmological hydrodynamical simulations [PDF]

, 2018
We study the redshift evolution of the gas-phase O/H and N/O abundances, both (i) for individual ISM regions within single spatially-resolved galaxies and (ii) when dealing with average abundances in the whole ISM of many unresolved galaxies. We make use
F. Vincenzo, C. Kobayashi
semanticscholar   +1 more source

Charge‐Induced Morphing Gels for Bioinspired Actuation

Advanced Functional Materials, EarlyView.
This study introduces a novel electroactive actuation mechanism that enables the gel material to generate substantial and reversible shape‐changing while preserving topological and isochoric (volumetric) equivalence. The resultant morphing behaviors can mimic the movements of muscle‐driven organelles in nature, including cilia‐like beating and ...
Ciqun Xu, Saba Firouznia, Charl F. J. Faul, Majid Taghavi, Jonathan Rossiter   +4 more
wiley   +1 more source